Flow cytometry is a technique of great importance in modern biology and medicine and it is finding increasing use in oncology, pathology, haematology, immunology and cell biology. This book describes the fundamental principles behind flow cytometry, the basic methods involved, and the results that can be obtained from this important technique. The various ways that flow cytometry can be used in both medicine and biology are fully described and a particularly detailed account is given of how artefactual results can arise and where 'noise' is generated. Anyone wishing to start using, or already using this technique will need to read this book.
Introduction to flow cytometry
. . . it is not the imagination of man that improves but his capacity to measure which increases... Alfred North Whitehead
Introduction to flow cytometry James V. Watson Clinical Oncology Unit, Medical Research Council, and Faculty of Clinical Medicine, The Medical School, University of Cambridge
The right of the University of Cambridge to print and sell all manner of books was granted by Henry VIII in 1534. The University has printed and published continuously since 1584.
CAMBRIDGE UNIVERSITY PRESS Cambridge New York
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PUBLISHED BY THE PRESS SYNDICATE OF THE UNIVERSITY OF CAMBRIDGE The Pitt Building, Trumpington Street, Cambridge, United Kingdom CAMBRIDGE UNIVERSITY PRESS The Edinburgh Building, Cambridge CB2 2RU, UK 40 West 20th Street, New York NY 10011-4211, USA 477 Williamstown Road, Port Melbourne, VIC 3207, Australia Ruiz de Alarcon 13, 28014 Madrid, Spain Dock House, The Waterfront, Cape Town 8001, South Africa http://www.cambridge.org © Cambridge University Press 1991 This book is in copyright. Subject to statutory exception and to the provisions of relevant collective licensing agreements, no reproduction of any part may take place without the written permission of Cambridge University Press. First published 1991 First paperback edition 2004 A catalogue record for this book is available from the British Library Library of Congress cataloguing in publication data Watson, James V Introduction to flow cytometry / James V Watson. p. cm. Includes bibliographical references and index. ISBN 0 521 38061 8 (hardback) 1. Flow cytometry. 2. Flow cytometry—Diagnostic use. 3. Cancer—Diagnosis. I. Title. QH585.5.F56W38 1991 574.87'028-dc20 90-45686 CIP ISBN 0 521 38061 8 hardback ISBN 0 521 61199 7 paperback
This book is dedicated to the memory of my father, James Robert XVI (2 April 1908 -27 August 1990) who, for as long as I can remember, taught me to think and to appreciate the importance of quantitation.
Contents
Acknowledgements 1 2
xv
Introduction
1
Fluid flow dynamics
5
2.1 2.2 2.3 2.4 2.5
Bernoulli and Euler Reynolds and laminar Hydrodynamic focussing Crosland-Taylor flow cell Flow rates and Poisson statistics
3 3.1 3.2 3.3
Light and optics Snell's Law Refractive index Focussing 3.3.1 Single beam 3.3.2 Multiple beams Interference and diffraction Optical filtration 3.5.1 Absorption filters 3.5.2 Neutral density filters 3.5.3 Interference filters 3.5A Band-pass filters 3.5.5 Dichroic mirrors 3.5.6 Dichroic combinations Light collection Flow chamber design 3.7.1 Cuvette 3.7.2 Jet-in-air 3.7.3 Modified cuvette 3.7.4 Spherico-ellipsoidal Fluorescence 3.8.1 Absorption and emission spectra 3.8.2 Fluorochromes 3.8.3 Fluorochrome combinations 3.8.4 Quenching and resonance energy transfer Excitation 3.9.1 Source size 3.9.2 Source brightness
3.4 3.5
3.6 3.7
3.S
3.9
flow
5 6 8 10 12 18 18 20 22 25 26 31 34 34 35 36 37 37 38 39 41 41 43 44 45 47 49 50 51 54 54 54 55
CONTENTS
3.10
4 4.1
4.2
4.3 4.4
5 5.1 5.2
5.3
5.4
6 6.1 6.2 6.3 6.4 6.5
3.9.3 Conventional sources 3.9 A Lasers 3.9.5 Beam and focussing geometry 3.9.6 Pulse shape Scattered light 3.10.1 Diffraction 3.10.2 Reflection and refraction 3.10.3 Anomalous diffraction 3.10.4 Rayleigh scattering
$& 57 53 60 61 ^2 ^2 62 ^2
Electronics Photodetectors 4.1.1 Photomultipliers 4.1.2 Solid-state devices Signal processing and amplification 4.2.1 Linear amplifiers 4.2.2 Log amplifiers 4.2.3 Differential amplifiers 4.2.4 Triggering and thresholds 4.2.5 Sequential illumination triggering Analogue-to-digital conversion Data capture 4.4.1 Buffering 4.4.2 Dedicated memory 4.4.3 List-mode
65 65 65 66 66 66 66 68 70 71 72 73 73 73 73
Computing Bits, bytes and binary Data processing 5.2.1 Data arrays 5.2.2 Multi-parameter data Data display 5.3.1 Mono-dimensional histograms 5.3.2 Bivariate data 5.3.3 Trivariate data 5.3.4 Multi-parameter data 5.3.5 Bit-mapping Data analysis 5.4.1 Counting within gates 5.4.2 Distribution assessment 5.4.3 Deconvolution of distributions 5.4.4 Distribution shape analysis 5.4.5 Background compensation
74 74 76 76 76 80 81 81 84 85 87 91 92 94 96 97 100
Appendix to Chapter 5
102
Cell sorting Ink-jet writing Electrostatic sorting Cell sorting times Sorting purity and yield Sorting efficiency
106 106 107 110 110 115
CONTENTS 7 7.1
7.2
73
7.4 7.5 8 8.1
8.2
83
8.4
9 9.1
9.2 9.3
9.4
xi
Preparation and staining Disaggregation 7.1.1 Mechanical 7.1.2 Enzymatic 7.1.3 Wax embedded material Permeabilization 7.2.1 Fixation 7.2.2 Hypotonic lysis 7.23 Detergent 7.2.4 Freeze-thaw 7.2.5 Lysolecithin Staining 7.3.1 Surface antigens 7.3.2 Antibody combination staining 733 Fluorochrome amplification 7.3.4 Intracellular antigens 73.5 Interactive stains 73.6 Non-interactive stains 73.7 Stoichiometry DNA denaturation Filtering
117 117 117 118 120 122 122 123 123 124 125 125 126 127 129 131 132 133 134 135 136
Miscellaneous techniques Slit-scanning 8.1.1 Object plane slit-scanning 8.1.2 Image plane slit-scanning Multi-angle light scatter 8.2.1 Sweep-scanning 8.2.2 Multi-detector Rare-event analysis 8.3.1 Statistics 8.3.2 Discrimination Fluorescence spectrum analysis 8.4.1 pH 8.4.2 Calcium 8.4.3 DNA
137 137 137 140 141 142 142 143 143 144 145 146 147 148
Instrument performance Noise 9.1.1 Electronic 9.1.2 Mechanical 9.1.3 Fluidic 9.1.4 Stray light 9.1.5 Light sources 9.1.6 Preparative 9.1.7 Biological Calibration Measurement range 9.3.1 Log amplifiers 9.3.2 Neutral density 9.3.3 Variable gain Coefficient of variation
150 150 151 154 154 155 156 157 158 158 159 159 160 160 165
filters
CONTENTS 9.5
9.6 9.7
9.8
9.9
Sensitivity 9.5.1 Exposure time 9.5.2 Excitation intensity 9.5.3 Bleaching 9.5.4 Light collection efficiency 9.5.5 Optical 9.5.6 Fluorochrome amplification 9.5.7 Sensitivity measurement Resolution and discrimination Precision 9.7.1 ADC offset 9.7.2 Non-linear response 9.7.3 Coincidence Quality control 9.8.1 Inspection 9.8.2 Coincidence correction 9.8.3 Pulse shape analysis 9.8.4 Time Instrument hygiene
filtration
166 166 166 167 167 167 169 169 170 172 173 174 176 176 177 177 179 182 184
10 10.1 10.2 10.3 10.4
Light scatter applications Forward scatter Dual-angle scatter Viability determination Multi-angle scatter
186 186 191 194 198
11 11.1
Nucleic acid analysis Nucleic acid stains 11.1.1 DNA specific 11.1.2 Nucleic acid specific 11.1.3 Non-specific poly-anion stains 11.1.4 RNA 'part-specific' The cell cycle The DNA histogram DNA histogram analysis 11.4.1 Age distribution theory 11.4.2 Rectilinear integration 11.4.3 Multiple Gaussian 11.4.4 Polynomial 11.4.5 Single Gaussian 11.4.6 TCW analysis Cell cycle kinetics 11.5.1 Stathmokinetic techniques 11.5.2 Mitotic selection 11.5.3 Modelling population kinetics 11.5.4 FPI analysis 11.5.5 Bromodeoxyuridine 11.5.6 Biotinolated nucleotides 'Ploidy' 11.6.1 Stoichiometry 11.6.2 Binding site modulation
201 201 201 203 204 206 207 208 211 211 213 214 215 216 223 223 224 225 228 233 235 241 242 243 243
11.2 11.3 11.4
11.5
11.6
11.7
11.8 12 12.1 12.2 12.3
12.4
13 13.1 13.2
13.3
13.4
13.5
13.6 13.7
14 14.1
CONTENTS
xiii
11.6.3 Standards 11.6.4 Logistics RNA and DNA 11.7.1 Acridine orange 11.7.2 Hoechst/pyronin-Y Emission spectrum analysis
244 246 246 247 256 259
Nucleic acids and protein Viable cells Non-viable cells Nuclear-associated antigens 12.3.1 Quantitation with antibodies 12.3.2 Turnover measurements 12.3.3 Cell cycle modulation 12.3A Dual antigens plus DNA Cytoplasmic antigens 12.4.1 Immunoglobulin 12.4.2 Cytoskeleton
266 266 268 268 269 273 273 282 283 283 285
Chromosomes Harvesting mitotic cells Chromosome preparation 13.2.1 Hexylene glycol 13.2.2 Polyamine 13.2.3 Hypotonic PI detergent 13.2.4 Ohnuki buffer 13.2.5 Magnesium sulphate Staining 13.3.1 Total DNA 13.3.2 A—T:G—C composition 13.3.3 Bromodeoxyuridine 13.3A Partial sequence specificity 13.3.5 Chromosome-associated proteins 13.3.6 In situ hybridization Flow karyotype analysis 13.4.1 Univariate 13.4.2 Bivariate Slit-scanning 13.5.1 Centromeric indices 13.5.2 Banding High-speed sorting Applications 13.7.1 Diagnosis 13.7.2 Genomic libraries 13.7.3 Gene mapping 13.7A Radiation bio-dosimetry Dynamic cellular events Incorporation of time 14.1.1 Discontinuous sequential sampling 14.1.2 Continuous interrupted sampling
288 288 290 290 290 291 291 291 292 292 293 293 297 297 299 299 299 300 301 301 302 303 303 303 304 305 308 309 310 310 310
/
CONTENTS
14.2
14.3 14.4 14.5 14.6 14.7 15 15.1
15.2
15.3
15A 16
14.1.3 Continuous time recording 14.1.4 'Stop—flow' cytometry in Enzyme kinetics 14.2.1 Substrates 14.2.2 Light absorption quantitation 14.2.3 Fluorescence quantitation 14.2.4 Cytoplasmic enzymes 14.2.5 Membrane enzymes 14.2.6 Dual substrate analysis 14.2.7 Inhibition kinetics 14.2.8 Short time scale kinetics Membrane potential Calcium Mitochondrial function Drug transport Concluding remarks
flow
311 312 317 317 319 320 320 328 330 332 333 335 336 339 339 343
Applications in oncology Diagnosis 15.1.1 Leukocyte classification 15.1.2 Cytological prescreening Prognosis 15.2.1 DNA index 15.2.2 Oncogenes Therapy selection 15.3.1 GSH metabolism 15.3.2 Drug resistance 15.3.3 Tumour growth rate Future prospects
345 348 349 349 351 351 356 366 367 368 380 384
Epilogue
385
References
387
Index
431
Acknowledgements
I thank all those who either knowlingly or unknowingly contributed to this book. The latter includes my friends and colleagues overseas, Joe Gray, Jim Jett, Scott Cram, Jan Visser, John Martin, John Steinkamp, Gary Salzman, Harry Crissman, Tudor Buican, Zbignew Darzynkeiwicz, Harald Steen, Gunter Valet, Alex Nakeff, Leon Wheeless, Jim Leary, David Hedley and Wolfgang Eisert with whom I have discussed many aspects of flow cytometry over a number of years. I also thank the various authors, as well as those mentioned above, whose work I have cited and whose data I have used as illustrations. Those who knowingly contributed include my friends and immediate colleagues in Cambridge who helped with both the construction and developmental use of the dual laser multi-parameter system in the MRC Clinical Oncology Unit. My thanks are extended to Norman Bleehen who asked me to take responsibility for the flow cytometry in our Unit in 1975. I'm still not sure, even after 15 years, if he thinks he made the correct decision. I particularly thank the successive directors of the MRC Laboratory of Molecular Biology in Cambridge, Max Perutz, Sidney Brenner and Aaron Klug who, without asking any questions, allowed me to 'run riot' in the mechanical engineering and electronics workshop which enabled me to build the 'big gun'. Every member of the mechanical workshop, including Dave Hart, Mick Bitten, Chris Raeburn, Terry Baily, Mick Fordham, Steven Stubbings and 'Gonzo' contributed over the years but it was Phil Atkin initially, and Chris Hellon latterly, who constructed the difficult highprecision bits-and-pieces. In the electronics division it was Frank Mallett who did the design work and Mike Thompson the construction and development work. I'd like to take this opportunity to apologize to Mike for giving him ulcers and I promise not to add any more detectors, I agree (a little reluctantly) that nine are enough for one instrument. I thank Steven Chambers and Ian Taylor who helped with the early work on the old Cytofluorograf 4800A and Steven gave invaluable assistance in commissioning the dual laser system in the early 1980s. Particular thanks are extended to the two Pauls, Workman and Smith, who helped to extend the scientific applications far beyond those envisaged in 1978 and 1979 during the design and construction phase of the instrument. I also thank our various Ph.D., M.D. and M.S. students, Caroline Dive, Richard Epstein, John Stewart, Vasi Sunderesan, Peter van Dam,
xvi
ACKNOWLEDGEMENTS
Tim Maughan, Mary Fox and Sally Morgan who have taken advantage of the system and who helped in the software development by pointing out the things it wouldn't do and which needed to be added. I thank Terry Rabbitts, Gerard Evan, Karol Sikora, Julian Blow, Ron Lasky, Jon Karn, Amy Kenter, Mark Walport, Ian Forgacs, Marigold Curling, Chris Hudson, Jo Milner and Bob Johnson for very fruitful collaborations. I thank the librarians of Trinity College, Cambridge, and the Royal Society, London; the former for access to Newton's Library and the latter for access to the 'early' works including the first edition of the Micrographia and the original handwritten Latin manuscript of the Principia. I thank all the staff of Cambridge University Press for their help in preparing this book, particularly the Scientific Editor, Robin Smith, and sub-editor Beverley Lawrence. It was Beverley who painstakingly corrected my spelling and inconsistencies of presentation and checked the reference list. My most heart-felt thanks are reserved till last. Firstly to Terry Horsnell, who runs the computing systems in the Cambridge MRC—LMB, and who has given me such invaluable help and support over many years. Secondly to Hilary Cox who took over from Steve Chambers and who now runs the whole show with complete unflappable calm even when everything is going wrong. All I can say is thanks a million you two, I owe you one! Finally, I thank my wife, Andrea, who is probably a saint as she hasn't divorced me (yet) although she has been a flow cytometry 'widow' for many years, and my four children who have been flow cytometry paternal 'orphans' for as long as they can remember. To them, I promise to go on holiday this year, mend the roof and fix the gutters, put the floor back in the dining room and finish the fire place, replace the carpets (where they exist), mend the stairs and repair the hole in the fence so the rabbit doesn't escape again to eat our neighbour's prize dahlias.
1 Introduction
Classical histological methods of investigating cellular pathology involve characterizing morphological features using light absorbing dyes and fluorescent probes. The first category of stains gives rise to different colours in different subcellular constituents due to differential binding and hence differential absorption of transmitted light. Staining was used increasingly in microscopy after Virchow's work with various pigments including those from blood (Virchow, 1847) and the most extensively used example is the combination of haemotoxylin (introduced by Waldeyer, 1863) and eosin. The former is a basophillic blue dye which binds to nuclear components and the latter is acidophillic which binds to cytoplasmic constituents. Heamotoxylin appears blue to the human eye as it absorbs red light and eosin appears yellow/orange due to blue light absorption. Without the aid of this type of differential stain combination the histopathologist would hardly exist as details of the unstained cell are essentially invisible. Immunoperoxidase staining of specific molecules using monoclonal antibodies (Kohler and Milstein, 1975) is an extension of this type of approach with the deposition of brown/black granules which absorb light of all wavelengths at a site where the antibody binds to its target molecule. This method, of course, is used in conjunction with other stain combinations to identify the site at which the antibody binds. With the orange/blue combination of eosin plus haemotoxylin as a counterstain for the immunoperoxidase we can locate the molecule of interest as being nuclear, cell surface or cytoplasmic. Fluorescent antibody probes, introduced years ago (Coons, Creech and Jones, 1941; Coons and Kaplan, 1950), can also be used in this type of morphological study where different molecules or classes of molecule can be identified by using two different antibodies coupled to different fluorochromes which emit light at different wavelengths. One example is the use of fluorescein and rhodamine which are both excited by blue/green light and which emit fluorescence in the green/yellow and red wavelength bands respectively. Another example using fluorescence is the combination with propidium iodide which stains DNA and fluorescein isothiocyanate which stains proteins. Under the fluorescence microscope the nucleus is red and the cytoplasm is green. It is very difficult to combine fluorescence with absorption staining, which relies on light transmission, due to the different light intensities involved and differential absorption of wavelengths
2
INTRODUCTION
which are necessary for fluorochrome excitation. Fluorescence methods now tend to rely exclusively on epi-excitation techniques. Classical techniques are excellent for qualitative studies but it is very difficult to obtain quantitative information from individual cells by eye using the fluorescence microscope. It is possible to answer the question 'what proportion of the population is labelled with a given probe7 by either immunoperoxidase or fluorescence techniques. However, it is virtually impossible to obtain reliable information about the quantity of that probe in, or on, a given cell except to score this as high, medium or low. Usually, however, all we can do is to give a score of positive or negative. The normal human eye has excellent wavelength discrimination (colour) but an almost total inability to quantitate objectively at a given wavelength. Future developments in pathology and cellular physiology will include the precise quantitation of specific molecules in both normal and abnormal cells. These molecules may differ both qualitatively and quantitatively in diseased cells and with the advent of monoclonal antibody technology and oligonucleotide hybridization (Southern, 1975; Thomas, 1980) we have the capacity to discriminate very precisely between different molecular species at the DNA, RNA and protein levels. There will, however, be many pathological states which are due to quantitative changes of a given molecule or molecules and classical microscope techniques in conjunction with the human eye are not capable of making this type of discrimination reliably. Flow cytometry is an investigational technique which is able to make multiple objective simultaneous measurements at the single cell level at rates of up to 5000 cells per second. The quantitative aspects of the technology take their origins from the work of Caspersson and colleagues in the 1930s where stained images were projected onto a wall and the amount of light absorbed in different areas of the images was quantitated with primitive photodetectors. Nucleic acid metabolism in Drosophila melanogaster salivary gland chromosomes was studied by banding pattern changes using this method (Caspersson and Schultz, 1938). Apart from their analytical capability many instruments have the additional feature of electrostatic cell sorting which places individual cells with predetermined characteristics in a test tube for subsequent morphological identification or biological manipulation. The technology has a number of advantages and disadvantages. The former includes objective quantitation of specific molecules, statistical precision, multi-parametric cross correlated data analysis, distributional information and hence subset identification, dynamic measurements, sensitivity, speed and the generation of a vast amount of data. The disadvantages include loss of 'geographical7 information from solid tissues as a single cell suspension is mandatory, absence of a direct visual record and the generation of vast amounts of data. The last of these is included under both headings as this is a two-edged sword. Data have to be converted to information. There is no merit in being the proud custodian of 40 000 MgBytes of data (the size of our data base on 1 December 1989) if the numbers are random and hence have no meaning. The
INTRODUCTION
3
conversion of data, particularly multi-parameter data, into information is a science in its own right and presents considerable problems. It is pertinent at this point to ask why we should wish to make measurements on an individual cell basis and at such rapid rates. The answers are really quite simple. If we take a sample of tissue, homogenize it and perform a given assay we obtain a grand average for that sample. Let us suppose that the answer is 100 units. However, we do not know if half the cells in the sample have zero units and the other half has 200 units or if all cells have exactly 100 units each. The answer is 100 units for each scenario. Individual cell analysis, by whatever means, is the only method of resolving this problem and hence of obtaining reliable data in heterogeneous populations. That in itself is justification irrespective of the other advantages that flow cytometry offers which importantly includes statistical precision. It is possible to use a fluorescence microscope to determine the proportion of fluorescently labelled cells in a population but the precision of manual counting is highly dependent on the proportion of labelled cells and the number of cells you are prepared to count. If the labelled fraction constitutes only 5% of the population and you count a total of 200 you will, on average, score 10 positive cells. However, due to statistical factors this could be anything between 3 and 17 cells which gives a range of 1.5% to 8.5% at the 95% confidence interval. Hence, the ability to analyse and count large numbers of cells very rapidly has major advantages particularly for analysis of minority subsets. However, the various flow cytometry techniques should not be regarded as being able entirely to replace existing methods, they should be regarded as an adjunct although 'classical' techniques just cannot compete with the speed of flow technology. Moreover, there are some things you can do using flow cytometry that just could not be done in any other way. The technique relies upon measuring both scattered light and fluorescence from suitably stained constituents in individual cells in the population. The stained cells are streamed single file in fluid suspension through the focus of a high-intensity light source. As each cell passes through the focus a flash of scattered and/or fluorescent light is emitted. This is collected by lens systems and filtered before reaching a photodetector which may be either a photomultiplier or a sold-state device. The photodetector quantitatively converts the light flash into an electronic signal which is digitized by an analogue-to-digital converter into a whole number (integer) which is then stored electronically. The first commercial flow system that actually worked was the Coulter counter where impedence changes were measured as cells passed through a narrow capillary orifice (Coulter, 1956). This type of approach was extended in the early 1960s by Kamentsky with measurements of DNA by UV absorption and size by violet light scattering in attempts to automate cervical cytology (Kamentsky, Melamed and Derman, 1965). Kamentsky and Melamed (1967) also adapted their instrument as a fluidic cell sorter but, it was Fulwyler (1965) at Los Alamos who produced the first cell sorter using electrostatically charged droplets, a development of Sweet's invention for ink-jet writing (1965). Volume measurements were
4
INTRODUCTION
able to be made with sufficient precision to sort normal white cells with a very high degree of purity (van Dilla, Fulwyler and Boone, 1967). Fluorescence measurements were introduced by van Dilla, Trujillo, Mullaney and Coulter, by Dittrich and Gohde and by Hulett, Bonner, Barrett and Herzenberg all in 1969. Since then the uses of flow cytometry have been expanding at an alarming rate and during the late 1960s and early 1970s major developments took place in fluorescence activated cell sorting at Stanford University (Hulett et al, 1969; Bonner et a\., 1972; Herzenberg, Sweet and Herzenberg, 1976). At first sight these instruments appear complex but many of the basic principles on which they operate were discovered centuries ago. Because of the fundamental importance in understanding the technology some of these principles of physics will be considered. I am well aware that most biologists tend to cringe at the mention of physics. However, there is nothing in the sections which contain some physics and technology that would cause any difficulty for a reasonable intelligent 16- or 17-year-old studying first-year sixth-form physics for advanced level GCSE examinations. Furthermore, the quantity of physics is strictly limited, with no 'fancy' mathematics, and an attempt has been made to relate the relevant concepts from physics directly to the technology, and the technology to the biology. This book aims to describe the technology and some of its applications and potential applications for students of pathology, medicine and cell biology, laboratory technicians and postgraduates who, hopefully, will have recourse to use the various techniques on a routine basis within the next decade. It is not intended for highly experienced users intimately involved with the technology who should know everything in this book already. The initial intention was a series of notes for users of the instruments in the MRC Clinical Oncology Unit at Cambridge so that I would not have to say the same things over and over again each time a new user wished to take advantage of the systems. The notes got bigger with time and I decided to put them into book form as a general introduction to the subject. To a large extent the book is based on the author's experience of designing, building, developing and working with the Cambridge MRC dual-laser multiparameter instrument in a highly interdisciplinary, varied and stimulating biological environment. A large proportion of the assays and results used as examples are drawn from our data base accumulated over the past 15 years. This does not mean that some of the assays cited as examples are unique to our instrument; they are not, it's just that it was easier to illustrate with what I know best. As a consequence there is a considerable bias towards the interests of our group and collaborators; however, even if you are not interested in what we have been doing the examples serve to illustrate some of the power, potential and problems associated with the technology.
Fluid flow dynamics
The most important essential feature of any flow cytometric instrument is a stable fluid stream which presents the cells one at a time to a sensing volume where the measurements are made. To obtain consistency of measurement each cell has to be presented to the same volume within the sensor and in order to understand how this is achieved we must consider some basic concepts of fluid dynamics.
2.1
Bernoulli and Euler
Bernoulli was a Swiss mathematician who experimented with various aspects of fluid flow dynamics. He constructed a number of pieces of glass apparatus through which he pumped water. One particular apparatus consisted of a tube with a central constriction and he added three manometers along the tube. One was placed at the constriction and the other two were placed one upstream and one downstream in relation to the constriction. This is depicted in figure 2.1. It is perhaps a little surprising at first sight to find that the hydrostatic pressure is reduced in the manometer placed at the constriction and that the pressures are approximately equal in the upstream and downstream manometers. As the velocity must increase in the constricted portion of the tube Bernoulli (1738) concluded that velocity and pressure in fluid flow must be inversely related and he derived the equation to describe this phenomenon. This is a beautiful simultaneous demonstration of two fundamental laws of physics, the law of conservation of energy and the second law of motion (Newton, 1687). The velocity is greater in the constriction, thus water must be accelerated which, from Newton's second law, requires a force. This in turn requires energy which is obtained from the decrease in hydrostatic pressure at the constriction. On exit from the constriction the velocity decreases and the kinetic energy required for the acceleration is reconverted to hydrostatic energy. The total energy in the system is the same at every point but this assumes different forms depending on which part of the system we are looking at. There is a conversion of some of the hydrostatic potential energy in the wider portion of the tube to kinetic energy at the constriction which is manifest by a decrease of 6h in the pressure at the constriction. Incidentally Bernoulli's experiment forms the basis for the whole of aviation. The aerofoil of a wing is so shaped that air has to traverse a greater
FLUID FLOW DYNAMICS
Figure 2.1. Bernoulli's experiment with fluid flow in a constricted tube showing the inverse relationship between velocity and pressure.
distance over the upper surface. This increases its velocity over the upper compared with the lower surface hence, the pressure is decreased over the upper surface giving rise to lift. Somewhat later, Euler (1755,1759) showed that the velocity profile of fluid flow in a tube is parabolic where the velocity is greatest in the center of the tube. This is depicted in figure 2.2. Thus, from Bernoulli's experiment the pressure must be lowest at the center of flow and there is a continuous decrease in pressure as we move from the periphery to the center which means that the pressure profile is longitudinal. If we now introduce a non-compressible particle into the flow towards the periphery there must be a greater pressure on its outer than on its inner aspect and it will tend to be forced towards the center of the stream. This is one of the processes which contribute to coaxial streaming (Goldsmith and Mason, 1961) and is one of the reason why blood cells do not touch the walls of medium and small arteries.
2.2
Reynolds and laminar flow
Coaxial streaming is only stable if flow is laminar and not turbulent. Reynolds (1883) found a relationship which describes fluid flow where Re = vdp/rj. The Reynolds number, Re, is a dimensionless quantity, v is the average velocity, d is the tube diameter, p is the fluid density and f] is the coefficient of viscosity. The critical Reynolds number is 2300, below which non-turbulent laminar flow is maintained and all flow cytometers should be designed to function well below this value, which is directly proportional to both velocity of flow and tube diameter. For any given fluid both p and r\ are constant thus, as fluid flows from a large to a small diameter tube vldl — v2d2, where the subscripts 1 and 2 refer to the large and small tubes respectively. As fluid is not compressible the same volume must pass a given cross section per unit time in both tubes. Let us assume that the velocity in a larger tube with a diameter of 20mm is 1 0 c m s ' 1 which means that a volume of n x 102 X 10 cm3 passes a given cross section each second. The fluid in the larger tube now flows into a smaller tube of 2 mm diameter and the volume passing a given cross section each second will be n x I 2 x vs cm3. The velocity, vs, can now
REYNOLDS AND LAMINAR FLOW
Figure 2.2. The velocity profile is parabolic in laminar flow with the greatest velocity in the center of flow and as a consequence the pressure profile is longitudinal A particle, P, introduced into theflowas shown will have a greater pressure on its outer aspect and the resulting force vector (oblique arrow) will tend to drive the particle towards the center of flow. be obtained from the relationship nxlO2 xlO = nxl2 Xvs which gives v = 103 c m s " 1 (the rest of the maths, where it occurs, is no more complicated than that). Thus, the velocity increases as the square of the ratio of the larger to the smaller diameter but the Reynolds number should not change. However, a number of problems arise. Firstly, v is the average velocity of the parabolic profile with the axial velocity considerably greater than that towards the walls. Secondly, due to the frictional viscous forces there is a boundary layer close to the vessel wall where the velocity is essentially zero. Thirdly, any 'sharp edges' in the vicinity of the transition from the larger to smaller diameter will increase the thickness of the boundary layer. This is illustrated in figure 2.3 with a 'square' junction between large- and small-born tubes. The net flow from left to right in the stippled regions is essentially zero and eddy currents are generated. Turbulence
Figure 2.3. The transition region of a large to a small-bore tube withfluidflow from left to right where the junction is 'square'. The boundary layer which builds up is essentially stationary and turbulence can occur in the thin transition zone between the boundary layer and the laminar flow region.
FLUID FLOW DYNAMICS
B 2.4. Erythrocytes are entering a constriction in flow. In panel A the cells are entering the small-bore tube in the laminar flow region and follow a well defined path. Note the uniform elongation of the cells due to the hydrodynamic forces. In panel B the cells are entering the small-bore tube very much closer to the walls and are caught in the turbulent flow region. Note the disordered flow pattern and random distortion. I thank Dr Volker Kachal for these photographs. occurs at the interface (transition zone) between this region and the laminar flow and is shown in figure 2.4 with erythrocytes entering a constriction in flow. The cells in panel A are within the laminar flow region and are not only uniformly orientated but also elongated. In panel B the cells are entering the constriction very much closer to the tube wall and are flowing in the turbulent transition zone. Note the comparatively disordered flow pattern and the random cellular distortion. Elimination of the 'sharp edges' in figures 23 and 2.4 at the junction of the two tubes with incorporation of a cone approximating to the stippled boundary layer in figure 23 will reduce considerably the chance of generating turbulence.
2.3
Hydrodynamic focussing
We can see from figure 2.3 that the boundary layer effectively decreases the diameter of the laminar flow region in the entrance of the smaller-diameter tube. This increases the velocity above the squared diameter relationship which
HYDRODYNAMIC FOCUSSING
9
increases the probability of turbulence. Moreover, the increase in velocity as fluid flows from the larger- to the smaller-diameter tube commences in the larger tube at some distance before the constriction is encountered. This acceleration starts in approximately the position that the stationary boundary layer begins to build up (see figure 2.3). The net result is illustrated in figure 2.5 where the cross-hatched central core in the larger-diameter tube is squeezed, by virtue of the increased velocity, into the thinner 'thread' flowing in the center of the small-bore tube. If the ratio of the tube diameters is 10:1 then the core shown in the larger tube will be 'compressed' by a factor of 10 when it is flowing in the smaller tube. This is hydrodynamic focussing (Spielman and Goren, 1968;|Kachal and Menke, 1979) which is also capable of orientating cells in flow (Fulwyler, 1977; Kachal, Kordwig and Glossner, 1977). The visible manifestation of hydrodynamic focussing can be seen in every-day life when you pull the plug out of the basin each morning after washing and/or shaving. The latter, of course, presumes that you are male. If you live in the USA and don't use a basin then fill it up anyway and observe the vortex formation as the water runs down the plug hole. I'm not implying that those in the USA belong to the fraternity of the great unwashed but things over there tend to be a little more
Figure 2.5. An illustration of hydrodynamic focussing where the cross-hatched core in the larger tube is 'compressed', by virtue of increasing velocity, into the thinner core in the smaller diameter tube.
10
FLUID FLOW DYNAMICS
advanced and showers and electric razors tend to be used for these two purposes. If the plug has been removed slowly so as not to disturb the body of water in the basin too much the vortex can be seen to pass down through the center of the waste pipe which is a good demonstration of coaxial streaming. The velocity of the vortex can also be examined by injecting small quantities of ink into the water at different positions in the basin with a syringe and needle. You'll find the velocity is greatest at the water/air interface.
2.4
Crosland-Taylor flow cell
Crosland-Taylor (1953) used the principles described above to construct a flow chamber for counting blood cells. This chamber is the fore-runner of all those used in flow cytometry and a representation based on the original is shown in figure 2.6. It consists of a closed cylinder with an inlet port, through which 'sheath' fluid is pumped, and an exit constriction. Cells are introduced into the flow by a needle whose tip is located just above the exit constriction. The combination of hydrodynamic focussing and the coaxial pressure drop causes cells to pass down Sample
Sheath fluid
Coaxial stream
Figure 2.6 The Crosland—Taylor type of flow chamber with hydrodynamic focussing of the sample in the exit nozzle by the sheath flow.
CROSLAND-TAYLOR FLOW CELL
11
Stained cells
ight collecting lens
Pulse processing
Computer storage Figure 2.7. Basic layout of a typical flow cytometer.
the center of flow through the exit nozzle. By suitably adjusting the nozzle size, the constriction cone, flow rates and relative pressures it is possible to constrain one cell at a time to pass through the nozzle. All we need now is a high-intensity light source to elicit fluorescence and light scatter, suitable light collection optics and electronics to quantitate the response from individual cells. A typical layout of a flow cytometer is shown in figure 2.7 where the planes of the cell stream, light illumination and light collection are placed orthogonally (90° between each). Precision in flow cytometry depends on many factors the first of which is accurate and stable positioning of the hydrodynamically focussed cells. Figures 2.6 and 2.5 illustrated the 'compression' of the cell stream into the coaxial center of flow in the exit nozzle, which is termed the core, and precision also depends on the position of cells within the core. For example, if cells of 10 |im in diameter are being analysed and the core diameter is 30 (im then the cells could lie anywhere in the 30 (xm of the core and they may not be equally illuminated by the exciting source (see section 3.9.5). It is important, therefore, to approximate the core diameter to the cell diameter and for 10 (im cells a core diameter of 12 (im to 15 Jim is required. The core diameter is dependent on the ratio of the sheath-to-core volumes entering the flow chamber and these in turn are dependent on the relative input pressures. In practice core diameters are not measured and the instrument is set up so that the pressure on the sample (which makes up the core) is progressively increased until cells just begin to flow through the chamber. This usually requires a pressure between 0.5 and 2.0 psi higher than that on the sheath but this is also dependent on the relative diameters and lengths of the input feed lines which vary between instruments. Increasing the sample pressure still further increases the cell through-put rate but begins to 'degrade' the data which is indicative of too great a core diameter (see section 3.9.5). Thus, the sample pressure should be just sufficient to pump cells into the flow chamber which is the point at which the core diameter is at a minimum. Single sheath systems can attain positional accuracy of the core within + 2 (im
12
FLUID FLOW DYNAMICS
which is adequate for most applications. However, flow chambers incorporating a double sheath (Eisert and Dennenloehr, 1981; Eisert, 1981), which confer greater stability on the axial stream, have been constructed and positional accuracy of + 0.5 Jim can be achieved. This is necessary for some types of assay (e.g. chromosome slit-scanning, see section 8.1 and chapter 13) where extreme positional accuracy is required.
2.5
Flow rates and Poisson statistics
The requirement to minimize the core diameter has implications for cell through-put rates that can be attained in any given instrument. Let us assume we have a 'typical' sample at a concentration of 106 cells ml" * and a core diameter of 10 |im (we must be running red cells or lymphocytes!). The area across the core is nr2 = 78.5 |im 2 which we will approximate to 80 |im 2. If the total sample is 1.0 ml the 'potential7 core length will be 12 500 meters of about 40 000 feet which is 7.6 miles (10 ml of sample would stretch from here to Oxford, wherever that is, or into low Earth orbit). Astonishing as it may seem this is correct. 1.0 ml = 1 cm X 1 cm X 1 cm = 1 cm3. Each centimeter contains 10 x 1000 jam, thus 1.0 ml = 10 x 1000 x 10 x 1000 X 10 x 1000 = 1012 um3. Dividing 1012 |im3 by the core area, 80 |im2, gives 1.25 X 1010 |im and dividing this by 106 (the number of microns in 1 meter) gives 1.25 x 104 = 12 500 meters. I've written it out like this mainly for my own benefit as I'm a physician and biologist! Now, if we have 10 6 cells in the sample of 1.0 ml which are stretched out over a distance of 12 500 meters then, on average, the cells will be spaced at intervals of 12 500 x 100/10 6 cm (1.0 meter = 100 cm) = 1.25 cm in the core. This is actually 1.27 cm if we don't make the SO |Lim2 approximation for the cross section area of the core. Figure 2.8 plots the average distance between cells in the core versus selected core diameters between 10 |Lim and 30 |Lim for sample concentrations of 106 and 5 x 106 cells ml ~ *. We can now convert the data in figure 2.8 to the number of cells per second which pass a fixed point, the count rate. The core velocity varies from cytometer to cytometer but this is usually between 2 m " 1 and 10 m s~ 1 . Thus, dividing these velocities by the distances between cells in a 10 |im core gives the count rates for 106 cells ml" 1 which are 157 and 785 cells s" 1 for velocities of 2 m s " 1 and 1 0 m s " 1 respectively. Figure 2.9 shows the count rates versus core diameter for these two flow rates with a cell concentration of 10 6 ml" 1 . If we are working with a concentration of 106 cells ml" 1 in a low flow rate, 2 m s " 1 , instrument (which has some advantages, see section 9.5.1) and we want to analyse cells faster than 157 hertz (1 hertz is 1 cycle per second) we have two options. Firstly, the sample pressure can be increased to increase the cell throughput. This increases the core diameter, and to raise the count rate by a factor of five (from 157 hertz to 785 hertz) we would increase the core diameter from 10 |im to 22 |im (see figure 2.9). This in turn decreases the measurement precision because not all cells may be equally illuminated (see section 3.9.5), and this is not generally
FLOW RATES AND POISSON STATISTICS
13
1.2 -
1.0 -
E o 0.8
0)
3 0
0.6
o c 0)
2
0.4
0.2 -
—I—
10
—I— 15
20
—I—
25
30
Core diameter, /im Figure 2.8. Average distance between cells versus core diameter for cell concentrations of 106 and 5 X 10 6 ml" 1 .
recommended. The second option is to increase the cell concentration by a factor of five, however, there are limitations to this. Referring back to figure 2.8 we can see that increasing the cell concentration by a factor of five will decrease the distance between cells by the same factor. Thus, with a core diameter of 10 |im we will decrease the distance between cells from 1.27 cm to 0.254 cm. This would be no problem if all cells were spaced exactly 0.254 cm apart, but they are not. Cells enter the system at random and their arrival at the analysis point is determined by Poisson statistics. As the concentration rises, so there is a greater probability that more than one cell will be in the sensing volume at any one time. This is called coincidence. We must now make a slight diversion and consider some statistics. It had to happen sometime but it's not difficult, just applied common sense, persistence and
14
FLUID FLOW DYNAMICS 10 6 cells ml ~1
Core diameter, /zm Figure 2.9. Count rate versus core diameter for flow rates of 1 0 m s " 1 and 2 m s " 1 with a cell concentration of 10 6 ml~ 1 .
the acceptance of some very simple basic rules. If a coin has been spun 10 times and we are told that it came down heads upwards on six occasions we can surmise with absolute confidence that it landed tails upwards on the other four occasions. This assumes, of course, that this is a regular coin with both a head and a tail and that it did not come to rest on its edge which is not impossible but extremely unlikely. The chance of the latter occurrence can be calculated with a number of assumptions about the angular velocity and momentum of the spin, the thickness of the edge compared with the radius, the elasticity of the coin (remember it's going to bounce) and a number of other things. Just for fun I did this calculation for a UK 2p coin and got a probability of 10" 1 4 . Extraordinary what some people do for fun isn't it, but I've been in Medicine for some time now and nothing surprises me!! This result is probably not in error by more than three orders of magnitude either way. However, if 10 ~ 14 is correct and the coin was spun once every 4.75 seconds you would expect it to land and come to rest on its edge just 1000 times in the whole of the lifetime of the Universe to date (15 000 000 000 years). That is what is meant by the chance of an occurrence being vanishingly small. Occasionally you just have to trust the mathematics without experimental verification, unless of course you have phenomenal stamina and even greater stupidity. We know that the result will be either a head or a tail, no other option is open, therefore, the number of times tails is observed must be the number of times heads was not observed, which is given by the number of spins minus the number of heads. If a large number of spins is carried out the frequencies of heads and tails will both tend to 0.5 as, for each spin, the probability of the outcome being heads, 0.5, is equal to the
FLOW RATES AND POISSON STATISTICS
15
probability of the outcome being tails. This type of statistical problem is described by the binomial distribution which will be encountered in section 6.4. A different type of statistical problem arises if we are standing by a road observing cars on the near side passing from right to left (we are in England). We can count how many cars pass in 10 minutes, or any other interval of time, hence we can calculate a flow rate. It is self-evidently obvious, however, that it would be absolutely pointless to try to count how many cars did not pass the same point in the same time interval and statistics involving these types of observations cannot be handled by the binomial distribution. Cars passing a point along a road are isolated events occurring in a continuum of time as are cells passing the analysis point in a flow cytometer, and statistics of this nature are described by the Poisson distribution. I will not go into the mathematical derivation of this distribution although it is very straightforward. If you want full details I would recommend chapter 8, 'Goals, floods and horse kicks - the Poisson distribution' in Facts from Figures by M.J. Moroney (first published in 1951 and still in print). In order to use the Poisson distribution all we need is z, defined as the average number of times an event occurs within a continuum. The latter could be length, time, volume, area or anything and the probability of observing the event zero times or once, twice, thrice, etc. within a defined, and constant, increment of that continuum is given by the successive expansion terms of the expression e z x e " z . The mathematical notation of each element, p(n), of the Poisson distribution is p(n) = zne~z/n\ where p(n) is the probability of n events being observed. The value of n can be anything from 0 to oo, and nl is factorial n. The notation for the summation for the whole distribution is, n= n=0 which has unit value, and is a pretty fancy way of writing 1. In most cases that are likely to be encountered in practice p(n) becomes vanishingly small for values of n greater than 30 or so as factorial 30, the divisor (that's the bit underneath in the fraction), is a very large number. Values for n greater than 4 should never occur in flow cytometry and the terms of the Poisson distribution up to and including 4 are tabulated below in table 2.1. Table 2.1 Frequency that the number of events, n, are observed
probability of observing the n events
0 1 2 3 4
z°e"70!
z'e "71! z2e ~72! z3e "73! z4e "74!
16
FLUID FLOW DYNAMICS
The first term z°e z /0! reduces to e z as z° and 0! are both unity, and the second term reduces to ze~ z as z1 is z, and 1! is unity. All we need to know now is the average expectancy, z, that a cell will be in the sensing volume, which we will assume is a 30 |im length of the 10 |im diameter core. At a concentration of 106 cells ml" 1 the average spacing is 1.27cm, therefore the number of cells per unit length is 1/1.27 = 0.787 cells cm" 1 . We can now calculate the average number of cells in a 30 |im length which is given by (0.787 x 30)/1000, as there are 1000 |im in lcm. This gives 0.023 61 as the average number of cells in the sensing volume at any one time which is our z to be plugged into the terms of the Poisson distribution. We can similarly calculate z for cell concentrations of 3.16 X 10 6 ml~ 1 , l C m l " 1 and 3.6 x lO'ml" 1 , which are 1.0 T-,
^Single Double 0.1 -
Triple
.2* 0.01 (0
o a.
0.001
0.0001 10°
3.1x10°
107
3.1x10 7
,-1 Cell concentration, ml Figure 2.10. Probabilities of finding 0, 1, 2 and 3 cells in the sensing volume for cell concentrations of K^ml" 1 , 3.16 x lO'ml" 1 , IC^rnT 1 and 3.16 x 10 7 ml" l with a core diameter of 10 jam.
FLOW RATES AND POISSON STATISTICS
17
0.073 23, 0.2361 and 0.7323 respectively. The value of 3.16 appears to be a strange number to choose until you appreciate that this is yJlO. When you plot this on semi-log paper it is placed conveniently half-way between each decade mark on the scale; it just looks tidy particularly for things like antibody dilutions. Figure 2.10 shows the probabilities of 0,1,2 and 3 cells being within the 30 (im length of the sensing volume for cell concentrations of 106 ml~ l , 3.16 x 106 ml~ \ 107 ml~ 2 and 3 . 1 6 x l 0 7 m l " 1 with a core diameter of lOjim. At 106 cells ml" 1 the probability of zero events being in the sensing volume at any given time is 0.9766. In other words most of the time (i.e., 97.66%) there are no cells being illuminated which is not surprising as they are only 10 (im in diameter and are spaced 1.27 cm apart on average. The respective probabilities of finding 1 and 2 cells in the volume are 0.0231 and 0.000 272. The latter appears to be very small but it does represent 1.18% of the probability of the single event occurrence which means that we should expect approximately 1.2% of events recorded at an input concentration of 106 cells m l " l to be coincidence of 2 or more cells in the sensing volume. If we go to the extreme and increase the cell concentration to 3.16 x 10 7 cells ml~ * we find that there will be no cells in the sensing volume for 48.08% of the time. However, there are probabilities of 0.3521, 0.1289 and 0.0315 that there will be 1,2 or 3 cells in the sensing volume respectively. Thus, there are 36.6% (0.1289 x 100/0.3521) and 8.95% (0.0315 X 100/0.3521) chances that there will be 2 or 3 events in the sensing volume respectively at any given time with 3.16 x 107 cells ml" 1 . It should also be pointed out that these various probabilities, at a given core diameter, are independent of the speed at which cells are flowing through the instrument. If the overall fluid flow rate is increased the coincident events just arrive faster. From figure 2.10 we can see that with a core diameter of 10|im we should not be working with cell concentrations greater than about 3.16 x 10 6 ml" l where there is a probability of 3.75% that 2 or more cells will be in the sensing volume at any one time. Most flow cytometers will be working with core diameters of between 10 |im and 17.5 Jim. Referring to figure 2.9 we can see that this gives maximum count rates of 500 and 2500 cells s ~ l for core velocities of 2 m s " l and 1 0 m s " 1 respectively at 106 ml" \ If we double the cell concentration to 2 x 10 6 ml" \ we will be within the 3.75% coincidence probability calculated above and have count rates of 1000 and 5000 cells s" 1 for the low' and 'high' flow rate instruments respectively. The implications of all this for cell sorting are considerable and are discussed in sections 6.3 and 6.4.
3 Light and optics
The quantitative aspects of flow cytometry are based upon the measurement of light, be this fluorescent, scattered or absorbed. Because of this fundamental dependence on light some of its properties and its behaviour on interaction with matter will be considered briefly.
3.1
Snell's Law
A light beam which encounters a surface at an angle where there is a change in refractive index at that surface (also termed a dielectric interface) will exhibit two phenomena. Firstly, some of the light will be reflected symetrically about the perpendicular to the surface at an angle equal to the incident angle. Second, the remainder of the light will cross the dielectric interface and enter the second medium. However, the angle at which the beam traverses the second medium is not the same as the incident angle. This is refraction and both phenomena are depicted in figure 3.1 where the beam passes from a low (A) to a high (B) refractive index material. The first descriptive observation of refraction appears in Plato's Republic (c. 3 70 BC) with the following quotation attributed to Socrates '... the same object appears straight when looked at out of water and crooked when in water.. / (from Herzberger, 1966). Amazingly, the first measurements of refraction were performed by Ptolemy of Alexandria (c. AD 150). He constructed a circular disc, looking much like a clock face, with two equal-length pointers free to rotate about the center and the circumference was marked out with 360 equal divisions. The lower pointer was set at a given angle and the disc was immersed in water up to the center. The upper pointer was then adjusted to be in line with the immersed lower pointer. On removal from the water the angle between the two pointers was recorded and the results of a number of readings appear in tabular form in Ptolemy's Optics (modern translation by Govi, 1885). Ptolemy also recorded the incident and refracted angles for glass and his results for both water and glass are redrawn from Herzberger (1966) in figure 3.2 where the points represent the experimentally recorded data and the curves represent the true relationships. The agreements are incredible and this serves as an extraordinary illustration of what
SNELL'S LAW
19
Figure 3.1. Reflection and refraction at the interface between a low (A) to a high (B) refractive index material.
60
Incident angle
Figure 3.2. Ptolemy's results for refracted versus incident angles (points) for water and glass compared with the true relationships (curves) redrawn from Herzberger (1966).
20
LIGHT AND OPTICS
can be achieved with considerable ingenuity, brilliantly clear thinking and very simple apparatus. The precise mathematical relationship between the incident angle, i°, and the refracted emergent angle, e°, was derived some 1500 years after Ptolomy and is given by, nx sin (i°)=
where nx and n2 are the refractive indices of the materials A and B respectively. This relationship was discovered empirically by Willebrord Snel of Leiden in 1621 (not published officially in print; Herzberger, 1966) and was later derived mathematically by Rene Descartes (1637).
3.2
Refractive index
The refractive index, n, of a material is found by rearranging the equation above to give, n = n2/n1 = sin(f)/sin(e) and the measurements of i° and e° are made at the air/material interface. By convention air (also vacuum) has a refractive index of unity hence, nx = 1.0, and n2 becomes n, the refractive index of the material. A given optical material has different refractive indices at different light wavelengths and refractive index varies from material to material. This was first described formally by Isaac Newton of Trinity College, Cambridge, from the results of his classical prism experiments. These are reputed to have been initiated in the cupola of the college chapel before the plague in 1665 and they first appeared in print in the Philosophical Transactions of the Royal Society (Newton,
1672a). Some 30 years later his findings were also published in his book Opticks (Newton, 1704) and reproductions of four of the figures from that publication are shown in figure 3.3. Opticks fig. 13 shows the experimental setup with light from the sun shining on a screen containing an aperture with the light passing through the aperture and incident on a prism. This produced a series of different coloured images of the sun on a white screen, MN, with a red image in the position T and an indigo/violet image at position 'P. Opticks fig. 15 (left diagram) showed that the setup depicted in fig. 13 did not completely resolve each image. This was solved by using a second prism placed in the light beam at 90° to the first as shown in Opticks fig. 14. The different coloured images of the sun were now projected obliquely on the screen which completely resolved each image as in the right diagram of fig. 15 with the red image at 'el' and the indigo/violet at 'ag'. This result suggested that the different colours were not further divisible which was proved by the self-explanatory experiment depicted in Opticks fig. 18. The refractive index of any material should be specified at a particular wavelength but if the latter is not specified it is convention to assume that this is 532 nm the mid range of the visible spectrum. The refractive index dependence on
REFRACTIVE INDEX
21
Bookl.PlateHL P a r t i .
M
Figure 3.3. Results of Newton's prism experiments reproduced by kind permission of the Librarian of Trinity College Cambridge from Opticks (1704), Wren Library bench mark NQ.16.198. Opticks fig. 13 shows the experimental setup with the prism splitting the spectrum from the sun. The red image appeared at T ' on the screen on the left and the indigo/violet appeared at T'. Opticksfig.14 used two prisms set orthoganally which projected the coloured images as shown in the right diagram of Opticksfig.15 (see text). Opticksfig.18 demonstrated that a given colour band was not further divisible.
LIGHT AND OPTICS
22 1.60
X 0
1.55
u (0
1.50
-
1.45
300
400
500
600
700
Wavelength
Figure 3.4. Refractive index plotted against wavelength for a variety of optical materials.
wavelength is illustrated in figure 3.4 for higher index materials (optical crown) through to low refractive index materials (fused silica). Water is obviously an important medium in flow cytometry which has a refractive index of 1.33 at 532 nm and this also varies with wavelength.
3.3
Focussing
Discrete parallel beams of light striking the interface shown in figure 3.1 will all be refracted through the same angle into the medium and the beams in the medium will also be parallel. However, if the surface is curved the angle of incidence will be different for each beam and these will not be parallel after refraction into the second medium. If the latter is of lower refractive index than the first medium the beams will diverge, but if the refractive index is higher in the second medium the beams will converge. This is illustrated in figure 3.5 (panels A and B) and forms the basis for light focussing. In order for the beams represented in figure 3.5 to appear to diverge from point A or converge to point B the curvature has to be a surface of revolution of a conic section. However, over 'small' angles this is well approximated by the surface of a sphere and the majority of lenses are constructed with spherical surfaces. Extending Snel's Law, with a little bit of mathematics, to spherical surfaces gives rise to the familiar paraxial lens formula,
where/is the focal length of the lens and where sx and s2 are the conjugate distances.
FOCUSSING
23
Figure 3.5. Monochromatic light refraction at a curved surface. The beam is passing from a high to a low refractive index material in the top panel and the emerging beam appears to diverge from point A. In the bottom panel the same curved surface is encountered but now the beam is passing from a low to a high refractive index medium and converges to point B. The meanings of the focal length and conjugate distances are shown in the ray diagram of figure 3.6 where, by convention, the propagation of light is always depicted as being from left to right. In the top panel light is being emitted from a point source at infinite distance and enters the lens as a parallel beam, hence s l is infinite and the first term on the right-hand side of the paraxial lens formula is zero. Thus, after refraction by the lens the parallel beam converges to a point at a distance f=s2 from the lens on the right. This is the focal length of the lens. If, however, the point source from which the light is being emitted on the left is closer to the lens than infinity then the beam entering the lens will not be parallel and the refracted beam on the right will converge (focus) at a greater distance from the lens than the focal length (bottom panel). The focal length is a constant of a particular lens at a given wavelength (this is wavelength dependent as refractive index is wavelength dependent) but the conjugate distances vary. Before we go any further it must be pointed out that the paraxial lens formula given above is a working approximation which strictly is applicable only for 'thin' spherical lenses for rays close to the optical axis. This is because the 'true' surface of revolution to obtain 'point' focussing is not circular but conic, however, in the paraxial region a circle approximates very closely to a conic section. Thus, a spherical lens does not focus all rays entering over the whole surface to a discrete point. This is called spherical aberration and is depicted in figure 3.7 where marginal rays focus slightly nearer the lens than do paraxial rays close to the central optical axis of the lens. This results in a 'focal volume' which is bounded by an 'envelope'. The most intense plane through the focal volume perpendicular to the optical axis is called the disc of least confusion which is indicated by the black arrow in figure 3.7.
24
LIGHT AND OPTICS
A
Figure 3.6. Ray diagram of refraction by a lens where, by convention, light is propagated from left to right. In the top panel light is being emitted from a point source at infinite distance and enters the lens as a parallel beam. After refraction this parallel beam converges to a point F at a distance from the lens equal to the focal length. In the lower panel light is being emitted from a point source at a finite distance from the lens and the beam is not parallel on encountering the lens. After refraction the beam on the right will now focus to a point at a greater distance from the lens than the focal length.
Figure 3.7. Spherical aberration. Marginal rays focus slightly nearer the lens than do rays close to the central optical axis of the lens. This results in a 'focal volume' which is bounded by an 'envelope'. The point of least confusion, maximum light flux, is indicated by the black arrow.
FOCUSSING
25
The refractive index dependence on wavelength has important consequences for the whole of optics as well as for dual-beam focussing in flow cytometry (see section 33.2). From figures 3.3 and 3.4 we can see that light of longer wavelengths will be refracted less than that of shorter wavelengths. Extending this result to the curved surfaces of a lens shows that red light is focussed at a greater distance from the lens than shorter wavelength violet light. This is termed chromatic aberration and microscope lens systems are designed to overcome this effect to a large extent. 3.3.1
Single beam Two systems are used in flow cytometry to focus the illuminating light to the point at which it intersects the cell stream. One type of system uses a spherical lens to give a focal spot size of 30-60 urn where the geometry is essentially identical to that in figure 3.7. The second system uses a pair of crossed cylindrical lenses to focus the light to a sheet about 120 |im wide and 4—7 |im deep. Cylindrical lenses are constructed with a curved surface in only one plane which focus a beam of incident light to a line in the focal plane. Two cylindrical lenses, with their focal planes at 90° to each other, can be used in flow cytometry as follows. The lens nearer to the laser has a long focal length which focusses light at the cell stream in the horizontal plane. The second lens, which is further from the laser, has a short focal length and focusses light in the vertical plane. Hence, the focal length of the lens nearer the laser must have a focal length equal to the distance between the lenses plus the focal length of the second lens. This is shown diagramatically in figure 3.8 where the light is focussed to a sheet across the cell stream. Generally, there is little to choose L1
L2
Figure 3.8. Focussing geometry of a crossed cylindrical lens pair where the beam is of square section and entering from the left. The lenses are facing the wrong way but it was easier to draw as shown.
26
LIGHT AND OPTICS
between these two focussing systems for the simpler types of assays. However, the crossed cylindrical lens pair does have the apparent disadvantage that the area under the pulse of light emitted from each cell has to be digitized and frequently the pulse height and width (time of flight through the beam) are also digitized. This has the disadvantage that more electronics are required and more data may need to be collected. The immediate advantages of the crossed cylindrical lens pair are as follows. Firstly, it is possible to focus two very different wavelength beams to the same point (see next section). Secondly, there is usually a higher light flux at the focus with the crossed pair. Thirdly, the sheet-like focussing allows greater latitude in positioning the core within the sheath, a point which will be discussed further in section 3.9.5. Finally, the increased data obtained with the crossed cylindrical lens pair (pulse height, width and area) can be used to give some low resolution object shape information (see section 3.9.6) and can be used for high resolution slitscanning (see section 8.1).
3.3.2
Multiple beams
Multiple beam focussing can get a little complicated. If you have only one beam skip this and go on to interference and diffraction in section 3.4. Figure 3.4 demonstrated the dependence of refractive index on wavelength and that shorter wavelength light is refracted to a greater extent than the longer wavelengths. Potentially, this could cause problems for dual- or triple-beam excitation as the focal length of a lens will change with wavelength. However, a number of methods have been devised to circumvent the problem. The simplest is to have one focussing lens system for each beam so that adjustments can be made for each wavelength independently (Shapiro et a\., 1977; Steinkamp, Stewart and Crissman, 1982). The usual arrangement is to have the light beams in the same horizontal plane each directed to the center of flow with the smallest possible angle between them. This system is preferable for triple-beam excitation but it does require considerable space particularly if large lasers are being used. A second method uses a dichroic mirror (see section 3.5.5) to 'mix' the two beams by reflecting one and transmitting the other which are then both focussed through either a spherical lens or a crossed cylindrical lens pair. This set-up is shown in figure 3.9 with the beams offset for greater clarity. The shorter wavelength beam, UV in the example, focusses closer to the lens than the longer wavelength beam, blue, at points SFL and LFL respectively. This clearly presents a problem; however, this can be overcome by using an auxiliary focussing lens before one of the beams reaches the dichroic mirror (Fellner-Feldegg, 1985). This auxiliary lens can be either diverging, A, or converging, B, and these have to be placed respectively in the short or long wavelength beams. If a diverging lens is used in the short wavelength beam the 'short focal length' point (SFL in figure 3.9) will be shifted towards the long focal length' point (LFL). The converse effect is to use a converging lens in the long wavelength beam which then shifts the LFL point towards SFL.
FOCUSSING
11
uv Laser focussing lens LFL
Blue Dichroic Figure 3.9. Two beams of different wavelengths (colours) are 'mixed' by a dichroic mirror then focussed through the same lens system where the beams have been offset for greater clarity. The points SFL and LFL are the focal points of the shorter and longer wavelength beams respectively. Placing an auxiliary converging lens in the light path of the longer wavelength beam before this strikes the mirror will shift LFL towards SFL. An auxiliary diverging lens for the shorter wavelength beam will shift SFL towards LFL.
The final method also uses a 'mixing7 dichroic mirror as shown in figure 3.9 but it focussed both beams to the same point through a single crossed cylindrical lens pair without the auxiliary lens (Watson, 1981). The trick is to increase the light path length of the longer wavelength beam through the focussing lens system. This is effected by exploiting both spherical aberration and astigmatic focal shift as follows. Spherical aberration, where marginal rays focus closer to a lens than paraxial rays of the same wavelength, was described in figure 3.7. We have also seen that longer wavelength light is refracted less than light of shorter wavelength and that if we pass two beams of different wavelengths through the center of a lens the longer wavelength beam will focus at a greater distance from the lens than the shorter wavelength beam as in figure 3.9. However, if we progressively displace the longer wavelength beam towards the periphery of the lens and keep this parallel to the optical axis it will focus progressively closer to the lens due to the effect of spherical aberration. Thus, it is possible to find a lateral displacement of the longer wavelength beam such that both beams focus to the same point. A crossed cylindrical lens pair is ideal for this type of manoeuvre as each lens focusses in only one plane, thus the focussing characteristics are dissociated in the horizontal and vertical planes. By parallel displacement of the longer wavelength beam in both planes with respect to the shorter wavelength beam passing through the center of the lens pair it is possible to focus both beams to the same point in both planes. This is illustrated in figure 3.10 with short (UV) and long (blue) wavelength beams passing through the system from left to right with the former in the paraxial position. Panel A shows the view from the top where the cylindrical lens Lt focusses both beams to the point F in the horizontal plane. If both beams had been UV then that in the peripheral position would have focussed closer to the lens due to spherical aberration. However, because it is blue it is refracted less than
28
LIGHT AND OPTICS
Figure 3.10. Dual-beam focussing of two different wavelength beams (blue and UV) to the same point through a crossed cylindrical lens pair where the light is propagated from left to right and the UV beam passes paraxially through the system. Panel A, the view from the top showing the horizontal displacement of the blue beam with respect to the UV. Panel B shows the downward displacement of the blue beam with respect to the UV. Spherical aberration due to marginal displacement of the blue beam induces a focal length shortening in the horizontal plane at the first lens, Lv and in the vertical plane at the second lens, L2. Panel C shows the positions of the beams looking into the system from the left and panel D shows their positions on a screen beyond the focal point on the right. it would have been if it had been UV and hence focusses at F. Note that the cylindrical lens L2 plays no part in focussing in this plane. Panel B shows the events taking place in the vertical plane where both beams pass through the first lens Lj with no refraction. Lens L2 then focusses both beams to F by the same processes as were described for the horizontal plane. Panels C and D respectively show the positions of the beams looking into the system from the left and on a screen beyond the system on the right. The net effect is that the blue beam passes obliquely through the lens system from bottom left to top right and traverses a greater distance in the system than the UV beam. This increase in path length of the blue beam with respect to the UV compensate for the difference in refractive index of the lens material (fused silica) at the two wavelengths. This method is capable of focussing the two beams to the same point but there are some applications (see section 12.2 and chapter 13) where the beams must be offset in the vertical plane for sequential illumination. This can be achieved by using astigmatic focal shift. Consider a light wave-front, W-v propagated from a point source, P, and incident on a spherical lens which is depicted in figure 3.11 A. The incident wave-front is retarded more at the center of the lens of height, h, than at the periphery by the optical path length jh2k, where k is a constant of the lens.
FOCUSSING
29
Figure 3.11. Astigmatism. The wave-front, Wir incident upon the lens in both panels is propagated from the point P, and the emergent wave-front is denoted We. Tilting the lens through 0°, panelB, causes a relative increase in curvature encounterd by the incident wavefront and results in the astigmatic focal shift, d", towards the lens with focussing at the point P". This is responsible for the change in axial wave-front, We, on emergence from the lens after refraction with subsequent focussing at the point P'. Let the lens be tilted through an angle (j)°as shown in figure 3.1 IB. If the lens is 'thin' and the angle (j)°is 'small' then, to a first approximation the same optical path difference will occur between the center and the periphery. However, the periphery of the lens is now closer to the center of the lens (h x cos (f)°) in the plane of the diagram and consequently there is a greater relative increment in curvature encountered by the wave-front Wj. This increase in curvature will decrease the focal length in this plane. However, there has been no change in the increment in curvature perpendicular to the plane of the diagram and the focal length is not changed in that plane. This is astigmatism and the astigmatic focal shift is denoted by d". Figure 3.12 shows the computed paths of four beams of monochromatic light through a 'thick' lens of short focal length. Three beams enter the center of the curved surface of the lens at angles of 0°, 15° and 30° to the optical axis and are labelled 0,15 and 30 respectively. A fourth beam enters the lens at 15° but is offset from the optical axis and is labelled 15d. The three beams entering the center of the lens are focussed on the right at the points marked 0,15 and 30. The focal point of
30
LIGHT AND OPTICS
15
Figure 3.12. Computed paths of beams entering a 'thick' lens at various angles of incidence and lateral displacements (see text). four further beams entering the center of the lens at 5°, 10°,20° and25° were also computed. The dashed curve shown, on which all of these points lie, represents a section in the plane of the diagram on which a thin beam of parallel light will be perfectly focussed if it enters the center of the first surface of the lens at any angle between 0° and 30°. Theastigmatic focal length shortening described above is clearly apparent as is the 'off-axis' deviation which is most prominent with 'thick' lenses. Consider now the four rays labelled a, b, c and d which all enter the lens at 15° but with different lateral displacements. Rays a and b intersect the above mentioned surface at the point a which is the focal point of the beam ab (this is also point 15). Rays b and c intersect at p which is the focal point of the beam be. Similarly, rays c and d intersect at the point y. Thus, we have not only an astigmatic focal shift due to the angle of incidence but also a focal length shortening with increasing lateral displacement due to 'off-axis' spherical aberration. In order to obtain sequential illumination for flow cytometry we require that the blue and UV focal points be separated in the vertical plane. Consider again figure 3.10. Horizontal or vertical displacement of the blue beam parallel to the UV will move the focal point along the optical axis, it will not move it off the axis. Off-axis shift can only be effected by an angle change. Let the paraxial beam entering the lens at 0° infigure 3.12 be of shorter wavelength than that of the beam shown. The focal point of this new beam will be closer to the lens and will tend to lie under the points a, P and y. Thus, vertical displacement of the two beams can be achieved by altering the angle of incidence and exploiting a combination of astigmatic and spherical aberrations in the longer wavelength beam. The displacements and angulation changes required to effect these procedures are very small and very high precision beam positioning capability in three dimensions is essential. Figure 3.13 shows multiple superimposed storage oscilloscope traces of light scatter pulses obtained simultaneously from micro-
INTERFERENCE AND DIFFRACTION
31
Figure 3.13. Multiple (2000) superimposed storage oscilloscope traces of light scatter pulses obtained simultaneously from microbeads with the blue beam, top, and the UV, inverted. The beams were focussed to the same point and each division on the oscilloscope screen represents 100 ns.
beads with the blue beam, top, and the UV, inverted. The beams were focussed to the same point and each division on the oscilloscope screen represents 100 ns (1 ns is one thousandth part of one millionth of a second). It can be seen that the beams are aligned such that the beads arrived at the two focal points within + 10 ns. The sample velocity was 1.8ms" 1 , thus the beams were aligned to within + 1 8 n m (1 nm is one thousandth part of one millionth of a meter). It is a tribute to our mechanical engineering workshop that this incredible degree of precision could be achieved, and to our electronics workshop that it could be measured.
3.4
Interference and diffraction
Diffraction, which can be constructive or destructive, is synonymous with interference. The terms just tend to be used in different contexts. Consider the parallel wave-front arising on the left of figure 3.14 and incident on an opaque
32
LIGHT AND OPTICS
screen, Si, containing a single slit which acts as a secondary point source for wave propagation beyond the slit, the principle introduced by Huygens (1690). The secondary wave is propagated as an expanding 'cylinder' which then strikes a second screen, S2, containing two slits, A and B, both of which act as point sources for further wave propagation beyond the second screen. At given points these tertiary waves are in phase and at varying degrees out of phase. If two waves are exactly in phase the effect is additive giving rise to constructive interference. If the waves are exactly out of phase destructive interference takes place. This can best be seen by looking along the diagram from the left where you will see alternating light and dark bands, which represent constructive and destructive interference respectively, fanning out along the length of the diagram. The resultant light intensity exhibits a sinusoidal pattern and is depicted in figure 3.14 on the 'screen' on the right. What we see is a series of light and dark bands (vertical slits) across the screen. These observations were originally presented to the Royal Society of London by Thomas Young in 1802 and the formal concept of interference, which established the wave nature of light, was introduced two years later (Young, 1804). Figure 3.14 was redrawn from Young's original publications where he indicated the positions of the destructive interference patterns by the letters C, D, E and F. The 'screen' on the right was added by the author. An opaque or semiopaque circular object (e.g. a cell) in a light beam will induce interference at the
S1
S2
Figure 3.14. Interference. This is a composite redrawn from Thomas Young's original diagrams (Young, 1802, 1804) with permission of the Librarian of the Royal Society of London. The parallel wavefront on the left is incident on a screen, Si, containing a single vertical slit of which we are viewing a horizontal section. The slit induces secondary wave propagation as a 'cylinder' emmanating from the slit which is now incident on a second screen containing two slits A and B. Each of these act as point sources for propagation of tertiary waves to the right which produce constructive and destructive interference. Look along the diagram from the left to see the alternating light and dark bands which represent constructive and destructive interference respectively. The latter were indicated by the letters, C, D, E and F by Young. The 'screen' on the far right which depicts the light intensity variation has been added by the author.
INTERFERENCE AND DIFFRACTION
33
edges of the object and we see a series of light and dark concentric rings known as the Airy disk (Airy, 1838, 1848). Interference also takes place as light passes through thin films. The manifestation of this can be seen as the different colours in soap bubbles and thin layer Musscovy glass which were observations published by Newton's great rival Robert Hooke in his Micrographia in 1665. However, the phenomenon had also been studied by Newton (1672b) and the findings tend to be associated with the latter scientist as 'Newton's rings'. It is also worth remarking that the phenomenon is readily observable in petrol (gas) stations after rain has fallen. A thin film of oil floats to the top of the water on the forecourt giving rise to interference within the film and multiple colours which can be quite striking. Consider the 'thin' slice of high refractive index material depicted in figure 3.15 with a beam of incident photons, A, encountering the interface at an angle. Some of the incident light will be reflected as 0Cj and the remainder will be refracted into the medium. The relative proportions of refracted and reflected light depend on the refractive index difference. Some of the light travelling in the medium will be refracted at the second interface which is now a high-to-low refractive index boundary. The refracted portion of the beam on exit from the film will be displaced but parallel to the original beam A. However, some of the light in the medium will be reflected within the medium at this second interface towards the first surface where it will be refracted as the beam oc2 parallel to OLV Now let us suppose that a second beam of identical photons, B, parallel to A was incident on the first surface at the point where the beam oc2 emerges from the surface. This is also shown in figure 3.15 where the reflected portion of the beam B, $v will not only be parallel to, but also coincident with the beam oc2. These beams may be exactly in-phase or at varying degrees out-of-phase (phase shifted) depending on the angle of incidence and thickness of the high refractive index material. If the beams a 2 and (^ are totally in-phase constructive interference will result; if they are totally out-ofphase destructive interference takes place.
Figure 3.15. Interference at a 'thin' film (see text).
LIGHT AND OPTICS
34
The phase shift described above is dependent on the refractive index, angle of incidence and thickness of the material, and the primary beams A and B do not have to be at an oblique angle to the surface. They can enter perpendicular to the surface (angle of incidence 0°) in which casethe thickness of the medium to obtain either constructive or destructive interference would be different from that required to obtain these effects if the beam was entering obliquely.
3.5
Optical filtration
Some form of optical filtration system is required whenever fluorescence is being observed or measured and filtration relies on only two properties, absorption and interference. These properties can be used either individually or in combination to give five types of filter, namely short- and long-pass filters, dichroic mirrors, band-pass and neutral density filters. Short- and long-pass filters respectively transmit (pass) light below and above a specific wavelength. The latter is usually specified as the 50% transmission wavelength. Dichroic mirrors are designed to reflect above and below the specified 50% transmission level and band-pass filters transmit light within a given wavelength band, where again the 50% transmission wavelength is specified for both the cut-on and cut-off. Neutral density filters attentuate light by specified quantities over a given wavelength range.
3.5.1
Absorption filters
Absorption filters are coloured glasses which absorb light of specific wavelengths. However, it is difficult to construct coloured glass to absorb longer
ttance
0.99
0.95 0.90 .
0)
0 ) »-
CO L,
» -
_ ,
•_ . ,
,
-w
v " T V v v ^ " " " "5 W IO CO CO CO CD
2
0.70
75 o
0.50
oooouoooouo oooo OUOOOOOOOOO 0:0:0:0: /
Fracti
mm
0.01 1O-3 10 10"410" 5
I
200
400
600
800
Wavelength (nanometers) Figure 3.16. Examples of coloured glass long pass filters from the Melles Griot catalogue.
OPTICAL FILTRATION
35
wavelengths without absorbing the shorter wavelengths (short-pass). It is much easier to absorb light below a specified wavelength and to transmit the longer wavelengths (long-pass). Hence, absorption filers tend to be of the long-pass variety and an example from the Melles Griot catalogue is given in figure 3.16. Two examples of absorption band-pass filters are shown in figure 3.17. The first are yellow/red absorbing filters which transmit blue-violet light (top panel figure 3.17) where the cut-on, in the region of 325 nm, is fairly sharp but the cut-off, in the 475 nm region, is less sharp. Also, light beyond 650 nm is being transmitted. A similar phenomenon is seen in the bottom panel of figure 3.17 which shows the characteristics of UV transmitting filters.
3.5.2
Neutral density filters
Neutral density filters, which have not received the attention or use in flow cytometry that they either could have or should have, are also absorption filters which are designed to absorb all wavelengths of light to an equal degree over a specified wavelength range. The attenuation is specified in optical density 0.99 -i
0.95 0.90 0.70 0.50
4-
- B G 37-
0.01 10 3 10
- B G 12-
JIS
10
(0
o o
(0
U G 5
/ /
200
400
UG11
600
800
1000
Wavelength (nanometers) Figure 3.17. Absorption band pass filters (Melles Griot). Top panel, red absorbing blue-violet glass filters and bottom panel UV transmitting black glass filters.
36
LIGHT AND OPTICS
(OD) units which are logarithmically calibrated. For example, OD filters of 1,2 and 3 attenuate the incident beam by factors of 10, 100 and 1000. Neutral density filters can be used to great effect when sequential samples with very different fluorescence intensities are being analysed on the same photodetector where comparisons between samples are required without changing the instrument settings. Examples of such usage will be given later in section 9.3.2. 3.5.3
Interference filters Interference filters are designed to reflect light of some wavelengths and to transmit others using both destructive and constructive interference in multiple layers of alternating high and low refractive index material. Interference in a single thin film was described in figure 3.15 and multiple stacks of such high and low refractive index material can be designed as resonance cavities which selectively reflect or transmit some light wavelengths and destroy others. The thicknesses of the coatings of high and low refractive index materials are critical and they vary according to the design wavelength and required angle of incident. When interference filters are designed for light entering perpendicular to the surface the respective thicknesses of the high and low refractive index material are exactly one quarter (f/l0) and one half (jA0) of the design wavelength which is called /l 0. A typical transmission curve for an interference filter is given in figure 3.18 which shows a sharp transmission spike at the design wavelength, /l 0. Note, also, that there is very good transmission in the regions of the \X0 and 2 X Xo harmonics. Within reasonable limits, the width of the Xo transmission peak shown in figure 100 -.
80
(0
60
40 O 0) 0.
20
K Wavelength figure 3.18. Interference transmission curve with a sharp spike at the design wavelength, Ao. There is very good transmission in the regions of the jXQ and 2 x l 0 harmonics.
OPTICAL FILTRATION
37
3.18 can be made as large or as small as required and by using a second filter designed for a different wavelength it would be possible to block out both the Ao and 2 x XQ transmission peaks shown in this figure. This would result in a shortpass filter for the \X0 region of the spectrum. 3.5.4
Band-pass filters Band-pass filters are constructed as a combination of interference and coloured glass absorption filters to transmit a specific wavelength band. For example a band-pass filter for the Xo transmission spike of figure 3.18 would use a coloured glass long-pass absorption filter centered in the trough immediatly to the left of the required transmission spike. This would absorb the shorter wavelength light on the left of the trough. A second interference filter would then be needed to block transmission above the trough to the right of the required spike. The latter, obviously, must be designed to transmit the Ao spike as efficiently as possible. It is never possible to obtain a band-pass filter where there is zero probability of transmitting an unwanted photon. There is always a shoulder in both the 'cut-on and 'cut-off' regions of the spectrum. These filters are also relatively expensive as their structure is complex and they must be made to very tight specifications. This is illustrated in figure 3.19 which shows a cross section of a typical, but relatively simple, two-cavity band-pass filter. More complex filters have many more layers and cavities. 3.5.5
Dichroic mirrors Dichroic mirrors also operate using interference but they are designed to be used at an inclination ot 45° and the thicknesses of the high and low refractive index layers deviate from the \kQ and \kQ which are used for perpendicular
unfiltered light in
| metal -dielectric multilayer blocking filter
|/f
:':•:.•
• ":
:
'
\[
'
Figure 3.19. Construction of a relatively simple, two-cavity band-pass filter. More complex filters have many more layers and cavities. Redrawn from the Melles Griot catalogue.
LIGHT AND OPTICS 0.9-
FT 395
FT 425 FT 460
FT 510
FT 580
0.7-
0.1 -
Figure 3.20. Transmission characteristics versus wavelength of the Zeiss dichroic mirrors. Redrawn from the Zeiss monograph, Fluorescence Microscopy. incidence. They are also designed to minimize absorption as both the reflected and transmitted rays are required. The wavelength specified is again that of the 50% transmission point and the Zeiss catalogue dichroic filter transmission characteristics are shown in figure 3.20. 3.5.6
Dichroic combinations Multi-fluorescence assays require that the UV-through-visible spectrum be divided into a number of different wavelength bands. This is effected using a series of dichroic mirrors. However, care must be exercised in their arrangement to minimize light loss. One arrangment of four of the Zeiss series of dichroics plus two from Melles Griot, with 50% transmissions centered at 390 nm, 420 nm, 460 nm, 510 nm, 560 nm and 630 nm respectively, is shown in figure 3.21. This splits the spectrum into seven primary bands namely, UV (<390nm), violet (390-420 nm), indigo/low-blue (420-460 nm), high-blue/green (460-510 nm), green (510-560 nm), yellow/orange (560-630 nm) and red ( > 630 nm). With this DC 390
DC 420
UV
Violet
DC 460
Indigo
DC 510
Blue
DC 560
Green
DC 630
Orange
Figure 3.21. Sequential arrangement of six dichroic mirrors giving seven spectral bands, namely UV( < 390 nm), violet (390-420 nm), indigo/low-blue (420-460 nm), high-blue/green (460-510 nm), green (510-560 nm), orange (560-630 nm) and red (>630nm).
LIGHT COLLECTION DC 420
39 DC 630
DC 510
-•Red
DC 560
DC 460
DC 390
-Indigo
Violet
- Green
Orange
Blue
Figure 3.22. Alternative dichroic arrangement to give the same seven spectral bands as in figure 3.21, but with fewer light losses, see table 3.1.
particular arrangement the red light has to pass through all six filters and will suffer some light loss at each transmission. At the other end of the spectrum the UV light is reflected off the first surface of the first dichroic and experiences no transmission. Generally, relatively more light is lost in transmission than in reflection and another arrangement of the dichroics is shown in figure 3.22. Here, the red light is transmitted through only three mirrors and table 3.1 shows a summary of the numbers of reflections and transmissions for each colour band with both configurations. Clearly, the arrangement in figure 3.22, which was implemented in our instrument, is superior overall.
Figure 3.21 3.22
3.6
Voilet 390-420 nm
Indigo 420-460 nm
Blue 460-510 nm
Green 510-560 nm
Orange 560-630 nm
>630
T:R
UV <390 nm
T R T R
0 1 0 2
1 1 1 1
2 1 1 2
3 1 2 1
4 1 2 2
5 1 3 1
6 0 3 0
Red nm
Light collection
The capacity to make any measurement at all in flow cytometry depends primarily on the quantity of light that can be collected from each cell hence, light collection efficiency is important. Light emitted from a point source is propagated equally in all directions. Thus, a wave front emerging from a point will expand as a sphere whose area is given by the expression 47Tr2. Consider that the ray direction
LIGHT AND OPTICS
40 100
90
Cone
1
120
150
180
/2 angle (degrees)
Figure 3.23. Proportion of total light emitted from a point source versus cone collection half-angle. Most flow cytometers operate in the hatched region B. High collection efficiency instruments operate in the hatched region A.
in figure 3.6 is reversed so that the lens is collecting light from the focal point which is emitting light in all directions. The quantity of light that can be collected is directly proportional to the angle at the apex of the cone of light which the lens intercepts. A measure of this light collecting capacity is given by the expression known as the numerical aperture, NA, where NA = n sin 9°; 9° is the conehalfangle and n is the refractive index of the medium from which the light is being emitted. The numerical aperture is a suitable method for specifying lens light collection capacity when the cone half-angle is relatively small. However, it is not entirely satisfactory for large half-angles when these exceed about 60° which is about the maximum that can be attained with refracting systems. A better method of representing collection capacity is to specify the quantity of light collected from a point source in proportion to the total light emitted. The latter is given by the expression 471, and the amount of light, L, emitted with a cone half-angle of 9° is given by the relationship, L = 27T(l-cos0°)
FLOW CHAMBER DESIGN
41
Thus, by taking the ratio of L to An we get, pi = \{1- cos 6°) where pL is the proportion of the total light collected at a given cone half-angle 9°. A plot of pL versus cone half-angle is shown in figure 3.23. Most flow cytometers operate with a cone half-angle between 15° and 25° and this region of the figure is cross hatched and labelled B. By reading off on the Y-axis we can see that this represents a light collection efficiency within the range of 2% to 5%. Some high light collection efficiency systems have been designed to give effective cone collection half-angles between 40° and 60° (Steen and Lindmo, 1979; Watson, 1985) but even with these systems the light collection efficiency is between only about 12% and 25% as can be seen from the cross-hatched area labelled A in figure 3.23. Lens systems, which rely upon refraction, are not capable of collecting more than about 25% of the total light emitted from a point source. In order to improve upon this we must abandon refraction and use reflection which will be discussed later (section 3.7.4). The light collection optical systems in flow cytometry vary from single spherical lenses to microscope objectives but the amount of light that can be collected from each cell depends critically on the type of flow chamber used and must be considered in conjunction with flow chamber design.
3.7
Flow chamber design
A number of different types of chamber have been constructed. They fall into two basic categories but all include the Crosland-Taylor concept. In the first type the beam is focussed on the cell stream while this is still contained within the chamber which is usually square or rectangular in cross section. In the second type a jet issues from a nozzle and interrogation of the cell stream by the laser takes place in the jet-in-air just below the orifice.
3.7.1
Cuvette
Square cross section chambers, where cells are analysed within the chamber, suffer from the disadvantage that the light cone emitted from the cell stream is refracted away from the collecting lens in both the vertical and horizontal planes. This is depicted in figure 3.24 which represents a cross section of such a chamber. The geometry is 'to scale7 and the secondary principle plane of the collecting lens, which is accepting a cone half-angle of 40°, is shown on the right. This is about the maximum that can be collected with a dry lens system but due to the diverging refraction the cone half-angle from the stream is only about 29°. However, this type of system does have the advantage that there is very little reflection of the primary exciting beam into the collecting lens. Furthermore, a microscope objective optically coupled with immersion oil to a rectangular section chamber can collect a 60° half-angle cone of light which increases the light collection efficiency from about 4% to 25%. Square cross section chambers can also
42
LIGHT AND OPTICS
2°PP
Figure 3.24. Horizontal section of the light collection geometry from a cuvette where light is refracted away from the collecting lens at the chamber/air interface. Similar refraction diverging from the collecting lens occurs in the vertical plane.
Jet
Vertical plane
Horizontal plane
Collecting lens view of light cone
Figure 3.25. Light collection geometry from a jet-in-air. In the vertical plane (top) light is refracted away from the light collecting lens as in figure 3.24. However, in the horizontal plane light is emitted radially with no refraction. Thus, the light collecting lens 'sees' an ellipse of light from the cell stream.
FLOW CHAMBER DESIGN
43
be modified using a mirror and lens which also increases the collection efficiency to 25% (see section 3.73). 3.7.2
Jet-in-air Consider the vertical jet-in-air system where the cells are in the center of a cylinder which is depicted in figure 3.25. In the vertical plane light is refracted away from the collecting lens at the jet/air interface as in figure 3.24. However, in the horizontal plane fluorescent light is emitted radially with no refraction at the jet/air interface. The net result is that the collecting lens 'sees' a horizontal ellipse of light from each cell. Furthermore, a not inconsiderable proportion of the primary exciting light beam is reflected from the air/jet interface into the collecting lens. This tends to be overcome by placing an obscurating bar in front of the lens to block this reflected light but this reduces the quantity of fluorescent light that can be collected. Also the collecting lens must be placed at some distance from the jet to avoid spray from the jet with a reduction in the solid angle of the light collection 7
0)
i
6
O 0)
Jet, O
5
O>
I ^ Cuvette 4 -
0) O) CD
5 2 o
<5
Q.
1O C
20°
40°
Collection V2 angle Figure 3.26. Proportion of light actually collected as a percentage of the total emitted for a dry lens system plotted against collection half-angle. The solid line is for a jet-in-air assuming a refractive index of 1.33 for water and a 1.0 mm width obscuration bar. The dashed line is for a square-cross-section cuvette.
44
LIGHT AND OPTICS
cone. The light collection efficiency, defined as light actually collected as a percentage of the total emitted, for both the jet-in-air and cuvette systems are plotted against collection half-angle in figure 3.26. The jet-in-air data were calculated assuming a refractive index of 1.33 for water and a 1.0 mm width obscuration bar to block the scattered light. These data show that the jet-in-air is marginally more efficient that the cuvette; however, the former cannot be modified for increased collection efficiency as described in the next section.
3.7.3
Modified cuvette
Fox and Coulter (1980) were the first to appreciate that addition of a lens to the surface of a square-cross-section cuvette could partly eliminate the problem of diverging refraction at the chamber/air interface. This idea was later extended with the addition of a short focal length lens plus a mirror (Watson, 1985). The system is shown in figure 3.27 where the quartz chamber has a refractive index of 1.42 and the modifying lens was constructed from crown glass with a higher
V/////////////7/7,
Figure 3.27. Addition of both a spherical lens and a mirror optically coupled to a square-cross-section chamber allows two 90° cones of light to be collected and increases light collection efficiency by 600%.
FLOW CHAMBER DESIGN
45
refractive index of 1.52. Thus, at the chamber/lens interface (optically coupled with immersion oil) there is now 'converging' refraction towards the light collection system. Furthermore, as the center of curvature of the lens was designed to be between the cell stream and the collecting lens there is further converging refraction towards the collecting lens at the glass/air interface. This increased the collection solid angle from a 55° cone to a 90° cone which improved the light collection efficiency from about 3.8% to 12%, a gain factor of 300%. A further gain factor of 300% was obtained by placing a second spherical lens, silvered on its curved surface on the opposite side of the cell stream thus reflecting back a second 90° light cone. This further modification enabled 25% of the total light emitted from the cell stream to be collected with a dry lens system.
3.7.4
Spherico-ellipsoidal
In order to improve light collection efficiency above about 25% we must turn to reflection. Skogen-Hagenson et al. (1977) used a hollow ellipsoidal reflector which had a 60% light collection efficiency in a laser-based instrument. However, this was bulky as the majority of the ellipsoid was used and it would not fit easily into standard flow cytometers. It was also difficult to keep clean as the fluid jet passed through the primary conjugate focus within the hollow reflecting surface. However, a compact chamber has been constructed with light collection efficiency >S5% by using a combination of spherical and ellipsoidal surfaces (Watson, 1989). Consider the ellipsoidal reflector depicted in figure 3.28A. Any light emitted from the conjugate focus A will, after reflection, pass through the second conjugate focus B. Now, let the distance AB be equal to AC, and replace the reflecting surface to the right of AC with a spherical surface of radius AB = AC centered at A. This is shown in figure 3.28B. All light emitted from point A to the left of the line AC will be reflected through point B by the ellipsoidal surface as before. All light emitted from point A to the right of the line AC will be reflected back on itself by the spherical surface and subsequently will be reflected through point B after striking the ellipsoidal reflector. By including a small aperture at B greater than 96% of emitted fluorescent light could be collected. This is not attainable in practice as there has to be a 'waist' for mounting which is shown in figure 3.28C. It should be noted that the chamber design shown in figure 3.28C is of solid construction with the silvered reflecting surfaces on the outsides of the chamber. The radius of curvature of the spherical reflector, centered at A, is slightly less than AB which is the distance between the conjugate foci of the ellipsoid. This is to accommodate the width of the 'waist'. A polished light exit 'pupil' is cut into the spherical surface with centre of curvature at B so that all rays reflected from the ellipsoidal surface are normal to the surface of the pupil. This ensures that the entire system is nonrefracting and hence completely achromatic. A 250 (im x 250 |im square section capillary bore passes through point A to accommodate the cell stream. The chamber depicted in figure 3.28C can be used in either a microscope or laser-based instrument. In the former mode the fluorescence microscope is
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LIGHT AND OPTICS
Figure 3.28. Panel A shows that any light emitted from the primary conjugate focus of an ellipsoid passes through the secondary conjugate focus after reflection. The distance AB is equal to AC and in panel B the ellipsoidal surface to the right of the line AC has been replaced with a spherical reflector of radius AB = AC centered at A. All light reflected to the right of the line AC is now reflected back on itself to strike the ellipsoidal surface and thence passes through the secondary conjugate focus B after reflection by the ellipsoidal surface. Thus 471, all round light collection, is achieved. Panel C shows the final design which incorporates a 'waist' for mounting and polished flats to allow a laser beam to enter. A light exit pupil was cut into the spherical surface which is centered on the secondary conjugate focus to ensure that the whole system is free from refraction and hence is completely achromatic.
FLUORESCENCE
47
focussed to the secondary conjugate focus, point B. As the system relies on reflection it is entirely achromatic, hence all exciting light passing through point B, irrespective of its wavelength, will pass through point A after reflection in the chamber. This gives 'all round' illumination of the objects inflowas they pass through point A. Furthermore, all fluorescent light emitted by the objects as they pass through point A will, after reflection, pass through point B. Thus, the excitation and emission light paths are coincident just as in normal epi-fluorescence microscope applications. In a laser-based system the beam is focussed directly to point A through a polished flat on the mounting 'waist7, and again all fluorescent light emitted from point A will pass through point B to which the light collection optics are focussed. The chamber was mounted on a fluorescence microscope and figure 3.29A shows the coaxial stream of an ethidium bromide solution made up in 5% triton X100 in which the optimum sample flow rate was exceeded by a factor of 10. A magnification objective of x 10 was used to visualize the center of the chamber, which because of its long focal length, could be focussed to the primary conjugate focus of the chamber, point A. A 460—490 nm excitation filter (blue light) was used to elicit fluorescence. The central illuminated volume, from which the 'streak' of fluorescence is being emitted, is clearly visible as too are the side walls of the capillary. The core stream can also be seen in the non-illuminated regions due to the relatively high refractive index of the 5% triton X-100 and the large diameter of the core induced by the 10-fold increase in sample flow rate. The microscope was then focussed to the secondary conjugate focus, point B, which is outside the chamber and from which the cytometric measurements are made. This is shown in figure 3.29B where there is magnification of the image due to reflection from the ellipsoidal surface. The image also appears somewhat blurred and three factors contribute to this. Firstly, at the secondary conjugate focus there are two images superimposed, one is the 'left-to-right7 image reflected primarily from the ellipsoidal surface and the second is the 'right-to-left' inverted image which is reflected from the spherical surface before striking the ellipsoidal reflector. Secondly, the square cross section of the capillary bore at the sheath/quartz interface induces some image degrading refraction; and finally, an image of finite dimension at the secondary conjugate focus is not flat.
3.8
Fluorescence
All biological molecules have the capacity to absorb light which increases the energy state of the molecule above its ground state. The molecule will then revert to its ground state by a number of mechanisms. These include heat dissipation due to an increased number of molecular collisions (the tar on a road melts on a hot day), direct transfer of the excess energy above the ground state to adjacent molecules either with or without attendent chemical alterations and the emission of light with a longer wavelength than that of the exciting light. This capacity to absorb then emit light is called luminescence and molecules exhibiting
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LIGHT AND OPTICS
DD
Figure 3.29. Panel A shows a photomicrograph of the center of the chamber taken with a low power objective which, because of its long focal length, could be focussed to the center of the chamber. DD = 'dark-disk' which is a shadow of the light pupil; CW = capillary wall; IC = illuminated coaxial core from which ethidium bromide fluorescence is being emitted; CR = core reflections from the square section of the capillary bore; NIC = non-illuminated core which is visible due to the relatively high refractive index of the 5% triton X-100 solution carrying the ethidium bromide. Panel B is a photomicrograph of the 'image' at the secondary conjugate focus taken with the same objective as used in panel A. Note the blurring and magnification which is discussed in the main text.
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this phenomenon frequently contain conjugated double bonds in a ring structure. However, not all molecules with this type of structure can emit light, but when this occurs within a short interval of time, usually nanoseconds, the phenomenon is termed fluorescence. When this occurs over a time interval of milliseconds to seconds it is termed phosphorescence. Generally, flow cytometers must take advantage of fluorescence as each cell is only contained within the exciting light beam for a few microseconds at most. 3.8.1
Absorption and emission spectra Molecules absorb light more efficiently at some wavelengths than at others and each has an absorption spectrum. The latter is dependent on molecular configuration, availability of excitable electrons and bond lengths within the structure. The shapes of absorption spectra not infrequently contain local maxima corresponding to those light wavelengths which induce resonance within the molecule or parts of the molecule. In order to obtain most efficient excitation the illuminating wavelength should be chosen to be as close as possible to the absorption maximum or to a large local maximum of each particular fluorochrome. The absorption spectrum of the fluorochrome propidium iodide is shown in figure 330. The maximum absorption occurs at about 490 nm, but there is a convenient local maximum in the UV at 340 nm which can be very useful in flow cy tome try. Absorption of light is a 'quantum' phenomenon and obeys the 'all or none' rule. A given photon either will or will not be absorbed, it's not possible to have part of the energy of a given photon absorbed. However, the efficiency of energy absorption by the molecule is dependent on not only the structure of the fluorophore, but also the orientation of the fluorophore with respect to the photon. A fluorescence photon emitted from a given fluorochrome molecule is always of lower energy (longer wavelength) than that of the exciting photon and is due to a
o
CO .Q CO O)
o
200
300
400 500 Wavelength, nm
Figure 3.30. Absorption spectrum of propidium iodide.
600
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LIGHT AND OPTICS
number of factors. Firstly, the fluorophore, which may be either the whole molecule or just part of a large molecule, may not have the inherent capacity to emit all the energy of the incident photon. This is most likely to occur when the fluorophore is part of a large molecule where non-radiative energy transfer takes place from the fluorophore to the rest of the molecule. Secondly, the absorbed energy may be partly dissipated to the microenvironment molecules adjacent to the fluorophore; and finally, bleaching may occur (see section 3.8.4). If we have a large number of randomly orientated fluorophores excited by a large number of photons we obtain a spectrum of fluorescence energy emissions which, because of the above factors, is a continuum and tends to be log-normally distributed, the general shape of which is shown in figures in section 3.83. 3.8.2
Fluorochromes A large number of biologically interesting fluorochromes exist which may be grouped into three operational categories, namely nucleic acid stains, immunofluorescence dyes and probes for functional activity. Only a short mention of the more commonly used fluorochromes will be given here as fuller details will be covered in the appropriate sections later on. The nucleic acid ligands include DNA-specific, RNA 'part'-spedfic and nonspecific stains. The best example in the last of these subcategories is acridine orange (AO) which has metachromatic fluorescence properties first noted by Meissel (1951) who observed that the nucleus fluoresces green (DNA) and the cytoplasm red (RNA) with the blue light excitation. The use of AO in flow cytometry to measure RNA and DNA simultaneously was pioneered by Darzynkiewicz and colleagues and you will hear much more about this later. Nucleic acid specific dyes include the bisbenzimidazoles (Hoechst 33258 and 33342), chromomycin A3, mithramycin, DIPI and DAPI. The phenanthridinium derivatives, ethidium bromide and propidium iodide, are both non-specific nucleic acid stains and if quantitation of DNA is required the cells must be treated with ribonuclease to remove the RNA. Apart from AO there are three dyes which can be used for RNA. These are thioflavine T, thiazole orange and pyronin-Y. A number of fluorochromes have been used as immunofluorescence probes. By far the most extensively used to date has been fluorescein however, a number of other probes are available. These include texas red, rhodamine, a stilbine derivative (SITS), dansyl chloride, phycoerythrin and allophycocyanin. A new fluorochrome amino-methyl coumarin acetic acid (AMCA) which is UV excited with blue emission has recently been developed (Khalfan et al., 1986) and is now commercially available. Utilization of these stains for immunofluorescence requires that the probe be covalent linking to an antibody. In some circumstances this may alter the fluorescence properties of the fluorochrome. For example, the fluorescence from fluorescein isothiocyanate (FITC) bound to protein is 80% quenched compared with free fluorescein in aqueous solution (Tengerdy, 1965). Arguably, the most exciting group of stains are those which probe for functional activity in viable cells under near physiological conditions. These
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include membrane potential reagents (cyanin and oxanol dyes); fluorogenic enzyme substrates based on fluorescein, coumarins, naphthols, monochlorabimane and resorufin; intracellular pH probes (fluorescein, coumarin and cyanobenzene derivatives) and finally, cytoplasmic calcium probes (Indo-I, Fura-II, Quin-II). 3.8.3
Fluorochrome combinations The shape of 'typical' fluorescence emission spectra with its skew to the right (see figure 3.31) has implications for assays in flow cytometry using multiple fluorochromes simultaneously. Perhaps the commonest such assay involves using fluorescein (green fluorescence) for protein, either directly with fluorescein isothiocyanate or indirectly with an antibody, together with propidium iodide (PI) for total DNA (red fluorescence) a combination first used by Crissman and Steinkamp (1973). Figure 3.31 shows the emission spectra of both fluorescein and PI/DNA excited by blue light together with the spectral windows through which the photodetectors 'see' the respective fluorescence bands intended for them. These windows are produced by splitting the spectrum with a dichroic mirror with 50% transmission at 560 nm which transmits orange/red light and reflects green/yellow. The respective detectors are then additionally 'guarded' by a 515-560 nm band-pass filter (green) and a 630 nm long-pass filter (red). This configuration minimizes the probability of a shorter wavelength 'red' photon (i.e. orange) entering the green photodetector and of a longer wavelength 'green' photon (i.e. yellow) entering the red detector. These probabilities are not zero (see sections 3.5.3 and 3.5.4). There is a small short wavelength tail from the PI/DNA spectrum, arrowed in figure 3.31, which overlaps the green band, and a very small long wavelength tail from the fluorescein spectrum which overlaps the red band. This combination of fluorochromes is used to assay for total DNA and surface
Fluorescein
Propidium Iodide
c
0)
500
650
700
Wavelength, nm Figure 3.31. Emission spectra of fluorescein and propidium iodide excited by blue light (490 nm). Also shown are the spectral 'windows' through which the photodetectors 'see' the respective bands intended for them. On the green channel the band pass is from 515-560 nm and on the red this is > 630 nm. The arrow shows the short wavelength tail from the propidium iodide emission which is included in the 515—560 nm band pass.
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immunofluorescence and the emission spectra plus the band-passes used for this combination, as illustrated in figure 3.31, look very satisfactory. However, figure 3.31 takes no account of the relative magnitudes of the emissions, and the signal from the PI/DNA complex might well be very bright, as DNA is 'abundant7, compared with that from fluorescenated antibody particularly when relatively few target molecules are present on the cell membrane. This is illustrated in figure 3.32 where the PI/DNA fluorescence emission has been increased by a factor of 15 compared with figure 3.31. The total emission reaching the photomultiplier now contains a considerable component (stippled) due to PI/DNA fluorescence. This breakthrough represents the 'background' above which the true green signal from fluorescein has to be measured. A method which partially compensates for this effect is given in section 4.2.3. The combination of fluorescein and propidium iodide, as mentioned in the previous paragraph, usually presents few problems. However, if we were to perform the same assay as depicted in figure 3.32 using the vital DNA stain Hoechst 33342 we would run into considerable problems quite apart from the requirement for two excitation wavelengths. The emission spectra for Hoechst 33342 stained DNA and fluorescein, comparable to those for PI/DNA plus fluorescein of figure 3.32, are shown in figure 3.33 together with the same bandTotal emission
a) c 0)
Propidium iodide emission
Fluorescein emission
500
550
600
Wavelength, nm Figure 3.32. The magnitude of the fluorescence from the propidium iodide/DNA complex has been increased by a factor of 15 compared with figure 3.31. The total emission now being collected through the 515—560 nm band-pass filter contains a significant fluorescence contribution from the propidium iodide/DNA complex indicated by the stippled area.
FLUORESCENCE Hoechst 33342
400
450
53
Fluorescein
500
550 Wavelength, nm
600
650
Figure 3.33. A similar illustration to that infigure3.31 except that Hoechst 33342 has been used for DNA instead of propidium iodide. The DNA signal breaking through into the green channel is relatively much greater than the comparable breakthrough in figure 3.31. If the Hoechst 33342/DNA emission were to be increased by a factor of 15 as infigure3.32 the green emission from fluorescein would be completely swamped. pass region required for fluorescein analysis. The emission spectrum from Hoechst 33342/DNA is very wide and overlaps the latter to a considerable degree. Clearly, the green 'background' fluorescence signal for this combination of fluorochromes is very much greater than for the combination of fluorescein and PI. If we wished to perform such an assay, for instance in live cells, using Hoechst 33342 for DNA and a surface marker simultaneously it would be better to probe the latter with a red fluorophore to reduce the spectral overlap. However, with immunofluorescence amplification of fluorescein and special adjustments and modifications to the laser it is possible to use this in combination with the Hoechst dyes; see section 12.1. The design of assays using combinations of fluorochromes must take into account the total quantity of fluorescence being emitted by each fluorophore as well as their spectral separation. In general, the combination should be designed to measure the fluorophore with the greatest absolute quantity of fluorescence at the longer wavelength as the long wavelength tail tends to be of greater magnitude and extent than that of the short wavelength due to the log-normal shape of the emission spectra. A further method of overcoming fluorescence emission spectrum overlap, which can only be used with multi-beam excitation, is to illuminate each cell sequentially. This system was introduced by Shapiro et al. (1977) where light scatter and fluorescence measurements were made from each cell at three interrogation stations, each with a different excitation wavelength, separated by 100 Jim. This type of system has also been developed by Steinkamp et al. (1982) and by Lebo et al (1987), and Crissman et al (1985a, b) have used their triple sequential illumination systems to analyse DNA, RNA and protein simultaneously (section 12.2). This technique, with two beams, has also been used in chromosome analysis (see chapter 13) and for three colour immunofluorescence studies (Loken and Lanier, 1984; Lanier and Loken, 1984; Parks, Hardy and Herzenberg, 1984).
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3.8.4
Quenching and resonance energy transfer Quenching is defined as a reduction of fluorescence yield due to loss of the absorbed excitation energy by any pathway other than light emission. This includes bleaching where there is a sufficient chemical modification of the fluorochrome structure to destroy its fluorescence properties. If the energy of a second photon is absorbed by a molecule in the excited state before it has discharged the energy absorbed from a first photon then a number of changes can occur. These range from complete disruption of the molecule with the formation of two or more new species, photolysis, to more minor alterations in electronic configuration. The latter are usually reversible as far as fluorescence is concerned and everyone who has used a fluorescence microscope will have observed the bleaching of fluorescein fluorescence and its recovery after the illumination is turned off for a few minutes. Resonant energy transfer is a term for a particular type of quenching where the excitation energy absorbed by one molecule is resonantly transferred to a second molecule. This is a non-radiative process and the first molecule, the donor, returns to its ground state leaving the second molecule, the acceptor, in an excited state which can then revert to the ground state by any of the mechanisms available, including light emission. Two conditions must coexist for this process to occur. Firstly, the emission energy spectrum of the donor must overlap the absorption spectrum of the acceptor and secondly, the molecules must be very close to each other. The efficiency of resonance energy transfer is inversely proportional to the sixth power of the distance between molecules and very little energy can be transferred beyond 60-70 angstroms (Shyer, 1978; Jovin, 1979).
3.9
Excitation
Due to the relatively small number of fluorescent molecules per cell and the short time that each cell is exposed to the exciting light it is necessary to achieve very high light fluxes at the intersection of the cell stream with the illumination. A high light flux means that a very large number of photons are passing through a small volume of space, remembering of course that the focus of a lens is not a point. This light flux requirement at the focus is obviously generated at the source of illumination which must be as small as possible and as bright as possible. Furthermore, light losses through the optical system, which transmits the light from source to object, must be minimized. 3.9.1
Source size The light source has to be small because of lens focussing characteristics, which were discussed in relation to point sources in section 3.3. However, with conventional illumination the source size isfiniteand is focussed to afiniteimage in the focal plane. This is depicted in figure 3.34 where three rays are emmanating from point A and passing left-to-right from the arrow head of the source (object)
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Figure 3.34. Representation of the focussing of a finite light source image in the focal plane of a lens.
which is at a height hx from the optical axis. Ray oc is parallel to the optical axis before encountering the lens which, after refraction by the lens, passes through the 'back' focal point, f2. Ray (3 passes through the center of the lens without focussing refraction (this is a 'thin' lens) and the third ray, y, passes through the 'front' focal point, iv and is refracted parallel to the optical axis on emerging from the lens. These three rays converge to point Z to form an inverted image of the source which is smaller than the source and of height h2 from the optical axis. Moving the object further to the left will decrease the size of the image and bring its focal plane closer to the 'back' focal point, f2. In theory, therefore, it is possible to distance the source from the lens to such an extent that the image is effectively a point. However, the quantity of light that can be collected by the lens decreases as the square of the distance of the source from the lens (it's that man Newton again, 1687) and we need as much light as we can get. Thus, there is a trade-off between the amount of light we can collect and the size of the image we can obtain. In practice we can only achieve effective 'compression' of the image down to about j^- of the object size. With finite sources the output from the source has to be collected, frequently using a back reflecting mirror to increase the number of photons captured, then collimated by a lens system before it is focussed. However, even with a back reflecting mirror only between about 10 and 20% of the light emitted from a finite source can be collected for the reasons given above and for those considered in section 3.6. 3.9.2
Source brightness It is obvious from the preceding section that the light source must be as bright as possible. The quantity of electromagnetic irradiation emitted from an incandescent source is directly proportional to its temperature, but the wavelength is inversely proportional to temperature. The inverse relationship of the latter is due to the fact that photons of longer wavelength are of lower energy than those of shorter wavelength. In order to obtain sufficient higher energy
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photons (UV, violet and blues) to be useful in flow cytometry an incandescent source must be very hot, in the region of 6000 K, and the majority of the energy radiated from such a source is emitted as heat. The latter must be disposed of, which requires heat-reflecting/transmitting mirrors in the light collection system. Generally, it doesn't matter which light source is used as long as it is 'small7 and it generates sufficient light of the required wavelength.
3.9.3
Conventional sources
The filaments of quartz-halogen lamps are relatively large, measuring about 1.0 mm x 3.0 mm, and even with the very best microscope objectives it is not possible to focus the light from these sources to small enough spot sizes for flow cytometry and further problems arise. Firstly, the light output is not constant over the whole of the filament area, which is usually constructed as a rectangular section coil. The light output from the hot wire of each turn of the coil is relatively
TYPICAL OUTPUT SPECTRA 100
O C
.2 CO
CO
o
a
0.001 300
400
500
Wavelength (nanometers) Figure 3.35. Light emission spectra of deuterium, xenon and mercury arc lamps between 300 nm and 550 nm. Redrawn from the Oriel Corporation catalogue.
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high but this is low between the turns which gives rise to alternating high and low intensities across the coil area. Secondly, the brightness of filament sources, which are not really very bright, is limited by the melting temperature of the filament material. Finally, a back-reflecting mirror is not effective as the filament obscures the back reflected light. The source sizes in arc lamps can be as little as 250 |im x 250 (im, which is sufficiently 'small' to be used in flow cytometry. They are also inherently brighter than filament sources as the temperature in the center of the arc, which doesn't contain anything that can melt, is considerably higher than can be obtained with filaments. Deuterium, xenon and mercury arc lamps are available and their light emission spectra between 300 nm and 550 nm, the region of maximum interest in flow cytometry, are redrawn from the Oriel Corporation catalogue in figure 335. Clearly, mercury arcs have the advantage, particularly as these have powerful emission lines in the UV to low blue region of the spectrum although there is little to choose between mercury and xenon in the high blue region. Deuterium is a nonstarter. 3.9.4
Lasers The best illumination source is undoubtedly the laser for a number of reasons. Firstly, the light is very bright. Secondly, the beam emitted by a laser is coherent which means that the light is polarized, the photons are all 'in step' and the beam is essentially parallel. This last attribute means that the 'effective' spot size of the illumination source is very small, tending to a point, as the beam is parallel and appears to be coming from infinity. Referring to figure 3.34 we can see that the three rays a, (3 and y are all approaching the lens at different angles. In a laser beam all rays are parallel to the optical axis, thus they can be focussed to very small spot sizes. Finally, they give a more stable output than more conventional sources. This is essential for quantitative studies and most lasers can be stabilized to within + 1 % over many hours of continuous operation. However, they do have a number of disadvantages including cost. Moreover, a laser will generally emit at only one well defined and specific wavelength at time, although tuning to a number of individual wavelengths from UV to red is possible depending on the type of laser being used. This is a considerable disadvantage if two fluorochromes with very different absorption spectra need to be investigated simultaneously as the only totally satisfactory solution is to use two lasers. Dye lasers, pumped by
Table 3.2. Lasing lines for argon, krypton, helium—neon and helium—cadmium lasers Laser Argon Krypton He-Ne He-Cd
Lasing lines, nm 351 363 457 465 476 488 501 514 528 337 356 406 413 56S 657 676 543 594 632 325 441
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part of the output from a medium to high power laser, can be tuned within a given wavelength range (Arndt-Jovin, Grimwade and Jovin, 1980). However, it is not possible to stabilize fully both the pumping and the dye laser simultaneously. Table 3.2 summarizes the excitation lines available from the commonly used lasers.
3.9.5
Beam and focussing geometry
The beam from a laser can assume various so-called Transverse Emission Modes, or TEM for short, which depend on a number of factors including plasma tube construction and mirror alignment. These modes are subscribed as 00,01,01*, 10, 11 etc., depending on the segmentation of the beam and the first three are shown in figure 3.36. The intensity of the beam is Gaussian distribution in TEM00, which is depicted in figure 3.37. It is convention to describe the width of a beam as the diameter across the beam where the irradiance falls to 0.1353 of that at the peak. This might seem to be a funny number to choose but it is the numerical value of 1/e2. Let us now assume that a typical 1.2 mm diameter beam is focussed down to a 50 |im diameter spot at the 1/e2 irradiance width and that a core stream diameter of 15 |im containing 10 |im cells is passing through the center of the focussed beam in the most intense section. This is depicted in figure 3.38 with two cells, A and B, in the center and at the periphery of the core respectively. Cell A, in the ideal position, has a 6% variation in light intensity across it. Cell B, in the worst position at the core periphery, suffers a 15% intensity variation. We can now see that very minor instability in the core position, of as little as + 2 urn, could make profound differences to the illumination intensity experienced by individual cells. With this degree of core instability the variation could easily amount to 40%, as depicted in figure 3.38 which is a reasonable to-scale representation of the reality. Two options are available to overcome this potential variation in illumination intensity. Firstly, a larger spot size could be used to 'spread out' the highest intensity region with respect to the core, but this also reduces the light flux which is not desirable. The second is to use a crossed cylindrical lens pair as described in section 3.3. With this option the focal spot is compressed from top-to-bottom to form an oval sheet. The intensity profile is still Gaussian distributed in which ever
TEM
00
01
01*
Figure 3.36. Illustration of the segmentation of a laser beam in various Transverse Emission Modes.
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1.0-
0.135-
Figure 3.37. The light intensity profile across a laser beam is Gaussian distributed in TEMOo- The width of a beam is defined as the diameter across the beam where the irradiance falls to 1/e2 of that at the peak.
50/x
Figure 3.38. A 15 jim diameter core passing through the center of the focussed Gaussian beam in the most intense section and containing two 10 |im cells. Cell A, in the ideal position, has a 6% variation in light intensity across it. Cell B, in the worst position at the core periphery, suffers a 15% intensity variation. Core position instability of as little as + 2 (am could give rise to a 40% illumination variation. radial plane the beam is 'sliced' but the standard deviation is 'tightest' in the vertical plane. Figure 3.39 shows a representation of the focal spot intensity obtained with a crossed cylindrical lens pair which 'spreads' the beam to 150 |im horizontally together with a 15 Jim diameter core directly analogous to that in figure 338. The potential variation in light intensity across a plane of a 10 |im cell is now less than
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Figure 3.39. Crossed cylindrical lens pair illumination with compression of the focal spot from top-to-bottom to form an oval sheet 150 |lm wide and 4—7 Jim deep. A 15 jim diameter core containing two cells, directly analagous to that in figure 3.3S, is shown and the potential variation in light intensity across a 10 Jim cell is now less than about 2% and there is now considerable latitude for any core positional instability.
about 2% and there is now considerable latitude for any core positional instability. Also, for a given beam power the light flux tends to be greater than with a circular spot.
3.9.6
Pulse shape
The type of focussing system used has a large influence on the electronic design due to the different shapes of the fluorescence intensity profiles from the two systems. With a single spherical lens the focal spot is circular and must be considerably larger than the objects being interrogated (see previous section). This means that the cell can be completely contained within the focal volume and the peak height of the intensity profile as the cell passes through the beam is directly proportional to fluorochrome content. However, with a crossed cylindrical lens pair the cell is not completely contained within the beam and the integrated area of the whole of the intensity profile must be quantitated to obtain proportionality with total fluorochrome content. In practice it is usual to record not only the pulse area, but also the peak height, which is proportional to maximum fluorochrome concentration, together with the time-of-flight through the beam, which is proportional to the diameter of the cell plus the width of the beam. Hence, more data are obtained with the crossed cylindrical lens pair. The fluorescence intensity profiles obtained with the two systems are compared and contrasted in figure 3.40.
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Entry
Exit
TimeIntegrated area
Figure 3.40. Comparison of fluorescence intensity profiles obtained with spherical lens (top) and crossed cylindrical pair focussing (bottom). At the top the cell is completely contained within the beam and pulse height, P, is proportional to the total quantity of fluorescence. At the bottom the cell is not completely contained within the beam and integrated area under the pulse is proportional to total fluorescence. The time-of-flight through the beam (pulse width, W) is proportional to cell diameter plus the width of the laser beam and pulse height, P, is proportional to peak concentration.
3.10 Scattered light Theoretically, Maxwell's equations of electromagnetism (1891) could be solved to describe the propagation of light scattered by objects of any size and refractive index. In practice, exact solutions have only been worked out for particles much smaller than the wavelength of the illuminating light (Rayleigh, 1871) and uniform spheres which approximate to the sizes of cells (Mie, 1908). No satisfactory solutions have been found for the reality of real cells which present almost insuperable problems for the theorist. Scatter depends on a number of optical processes including diffraction, reflection, refraction, and Rayleigh scattering. In a biological cell these optical processes in turn depend on total size, refractive index of the medium, the number of dielectric interfaces within the cell (granularity) that the wave-front passes through plus their sizes, light wavelength and angle of observation. Furthermore, any intracellular refractive index changes may also give rise to both constructive and destructive interference. Clearly, light scatter from intact cells is extremely complex and consequently ill-understood; however, under specific conditions, it can give information about cell size and some morphological data which is low resolution at present.
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3.10.1 Diffraction An opaque particle in a beam of light, which is large compared with the light wavelength, will absorb the light incident upon it which creates a 'hole' in the wave-front. Each point on the circumference of this 'hole' in the wave-front will act as a focus for secondary irradiation (Huygens' principle). The diffraction pattern of 632 nm light (helium-neon) produced by a circular disk corresponding to a 10 urn sphere suspended in medium with refractive index of 1.33 is shown in figure 3.41. This is similar to the pattern shown in figure 3.14 and diffraction is the dominant contributor to light scatter at narrow forward angles. 3.10.2 Reflection and refraction Both of these phenomena contribute to the total quantity of light scattered from an object into a detector at any given angle. The exact magnitudes of their respective contributions from unstained cells are not known. However, cells stained with immuno-gold scatter very large quantitities of light to 90° but their forward scatter characteristics are similar to unstained cells. Very granular cells, e.g. polymorphonuclear leucocytes and macrophages, also exhibit large scatter signals to 90° and it is now generally accepted that reflection and refraction play a major role in scattering light to larger angles. 3.10.3 Anomalous diffraction Diffraction described in sections 3.4 and 3.10.1 considered opaque objects in the path of the light beam where there were large differences in refractive index encountered between two media (screens with slits and opaque objects). With biological material the refractive index difference between the supporting medium (water or saline) and the object of interest is frequently small. Anomalous diffraction is a term which describes interference due to a phase shift induced by an effective path length difference when an object is large compared with the incident light wavelength and where the refractive index difference is small. The phaseshifted wave on emergence from the object then interferes with the wave passing round the object to give rise to a scatter pattern. 3.10.4 Rayleigh scattering This term is applied to particles, such as macromolecules or small organelles which are smaller than the wavelength of the incident light. The latter causes displacement of atomic charges in the particle with the induction of a dipole which oscillates in phase with the illuminating light. This oscillation now acts as a point source which re-irradiates light in all directions. All of these processes will contribute to the amount of light scattered into a detector at any given angle. Brunsting and Mullaney (1972) have compared the total light scattered by Chinese hamster ovary (CHO) cells at various angles with homogenous and coated microspheres, and their data are reproduced in figure 3.42. Up to an angle of about 7.5° all three types of objects gave very similar
SCATTERED LIGHT
63
10
10
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Angle (degrees) Figure 3.41. Diffraction pattern of 632 nm light (helium-neon) produced by a circular disc corresponding to a lOjlm sphere suspended in medium with refractive index of 1.33. Redrawn from Salzman et al., 1979. This is similar to the pattern in figure 3.14.
results which were compatible with diffraction making the dominant contribution. At angles greater than 7.5° the CHO cells gave results, compatible with Mie theory, that were between those from the artificial objects. The major problem with biological material is the non-uniformity. Scattered light in the forward direction seems to be dominated by diffraction (regular and anomalous) at the medium/cytoplasmic and cytoplasmic/nuclear interfaces. Light scattered to 90° tends to be related more to the number of dielectric interfaces through which the photon passes and to the magnitude of those changes in refractive index. Thus, 90° scatter is more related to reflection and refraction from intracellular structures though diffraction and Rayleigh scattering will also contribute. It has become part of the dogma of flow cytometry that forward light scatter is proportional to particle size. In most cases this is true, but the exact position of the detector in relation to the particle, the light collection angle, type of flow chamber and focussing system used, the laser wavelength and illuminating power as well as the composition of the particle can all influence the total quantity of light scattered
LIGHT AND OPTICS
64
c 0
103-
10
5
10
15
20
25
Scattering angle (degrees) Figure 3.42. Comparison of the total light scattered by Chinese hamster ovary cells (heavy solid line) at various angles with homogenous (dashed line) and coated microspheres (light solid line). Redrawn from Brunsting and Mullaney, 1972. Up to an angle of about 7.5° all three types of objects gave very similar results which were compatible with diffraction making the dominant contribution.
into the detector. Some of these points, which will be considered further in chapter 10, demonstrate that forward light scatter should not be related indiscriminately to the size of a particular cell or cell type unless this has been proven to be true by an independent method. However, although there is room for considerable improvement in our theoretical interpretation of both forward and 90° light scatter these measurements can give valuable information (see chapter 10) even though the theory is still poorly understood in the reality of the biological system.
4 Electronics
4.1
Photodetectors
Photodetectors are light-sensitive devices which proportionally convert light energy (photons) into electrical energy and they fall into two categories. 4.1.1
Photomultipliers In photomultipliers the incident photons strike the photocathode which then emits electrons in direct proportion to the number of photons striking the cathode. This is the point at which the light flux is transduced (changed) into the electronic signal. The electron flux emitted from the photocathode is then amplified through a dynode chain within the photomultiplier to produce a current. There are now literally hundreds of different varieties of photomultiplier tubes. They vary in their photocathode material and construction, their 'windows' through which the light passes before striking the photocathode and in their dynode chain construction. Different photocathode materials and construction have different sensitivities to light of different wavelengths. Typically, the S l l and bialkali tubes are relatively more sensitive in the high UV, violet, indigo, blue and through to the green. The S20 tubes are relatively more sensitive to the lower energy wavelengths, namely the yellows, oranges and reds. In order to obtain the greatest efficiency for the conversion of light into electrons the photomultiplier should be chosen to be maximally sensitive to the particular wavelength band that is to be measured with that particular photomultiplier tube. For example, it makes no sense to use an S20 tube with an extended red response to measure violet and blue light, and equally, it makes no sense to use an S l l tube to measure red light. Quartz transmits UV light much more efficiently than optical crown glass and photomultipliers which are required to quantitate UV and violet light should be equipped with quartz windows. All photomultipliers require a high tension voltage between the cathode and anode. Typically, there will be a potential difference of approximately 100 volts between each dynode within the amplifying chain inside the photomultiplier. Thus, a 10 dynode chain tube will require a high tension supply of at least 1000 volts which has to be very stable.
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ELECTRONICS
4.1.2
Solid-state devices The second type of detector is the solid-state device. These differ from photomultipliers in that they generate a current when they are illuminated and do not need a high tension supply. Generally, they are less sensitive than photomultipliers and they too tend to have a spectral response being more sensitive towards the red end of the spectrum. Solid-state detectors have been developed that approach the sensitivity of photomultipliers but these, the charged coupled devices, require cooling to liquid nitrogen temperatures and they are not yet a regular feature within the flow cytometry field.
4.2
Signal processing and amplification
The current generated by the photodetector will be within the range of a few tens of microamperes and contains three components. The first is due to any background light entering the detector which is not directly associated with the measurement being made. The second is 'dark-current' generated within a photomultiplier which varies not only with the high tension voltage across the PMT, but also with its temperature. Each of these components contributes to a background current and the various factors giving rise to this 'noise' will be discussed in section 9.1. The third component of the current is due to the specific signal we wish to measure. The first step in signal processing is to convert the output current from the detector into a voltage which is then amplified. This is often a two-stage procedure with a pre-amplification step in which the electronics frequently contain circuitry to 'iron out' any fluctuations in the base-line voltage. The second amplification step may be carried out with either linear or log amplifiers and there is always a finite upper limit to the amplified voltage which is usually either 5 or 10 volts. 4.2.1
Linear amplifiers The output signal from a linear amplifier is directly proportional to the input signal where the output is larger by a defined quantity for each particular amplifier, the gain, with respect to the input. In some instruments the gain of linear amplifiers can be varied with implications for the measurement range; see section 9.3. Let us suppose the amplifier has a maximum output of 10 volts which is directed through to a voltmeter with a scale of 1 to 1000. The 10 volt maximum signal will have a scale reading of 1000 and signals of 5.0 and 2.5 volts would appear on the scale at 500 and 250 respectively, i.e. the response is linear. 4.2.2
Log amplifiers Log amplifiers were introduced to increase the dynamic range within the instrument and they operate on logarithmic scales of either 3 or 4 decades. If we take a 4 decade log amplifier with a 10 volt maximum output and again feed the output into our voltmeter we will still get a scale reading of 1000 for 10 volts
SIGNAL PROCESSING AND AMPLIFICATION
67
1000-1
Input
Figure 4.1. Comparison of the outputs from linear and log amplifiers.
output. However, as this is a 4 decade amplifier each 10-fold decrease in the input signal will give an amplified signal which decrements the maximum output range by \. Thus, input signals which are amplified to 1.0, 0.1 and 0.01 volts will give voltmeter scale readings of 750, 500 and 250 respectively. A comparative representation of the outputs from a linear and a log amplifier are shown in figure 4.1 where the input is in millivolts and the output is in volts x 100. Figure 4.2 compares histograms obtained with each type of amplifier. Log amplifiers are designed to 'expand7 the smaller signals which in turn 'compresses' the larger signals. However, we have to question the logic of using a 4 decade log amplifier. Let us suppose that the maximum output current from the photodetector is 20 \iA and that during the voltage conversion and amplification steps this is converted to the 10 volt maximum output signal. A 4 decade log amplifier gives a range of 104 which means that the minimum output current from the photodetector would be 20 x 10" 4 |iA which is 2 nA. Thus, the current input to the log amplifier over the first amplification decade would be in the range 2 nA
6$
ELECTRONICS
Linear amplification
Fluorescence intensity
Figure 4.2. Comparisons of histograms obtained with log and linear amplifiers. to 20 nA, and 20 nA would give a scale reading of 250 on our voltmeter. It is doubtful if circuitry can be built, without cooling to liquid nitrogen temperatures, with current noise levels less than 20 nA. This means that the first 250 divisions on our voltmeter are only likely to contain electronic noise from a 4 decade amplifier and hence are 'wasted'. There seems to be little point, therefore, in going beyond a 3 decade log amplifier. 4.2.3
Differential amplifiers Differential amplifiers, also known as compensators or linear subtraction devices, are designed to correct for breakthrough of fluorescence from one fluorophore into the analysis window of another and to reduce noise (Steinkamp, 1983). Examples include fluorescein (green) into the orange/red photomultiplier quantitating light from rhodamine or phycoerythrin fluorescence and propidium iodide DNA fluorescence (red) into the green detector quantitating fluorescein. Figure 4.3 shows an example of the last of these where propidium iodide stained DNA (red fluorescence) was being scored on the abscissa versus a fluorescenated monoclonal antibody probed nuclear associated antigen (green) on the ordinate. The monodimensional histograms associated with the two measurements are shown adjacent to the respective axes. These data were from a control sample where panels A and C represent the PBS controls (nofluorescein)and where panels B and D were obtained with added second antibody (fluorescenated) but no first antibody. The instrument was set up to record the Gl DNA peak in panel A at channel 200 on the abscissa. The gain on the green channel was then increased so that the short wavelength tail from the PI/DNA emission spectrum broke through
SIGNAL PROCESSING AND AMPLIFICATION
69
Figure 4.3. Breakthrough of the short wavelength tail from propidium iodide stained DNA (red fluorescence) into the green channel, panel A. This has been compensated for in panel C. Panels B and D show comparable data for a fluorescence control sample containingfluorescenatedsecond antibody but no first antibody. the green band pass filter to record the Gl peak at about channel 25. Clearly, there is a direct relationship between the two measurements. In panel B there is a slight increase in the green signal due to non-specific binding of the fluorescenated second antibody. Compensation was carried out on the data of panel A and the result of this is shown in panel C. The same compensation was also carried out on the data in panel B and these results are shown in panel D which is the background signal above which and subsequent specific green signal due to first antibody binding would have to be measured. Figure 4.4 shows a schematic of the processes involved in a differential amplifier
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ELECTRONICS
to correct for this artefact. In this example we are compensating on the green channel for red breakthrough. The red signal (pulse B) is input to a proportional pulse divider (PPD) which gives two output pulses, C and D. These always sum to the value of the input pulse but the ratio of the outputs can be varied and pulse C which will be used for the compensation, is adjusted to be the same size as A, the green background signal. Pulse C is now amplified by a factor of 2 and divided equally into two (AD). This gives two output pulses (E and F) each of which is the same size as the input pulse C. One of these pulses, F, is now added back to the divided red pulse D (PA) which restores this to its original size, B. Compensation on the green channel is effected by inputting pulse E into an inverter (PI) which turns it upside down to give the inverted output pulse G. This is now added to the green input pulse A (PA) to give an output of zero.
Figure 4.4. Block diagram illustrating the processes involved in differential amplification to correct for breakthrough from one channel into another. In the example of a control sample (figure 4.3) the background signal in the green channel due to red, PI/DNA, breakthrough has been eliminated; however, there has been no change in the DNA histogram, red signals.
4.2.4
Triggering and thresholds
The electronics are designed so that signal processing only begins at a set voltage, or threshold, above the background base line level. This is important as there has to be some criterion which sets the electronic wheels in motion and tells them when to start turning. You cannot have the electronics in action all the time as you would never be able to discriminate between rubbish, random fluctuations and reality (cells hopefully). This is illustrated in figure 4.5 with two pulses, one of which triggers the system at voltage T, whereas the other, which does not reach voltage T, does not. It is also important to be able to specify a master triggering channel, particularly for multi-parameter work (multi-parameter in this context means more than one), which is capable of controlling the electronic initiation and examples are given in section 9.1.1.
SIGNAL PROCESSING AND AMPLIFICATION
71
Scored
Not scored
Time—• Figure 4.5. Illustration of triggering. The signal from an object must exceed a voltage T in order to start the electronics. The triggering voltage threshold, and the way in which this is set, must also be considered in relation to the use of log amplifiers. The threshold can be set either in analogue by a potentiometer, which is essentially continuously variable, or digitally via computer. If digital settings are used these will be of either 8-bit or 10-bit precision giving 256 or 1024 digitization steps respectively. If the full output range of the amplifier (10 volts) is used for threshold setting then each step will be either 39.06 mV or 9.76 mV respectively with 8-bit and 10-bit precision. This means that only a 2 log order amplifier could be used with 8-bit precision threshold setting where this covers the whole voltage output range of the amplifier. However, with 10-bit precision we could use a 3 decade log amplifier. This problem with digital setting can be solved by restricting the upper limit of the threshold voltage range to a fraction of the maximum output from the amplifier. In practice, if this range is set to 1 volt then a 3 decade log amplifier could be used with 8-bit precision digital threshold setting, but this does require that there are never any noise signals above 1 volt. This is reasonable as, if there are noise signals above 1 volt, then it will be obvious by simple inspection that the specimen is of such terrible quality that it should never enter the instrument; however, you do get them occasionally. These types of problems should not arise with potentiometer setting. 4.2.5
Sequential illumination triggering Life gets a little more complicated if signals are being elicited from two beams sequentially. In this case it is important to trigger the system on a signal from the first beam (often scatter). If you use a parameter from the second beam as the master, the electronics will not have known that they should have started working as the cell passed through the first beam and you will have lost those data. This can be overcome if you have an instrument equipped with sophisticated 'delay' electronics, but this is not a regular feature. Moreover, it is also important to
72
ELECTRONICS
disable the triggering from the first beam until the cell has passed through the second beam. Ideally, a scatter signal from the second beam, which unlike fluorescence signals will always be present, should be used to signal that the cell has passed the second analysis point.
4.3
Analogue-to-digital conversion
The amplified signal at this point is still in analogue form. It now has to be converted to a whole number which can then be stored electronically. The analogue-to-digital converter (ADC) has a fixed range, and in flow cytometry this is usually from zero to 255 inclusive or from zero to 1023. These respectively are termed 8-bit and 10-bit resolution ADCs. A description of the workings of an ADC is not in order here but it is important to know that these can be set up relatively arbitrarily. Thus, the origin can be offset either to the left or right. Furthermore, they can also be set to ignore any signals greater than their maximum be this 255 or 1023. The latter is not good practice and any signals of 255 and above in an 8-bit ADC should be scored as 255. Equally, with a 10-bit ADC any signals equal to or greater than 1023 should be scored as 1023 and not ignored. It is not generally appreciated that any instrument in which an analogue-todigital conversion step is used will introduce a positive skew into the distribution of the parameter being measured. Thus, if a given signal in a 1024 ADC is scored with a value of 100 we need a minimum increase of 1% in another signal for it to be scored as 101. However, if a signal has a value of 1000 we need an increase of only 0.1% for a second signal to be digitized as 1001. Thus, the resolution increases with the magnitude of the signal. The effect on standard deviation (SD) of a distribution is as follows. Consider a distribution with a standard deviation of 5 and mean of 100. The coefficient of variation (CV), which is defined as the ratio of the SD to the mean (see section 9.4), is equal to 0.05. For a second distribution with SD of 5 and mean of 1000 the CV is 0.005. If, however, the first distribution (mean= 100, SD = 5) had been recorded with the photodetector gain increased by a factor of 10 then the mean would appear in channel 1000. A cell previously recorded in channel 101 would now appear in channel 1010. Hence, the SD would be 50 and the CV is constant and maintained at 0.05. However, there is a limitation to the constancy of the CV. Consider a distribution with mean of 100 and CV of 0.5%. About 70% of the distribution would be scored in channel 100. However, if this same distribution had been scored in channel 10 the whole of the distribution would have been scored in that channel and the CV would be about 2%. Thus, the CV is only constant above the point at which the ADC step can resolve the dispersion in the distribution. A practical example obtained with microbeads is shown later in figure 9.11. If there is a large spread (CVs > 0.2) in a measured parameter from a population the distribution will cover a large proportion of the digitization steps in the ADC.
ANALOGUE-TO-DIGITAL CONVERSION
73
Thus, cells which elicit a small response will have a smaller local SD than those cells with a large response which introduces an artefactual positive skew into the recorded data. This also applies to data sets with relatively low CVs but in these cases the effect is less apparent.
4.4
Data capture
The original light pulses from the detector have now undergone a number of transductions and transformations from a photon to an electron flux, thence to a voltage which was amplified and threshold filtered, and in turn the filtered pulse was digitized into an electronic whole number which now has to be stored. These electronic numbers are the data. 4.4.1
Buffering The first step in the storage process involves placing the data in a FIFO (First-In-First-Out) buffer. This is a fast operation which is carried out in hardware under assembler language control. As this is a faster process than some of the subsequent manoeuvres it is usual to have two FIFOs. When the first buffer is full the data stream is immediately diverted to the second buffer and while the second is being filled the first is emptied.
4.4.2
Dedicated memory
The data can now be read out of the buffer and stored within assigned hardware memory locations. This type of storage should only be used for monodimensional histograms as the overheads in terms of storage requirements become prohibitive even for two-dimensional correlated data with 10-bit resolution, see section 5.2. However, dedicated memory storage does have the advantage of almost instantaneous recall and display.
4.4.3
List-mode
List-mode data collection means that the data are stored on computer disk in a long sequential list in the order in which they entered the FIFOs. The list is carefully structured so that the data from the first cell are stored sequentially before those from the second cell. If, for example, we are collecting data from four detectors and digitizing pulse height, integrated area and pulse width from each detector we will have three units of data from each of the four detectors giving a total of 12 units of data. It doesn't matter in which order these various data are stored as long as they are stored in the same order for each cell and that the data from sequential cells do not get mixed up. Recalling data from list-mode storage is slower than from dedicated memory but there is much more information as there are all the cross-correlates; see sections 5.33 and 5.3.4.
5 Computing
Computing procedures in flow cytometry, particularly for multi-parameter analysis, are becoming increasingly sophisticated. Developments are taking place rapidly and a number of packages, independent of the large organizations (Beckton—Dickenson and Coulter), are becoming available commercially. The every-day user of the technology is increasingly at the mercy of the packaged product menu and many of these, be they from large or small organizations, have limitations. This section is included to familiarize the totally uninformed reader with the most basic vocabulary and computing processes so that if you have to request, complain or argue about something with a supplier you will at least have some idea of what the words mean. Anyone who knows all about bits, bytes and binary should skip the next subsection. If you also know how to process eightdimensional data, manipulate six-parameter data, display three-dimensional data in stereo, perspective and in colour and assess distribution shapes with 28K addressable memory using a micro-processor then skip all these subsections and G O T O cell sorting.
5.1
Bits, bytes and binary
In order for the non-informed to understand some of the processes involved we must start with some definitions, a respresentation of how numbers are stored by a computer and a description of how some of the operations are carried out. A storage location is called a word. That wasn't too difficult was it? Remember I'm writing for biologists. Generally, a word contains 16 bits, which is equivalent to 2 bytes and it doesn't take the greatest intellect in the world to appreciate that there must be 8 bits in a byte. I'm not being patronizing; it took me some time to become totally familiar with all this, and for those who know nothing about these things (you are the only ones who should be reading this section) there is nothing more complicated than that to follow. A 16-bit word can have any integer (whole number) value within the fixed range of — 32 768 to + 32 767 inclusive. This is called an INTEGER*2 word where the "21 indicates the number of bytes and it is the standard integer word length for 16-bit computers. If we want to handle either integers with values outside this range or non-integers which contain a decimal point we have to use 32-bits of
BITS, BYTES AND BINARY 1 5 14 1 3 1 2 11 1 0
CM
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00
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(0
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00
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9
8
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00 CM
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Figure 5.1. A representation of a 16-bit word where the bit-number, starting from the right, is shown above its respective bit.
store. These are the so called REAL*4 words which contain 4 bytes. In the newer generation of 32-bit micro-computers the standard integer word length is INTEGER*4 (4 bytes) which gives a whole number range of—2 147 483 648 to + 2 147 483 647 inclusive. This feature is also an option in some 16-bit computers with more modern operating systems and computer languages (e.g. FORTRAN 77, PASCAL and 'C). It is also possible to declare variables as REAL*8 in all languages, and the storage assigned for such variables will be 8 bytes which is 64 bits. A representation of a 16-bit word is shown in figure 5.1 where the bit-number, starting from the right, is shown above its respective bit. Incidentally, numbering starts at zero in computers and not unity. Each bit can be set only to zero or unity. If a given bit is set to 1 the numerical value assigned is 2" where n is the bit-number; remember that 2° = 1. The only exception to this is bit 15 which is the sign bit and if this is unity the number is interpreted as being negative. Thus, if hit 2 is unity and every other bit is set to zero the value of the whole word is 4. If bits 2,1 and 0 are set to unity respective values of 4, 2 and 1 are contributed to the word value yielding 7. Similarly, if bit 5 only is unity the word value is 32 and if bits 0 through 5 are all unity the value is 32 + 16 + 8 + 4 + 2 + 1 = 63. Hence in binary notation 100 is equivalent to 4, 101 equates to 5, 110 to 6, 111 to 7, 100000 to 32 and 111111 to 63. The binary system is made less cumbersome by converting to octal notation. This is effected by summing the values associated with the binary notation in groups of 3 bits starting from the right of the word where each bit in the string of 3 contributes a value of 1, 2 or 4. Hence, binary 100000 (i.e. 32) reduces to octal 40 (denoted "40 in DEC RT-11) as bits 5 through 3 are binary 100 and contribute 4, and bits 2 through 0 are binary 000 and contribute zeros to the octal number. Binary 111111 (i.e. 63) reduces to "77 as bits 5 through 3 and bits 2 through 0 each contribute 4 + 2 + 1 = 7. Binary 101010 (i.e. 42) has an octal value of "52 as bits 5, 4 and 3 contribute 4 + 0 + 1 = 5 and bits 2, 1 and 0 contribute 0 + 2 + 0 = 2 respectively. Dividing binary 101010 by 4 shifts all bits two places to the right with loss of the two least significant bits, those furthest on the right, and we now obtain 001010. This is octal "12 as bits 5 through 3 contribute 0 + 0 + 1 and bits 2 through 0 contribute 0 + 2 + 0 to the octal number which has a numerical value of 0 + 0 + 8 + 0 + 2 + 0 = 10. This demonstrates the rounding down that occurs with integer arithmetic. Obviously, **- should be 10.5 but, the
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COMPUTING
loss of the two least significant bits causes the rounding down to 10. If we wish to preserve the decimal point and fractions of unity we have to use REAL*4 words. Multiplication is the converse of division where all bits are shifted the left. Hence, on multiplying binary 101010 by 4 we shift everything two places to the left and get binary 10101000 which, for convenience, is split into the three binary components 010—101-000 which contribute to the octal number (the leading zero of the 010 component is usually dropped). The most significant three bits (binary 010) contribute 2, the middle three bits (binary 101) contribute 5 and the least significant three bits (binary 000) contribute 0 giving the octal number "250. This
equates to 128 + 0 + 32 + 0 + 8 + 0 + 0 + 0=168.
5.2
Data processing
Data processing is part of the business whereby data are converted to information and there are a number of ways in which this can be carried out. 5.2.1
Data arrays A single-parameter data processing procedure assigns storage space for a data array where the number of storage locations corresponds to the number of digitization steps of the analogue-to-digital converters (ADC) in the system. Hence a 1024 ADC would require an array of 1024 and all cells with the same value would be summed into that particular array location. The most obvious universally appreciated data set of this type is the DNA histogram which is shown on the X-axis of figure 5.2. With a Gl peak of a 'good' data set recorded in channel 200 there will be data in only channels 180 to 440 thus, over 70% of the array will contain no data and represents wasted space. A similar two-parameter processing procedure would have to assign a two dimensional (2-D) array of 1024 x 1024 storage locations. Immediately we have a major problem as this represents 2 MgBytes of store which is beyond most mainframe computers to which the majority could have access. In the bivariate distribution of figure 5.2, which is a contour plot (see section 5.3.2) of 90° scatter versus DNA, it is obvious that the vast majority of the array contains no data. With a data set of 10 000 cells in which no two cells have the same coordinates over 99% of the 1024 x 1024 array contains zeros and represents wasted space. Extending this type of data processing system to three parameters each with 1024 resolution could not even be contemplated as this would require the assignment of a 1024 X 1024 x 1024 array, i.e. 2K MgBytes of memory. 5.2.2
Multi-parameter data Two major problems arise in handling multiparameter data sets. Firstly, in standard FORTRAN IV, which is largely obsolete but is a language in which many programs are written, it is not possible to assign directly addressable arrays with greater than three dimensions. Even if it was, we would not be able to use them with 10-bit (1024) resolution for the reason outlined above. Secondly, the
DATA PROCESSING
77
DNA
<
o
0)
°o 0)
figure 5.2. Bivariate distribution of 90° light scatter versus DNA presented as a contour plot.
frequency of each set of identical n-dimensional coordinates within the data base must be found. For example, we have to find the number of times say x = 480, y = 210 and z = 863 occurs in the list-mode data set and how many times the set of x = 23,y = 493 and z = 126 occurs. A coordinate-by-coordinate comparison could be made but this results in a massive computation for 3-D data with 10 000 sets of coordinates, one set for each cell, and becomes prohibitive as the dimensionality of the data set increases further. We have routine applications in our laboratory which require 4- and 5-D analyses and for some applications this has been extended to seven dimensions. Hence, methods have been developed to process data sets with up to eight dimensions which is the maximum that can be handled rapidly by a 16-bit computer. The procedure involves three steps, namely coordinate coding, ranking plus frequency determination then decoding with data packing. (1) Single number coordinate coding A multi-dimensional array is not stored as such in computer memory but as a mono-dimensional linear array and the positions of the array elements are located using the array vector mapping equation. This equation, with the addition of 1, can be used as a means of coding multi-dimensional coordinates as a single number, CODE (Watson, Horsnell and Smith, 1988). It was introduced for data reduction by the author at the Meeting of the Society for Analytical Cytology, Schloss Elmau, in 1982, and has subsequently been used by Mann (1987). The form of this equation is
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COMPUTING
as follows, CODE = 1 + ( J - 1 ) + X(i/-l) + XY(zwhere CODE is unique for a given set of the 3-D coordinates x, y and z and where X and Y are the maximum values of the x and y measurements. The equation is written in this form as the terms (x—l),(y — 1) and (z — 1) must be handled as the whole of each expression within the parentheses. The reasons for this will be apparent in the following worked example. The coordinates x = 3,y = 2 and z = 4, where X, Y and Z are all 5, have a CODE of S3 which can be decoded as follows. On dividing through the above equation by XY and rearranging we get XY Using integer arithmetic in this equation, which rounds down to the nearest integer (see section 5.1), we can see that the first two terms on the right-handside (RHS), ( x - l ) / X Y and X(y-1)/XY will be zero as XY=25 and the largest possible numerator in these terms, X(y — 1), will have a maximum value of 20, hence, (CODE-1)
XY
=Z
~'
Thus, the z coordinate is given by, (CODE-1)
82
Again using integer arithmetic the term (**-) = 3, hence z = 4. The y coordinate can now be decoded. As the z coordinate has been obtained the last term in the coding equation, XY(z — 1) = 75. This is subtracted from the original CODE to give, CODE-l-XY(z-l) = ( j Dividing through by X, which is equal to 5, gives,
With integer arithmetic this reduces to, 1 = 0 + 1/— 1, hence y = 2 The x coordinate can now be extracted by inserting the decoded z and y coordinates into the coding equation giving, 83 = 1 + ( * - ! ) + 5 ( 2 - l ) + 25(4-l), hence x = 3.
DATA PROCESSING
79
The coding equation can be expanded for any number of dimensions but in practice this procedure is limited by the magnitude of a number that can be handled by a particular computer. The maximum code is 2 48 using 64-bit precision (double precision floating point) with FORTRAN in a 16-bit computer (PDP 11/40 and LSI 11/73) as with values larger than this rounding down problems are encountered during decoding. Hence with 10-bit data precision we can code four-dimensional data as a single number as the maximum code will be 2 40 . If data sets with more than four-dimensions are needed the data precision must be reduced. Thus, six-dimensional data must be reduced to 8-bit precision (0—255), and eight-dimensional data must be reduced to 6-bit precision (0—63), as in both cases the maximum code will be 2 48 . (2) Ranking the coded data Each set of w-dimensional coordinates is coded as a single number and stored sequentially in a mono-dimensional array. The maximum dimensions of this 64-bit precision coded array is the number of cells in the data set and in our PDP system this is stored in virtual memory. The array is now ranked in ascending order according to the magnitude of the value in each element of the array. It is now a simple process to find the frequency with which a given code occurs in a single pass through the array with concomitant reduction in storaged requirements as the frequency with which a given code appears is stored in a 16-bit array. (3) Decoding, data packing and unpacking
The data now exist in the form of two
arrays, one of 64-bit precision and one of 16-bit precision. The latter contains the frequency of a given code in the array location corresponding to its code value in the former. Thus, 80 bits are needed for each record in order to store a given set of coded coordinates together with the frequency. This can be relatively costly in terms of storage and the following space saving procedures have been developed. These use 'bit-shifting' routines which move a specified number of bits from one location in a first variable to a specified location in a second variable. VAX FORTRAN 77 contains such a subroutine, MVBITS, and an assembler language look-alike' routine, also called MVBITS, has been written for PDP 16-bit computers using RT-11. This routine is given at the end of this chapter together with two FORTRAN routines which perform similar operations.
The data are decoded according to the procedures described in the worked example above and the coordinates are packed, using the MVBITS routine, into two, three or four 16-bit integer packed data words (IPDW) depending on the data resolution and data set dimensionality. A schematic summary for 6-bit data resolution is shown in figure 53. Taking 4-D data as an example, the fourth and third coordinates are stored in bit locations 10 through 15 and 4 through 9 respectively (bit positions are numbered from the right starting at zero) in IPDW(l). The second coordinate straddles IPDW(l) and IPDW(2), where the top
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COMPUTING
Coordinate
1
S> 3-D
1
7
8
6
4
, 5
y/ 1
4-D •
1
. 3
2 ,
:
1
X
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1
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• 1
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IPDW(1)
X:
:X
/ : : X
1
IPDW(2)
F j
IPDW(3)
„
F
X
J
IPDW(4)
Figure 5.3. Summary of 6-bit resolution data packing.
four bits are located in bit positions 0 through 3 in IPDW(l) and the bottom two bits are located in bits 14 and 15 of IPDW(2). The first coordinate and the frequency are located in bit positions 8 through 13 and 0 through 7 in IPDW(2). The 10-bit resolution data (up to four dimensions) and 8-bit resolution data (up to six dimensions) are similarly packed, but obviously into different bit positions. With 4-D data and 10-bit resolution the fourth coordinate is packed into bit positions 6 through 15 in IPDW(l) and the highest six bits of coordinate 2 are packed into bit positions 0 through 5. IPDW(2) contains the lowest four bits of coordinate 2, coordinate 3 and the highest two bits of coordinate 4 in bit positions 12 through 15, 2 through 11 and 0 through 1 respectively. The lowest eight bits of coordinate 4 and the frequency are now packed into bit positions 8 through 15 and 0 through 7 in IPDW(3). The data can be unpacked by reversing these procedures.
5.3
Data display
Any system which produces large quantities of data, particularly if these are multi-dimensional, must have efficient and 'user-friendly' data presentation methods. This is another important step in converting data, which is just a series of numbers, into information. The distinction between data and information was made previously and I know I keep going on about this but it is very important. Data display is another necessary requirement for this transformation.
DATA DISPLAY
5.3.1
81
Mono-dimensional histograms
The simplest data set in flow cytometry is the mono-dimensional histogram where, like any other histogram, frequency is scored on the Y-axis (ordinate) versus the magnitude of the measurement (fluorescence or scatter intensity) on the X-axis (abscissa). The X-axis of figure 5.2 showed an example of a DNA histogram which has two peaks separated by a trough. The first peak corresponds to cells with Gl DNA content and the second, recorded at double the abscissa scale reading, corresponds to cells with G2 + M DNA content. Cells between the peaks are at various stages of DNA synthesis. This type of histogram can be analysed by a number of computer programs to give the proportions of cells in Gl, S and G2 + M (see section 11.4). The Y-axis of figure 5.2 is an even simpler data set of a histogram of frequency versus 90°scatter. In spite of the simplicity of such data sets they contain a considerable quantity of information. Here, we may ask if the spread in the data conforms to a particular distribution (see sections 5.4.4) and we can also determine how many molecules correspond to each channel of the histogram (see section 9.2). 5.3.2
Bivariate data A bivariate data set is one in which two measurements were made on each cell in the sample and a number of methods have been developed to present the data within these two-dimensional data spaces. (a) Dot-plots The simplest method of presenting bivariate data is to display the two measurements from each cell as a dot with X and Y coordinates proportional to the two measurements. This is shown in figure 5.4 where forward scatter is plotted on the ordinate versus 90° scatter on the abscissa from mouse bone marrow with the associated mono-dimensional histograms adjacent to the respective axes. The problem with this type of display is that it gives little depth or height perception. Once a pixel on the oscilloscope screen is lit up with the first cell to be scored in that location it cannot be lit up again if another cell has exactly the same coordinates. This can be overcome to some extent in systems with gray scale capability but the majority of 'earlier instruments do not have this feature. (b) Contour maps A second method is to present the data as a contour plot where lines are drawn to connect points of the same frequency. This is directly analogous to a terrestrial contour relief map which shows distances above sea level. The data in the previous figure are redrawn in this form in figure 5.5 and an elliptical gate, Pi, has been placed on the most prominent peak for future reference (section 5.3.4).
COMPUTING
Figure 5.4. Dot-plots of 90° scatter on the ordinate versus forward scatter on the abscissa from mouse bone marrow with the associated mono-dimensional histograms adjacent to the respective axes.
PA
Figure 5.5. Contour map displays of the data shown in figure 5.4.
DATA DISPLAY CQ2704-. 0 0 1 PA
2UM FDA MARROW C
2UM FDA MAPRO* C 27-APR-87
ILTERIN
CD2704-. 001 PA
Figure 5.6. Two perspective 'hidden surface elimination' views of the same data as in the previous two figures. The 'dip' in the center of the data is now clearly apparent.
84
COMPUTING (c) Stereo-perspective colour graphics
This type of display presents the data as a 'solid-model7 in stereo, perspective and colour with frequency on the Y-axis (vertical) versus the two measurements on the X- and Z-axes, and an example is shown here in black and white in figure 5.6 and in colour on the front cover. This is the same data set presented in the previous two figures and it is clear that this is a far superior display system where the depth and height perception is self-evident. However, we must also be able to rotate these displays in order to be able to see round the 'back7 as the 'hidden' surfaces and lines are eliminated which may also mask some data. This is by far the best method of presenting data in a two-dimensional data space but it did present a formidable computing problem to write the graphics routines in under 4K memory for use on a micro-computer with 28K addressable memory. 5.3.3
Trivariate data Three-parameter data are a little more difficult to display and ideally, stereoscopic views should be used. An example from bone marrow for the hydrolysis of two esterase substrates (horizontal axes) versus time (vertical axis) is shown in figure 5.7. Four populations can be identified and line vectors have been drawn through the medians of each of the 10 contoured time-slices. This figure should be inspected with a stereoviewer.
Figure 5.7. Stereo-perspective 3-D display for the hydrolysis of two esterase substrates (methylumbelliferyl acetate, 440RF AREA, versus fluorescein diacetate, 520RF AREA) versus time (vertical axis). The four vectors have been drawn through the medians of the populations at each of the 10 time-slices.
DATA DISPLAY
85
5.3.4
Multi-parameter data The world in which we live is three dimensional and conceptually it is difficult to visualize the geometry and meaning of a data space containing four or more dimensions. It is not possible to display four-dimensional data within a geometrical space as shown for three dimensions in figure 5.7, and multidimensional data are best displayed in a series of related two-dimensional data spaces. This process is illustrated as follows. The light scatter data from mouse bone marrow cells in figure 5.5 were gated to include the most prominent peak within the gate. We have the option of using either rectangular or oval gates in our system but we most frequently use the latter as biology doesn't tend to have sharp edges. During this particular assay we were measuring esterase activity (green fluorescence, 515—560 nm, from fluorescein diacetate hydrolysis, 488 nm excitation) versus time, simultaneously with both forward and 90° light scatter. Figure 5.S shows the esterase activity, where green fluorescence is plotted versus time for the gated population of figure 5.5, and three subsets, with high, medium and low activity are apparent. The designation of this data space is Pl/SA, indicating region 1 of the primary data space (Pi) and all of the secondary data space (SA). Incidentally, gating in the primary, secondary and tertiary data spaces is denoted by P, S and T respectively in our system. Each of these subsets was similarly gated with elliptical regions (only the bits of the ovals within the bounds of the data spaces are shown) which are marked as Si, S2 and S3 respectively. The primary data space (figure 5.5) displayed the pulse width for forward versus 90° scatter
P1/SA
TIME
Figure 5.8. Esterase activity, where green fluorescence is plotted versus time for the gated population of figure 5.5 and three subsets, with high, medium and low activity are apparent.
86
COMPUTING
(488FS WDTH versus 488RS WDTH). We wanted to determine if the three subsets of figure 5.S exhibited different light scattering properties by looking at total 90° scatter (AREA under the pulse, 488RS AREA) versus forward scatter peak height (488FS PEAK). These data are shown in figure 5.9 where Pl/Sl/TA means primary data space region 1 (Pi), region 1 of the secondary data space (Si) and TA means all of the tertiary data space. The P1/S2/TA and P1/S3/TA designations are similar except that these refer to secondary data space regions S2 and S3 respectively. It is obviously important to have some systematic mnemonic coding system such as this otherwise you can very easily get lost. We can now see that P1/S2/TA and P1/S3/TA exhibit identical patterns but cells in Pl/Sl/TA show decreased pulse height in the forward direction (488FS PEAK) and a very much wider spread in their total light scattering properties at 90° (488RS AREA). This example demonstrates how a six-dimensional cross-correlated data set can be handled and understood using a series of two-dimensional data spaces displayed in three sequential steps. The data spaces were linked by a three-dimensional hierarchical gating structure which is described in the next section.
P1/S1/TA
P1/S2/TA
488RS AREA
488RS AREA
P1/S3/TA
488RS AREA
Figure 5.9. The 90° light scatter pulse area (488RS AREA) plotted against forward scatter pulse peak height (488FS PEAK) for the cells in the three subsets of figure 5.8.
DATA DISPLAY
5.3.5
8>7
Bit-mapping Bit-mapping is nothing more than technical jargon for a particular type of indexing. Let us suppose we have a 16-bit two-dimensional data array containing 128 X 128 (X, Y) coordinates, which requires 16K of memory. Each element of the array records the number of cells, frequency, at that (X,Y) location. Any given element could contain 32 767 cells (section 5.1) but, as most flow cytometric data sets do not contain more than about 10 000 cells in total the vast majority of the assigned memory is completely wasted (see section 5.2.1). Thus, we can afford to use some of the space as an indexing system, the bit-map. The simplest form of bitmap is one in which a single bit is reserved to record if a given coordinate is within a gated region, whatever shape this might be. The bit-map is also arranged as a 128 x 128 array where each bit corresponds in position to its respective (X,Y) coordinate of the data array. If a coordinate is within the bounds of the region the map-bit (mabit with a silent 'p', or mapit with a silent 'b', I think I'll use mabit, to coin a term) is set to 1. If a coordinate is not within the region the mabit remains set to zero. Using a single mabit we need 16K bits of memory (IK words) for the bitmap o f a l 2 8 x l 2 8 array which then allows us to accumulate only 16 384 cells in each storage location of the array but this is still 'overkill7 for most purposes. The beauty of this system is that we can search much more rapidly through a IK array for bits set to 0 or 1 than we can through a 16K array for coordinates that are within a gated region. This is particularly true where the region occupies a minority area in the two-dimensional data space, however, if the region occupies the whole data space then little is gained. Flow cytometric data are generally interesting only if different clusters are apparent within data spaces. That, after all, is the primary reason for using flow cytometric technology to obtain multiple simultaneous correlated measurements on an individual cell basis. Thus, bit-mapping will usually increase very considerably the speed at which we can sift through the data. The multi-parameter display system developed in our laboratories allows up to seven gated regions to be set in each two-dimensional data space where the sixdimensional data used as the illustration in the previous section were reduced to 6bit precision (0—63) for the reasons given in section 5.2.2. The primary data space (e.g. figure 5.5) is a 64 X 64 array containing the cell frequencies at every (X,Y) coordinate which are stored in the upper 13 bits of each word in the array. The lowest three bits, the mabits, are reserved for recording the region to which a given coordinate may subsequently be assigned. Three mabits give us a range of 0 through 7 which enables seven regions to be set with zero corresponding to no assignment and initially these three mabits are set to zero. When a region is placed around a cluster the mabits are set to the value corresponding to the number of the region. For example, a single region was set in figure 5.5 and all coordinates falling within this region had the mabits set to a combined value of 1, i.e. 001 in binary Three regions were set in figure 5.8 and the mabits of the coordinates within those three regions were given values of 1, 2 and 3 respectively. Once the position of a
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FILE JK27127. 000 ASSAY VI PA
DATE 27-JLIL-88
H
1
1
1-
630RF AREft
Figure 5.10. Two-dimensional contour plot of green fluorescence (bromodeoxyuridine incorporation) versus red fluorescence (DNA) in which 4 gated regions have been set. Regions 1 and 2 correspond to Gl and G2 4-M cells respectively. Region 3 includes labelled cells in mid S-phase and region 4 surrounds the other three regions.
given region is verified the mabits retain their values even if a second or more regions overlap the first; the value of the mabits can only be altered if their value is zero. This is illustrated in figure 5.10 which shows a two-dimensional contour plot of green fluorescence (bromodeoxyuridine incorporation) versus red fluorescence (DNA) in which four gated regions have been set. Regions 1 and 2 correspond to G l and G2 4- M cells respectively. Region 3 includes labelled cells in mid S-phase and region 4 surrounds the other three regions. The individual regions are shown in figure 5.11 where the region 4 data space (P4, bottom right) exhibits 'gaps' due to the absence of cells which are in the other regions. We can now return to the six-dimensional data handling problem where up to seven regions can be bit-mapped in the primary array which will subsequently be referred to as the A-B data space. In the example cited in figure 5.5 only one region was set for simplicity and we now have to find the green fluorescence (esterase activity), time, 90° scatter pulse area and forward scatter peak height data associated with the coordinates in the Pi gated region of the primary A-B data space which is forward versus 90° scatter. These parameters, namely green
DATA DISPLAY
89
fluorescence, time, forward scatter peak height and 90° scatter pulse area subsequently will be referred to as C, D, E and F respectively. We must now refer back to section 5.2.2 where we saw that multi-dimensional arrays are stored as linear arrays and that the elements of the multi-dimensional array are located within the linear array using the vector mapping equation. The location, L, of given x and y coordinates of a 64 x 64 two-dimensional array within the monodimensional array are given by L = 1 + (x — 1) + 64 x (y— 1). Thus, for example, the location of the two-dimensional coordinates x = 2S and y = 20 will be position 1244 in the linear array. The region set in the A-B data space will have an upper and lower location boundary within the A—B space defined by the region size and shape which can be calculated from the mapping equation. Furthermore, the sixdimensional cross-correlated data set was also coded using this same equation and ranked in ascending order according to code number magnitude (section 5.2.2). This data file is now read one block (256 words) at a time from disk and the A-B
FILE JK2707. 000 ASSAY VI Pi
DATE 27-JUL-89
FILE JK27B7- 000 ASSAY VI P2
630RF AREA
630RF AREA
FILE JK27B7. 000 ASSAY VI P3
DfcTE 27-JUL-98
630RF AREA
OftTE 27-JUL-88
FILE JK2707. 000 ASSAY VI P4
DftTE 27-JUL-B9
630RF AREA o
A Figure 5.11. The individual regions of figure 5.10. Panels Pi, P2, P3 and P4 correspond to regions 1,2,3 and 4 respectively. The P4 data space exhibits 'gaps' due to the absence of cells which are in the other regions.
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COMPUTING
data space information for the LAST entry is extracted and its location, L, is determined. If this is less than the lower boundary location of the region then the next block is read. However, as soon as the A—B data space location of the last entry is above the lower boundary location of the region we have found the first block in the six-dimensional file which contains the required data. By the same token, when the location of the A-B data space information of the FIRST entry in the data block is greater than the upper limit boundary location of the region there is no need to search further as all the required data will have been extracted. In practice the search procedure is a little more complicated than just described as, for large data sets, which are always those not well clustered, every second, fourth or eighth block is read depending on data set length but the principles involved are identical. Obviously, further complexity arises with multiple gated regions but these are not too difficult to overcome. The segment found in the cross-correlated file contains the six-dimensional data which pertain to the region set in the A—B data space, including the A—B data. The latter is not needed as this has already been looked at and the region set within it. However, we do need to record the region identifier and extract the fourdimensional data we have yet to display and analyse. The secondary and tertiary data spaces will contain the C-D and E-F data respectively. The former are placed directly into one of seven two-dimensional arrays with 64 x 64 locations each, where the C—D data associated with region 1 goes into the first array and C—D data associated with region 7 are placed in the last. Thus, the bit-mapped regions of the primary (A—B) data space are mapped respectively to the C—D data spaces by virtue of the secondary data space array identifier. Gating, again with up to seven regions, will be carried out in the C-D data spaces, of which there is a maximum of seven, and these regions will be bit-mapped as previously described. However, we have not yet set any regions in any of the C—D data spaces so we have to preserve the associations between the C—D and E—F data from the six-dimensional crosscorrelated datafile.These coordinates are extracted and for each record are loaded, using the bit-shifting routines, into an auxiliary array together with the frequency. This requires two 16-bit words and the data are arranged according to the scheme shown in figure 5.12. The C and D coordinates occupy the first and second six bits of word 1 respectively leaving the top four bits, 12-through-15, for the four least significant bits of coordinate E. The second word contains the top two bits of coordinate E in bits 0 and 1 and coordinate F is placed in bits 2-through-7. This leaves the top eight bits of the second word to record the frequency with which coordinates C, D, E and F occur in association. I said earlier that the A-B data space region also had to be recorded but this does not appear in either word of the auxiliary array. However, we do not have to have this for every record. Region 1 of the A-B data space is dealt with first and recorded first in the auxiliary array, the second is dealt with second and you can guess the rest of this sentence. Hence, all we need to do is keep track of where the records associated with regions 2,3, 4 etc. start in the auxiliary array. We don't have to record this information for region 1 as this always starts at location 9 with the first eight locations being reserved for the
DATA ANALYSIS
91
Word 2 15 14 13 12 1 1 1 0
9
8
7
6
Word 1 5
4
3
2
1
0
15 14 13 12 11 10
9
8
7
6
5
4
3
2
1
0
Freq Figure 5.12. Arrangement of two 16-bit words containing multi-dimensional coordinates and the frequency with which they occur.
directory to the array. The directory records the number of regions set in the A—B data space in location 1. Locations 2 through 7 are reserved for the starting positions of their respective regions and the eighth location records the finishing point of the last region. Thus, the A-B data space regions are mapped to all combinations of C, D, E and F coordinates and their frequencies. We are now in a position to display the secondary (C—D) data space information for any of the seven regions which could have been set in the A—B data space. This was shown in figure 5.S for the only region set in the A—B space of figure 5.5. Three regions were then set, and bit-mapped, in the C-D data space of figure 5.8. Once the secondary (C-D) data space regions have been verified we can refer to the auxiliary array to find the C-D coordinates within the array corresponding to the bit-mapped regions of the C—D data space. This is carried out using the procedures already described. The E—F data in the same record in the auxiliary array as these C—D coordinates are now extracted together with their frequencies for display as the tertiary, E-F, data space which was shown in figure 5.9. Bit-mapped region setting can then be carried out in this tertiary data space. The final form of the auxiliary array, which can be written to disk as a permanent file if required, contains the E—F coordinates and their frequencies together with an index. The latter records the region identifiers with which the E—F data are associated in both the primary (A-B) and secondary (C-D) data spaces, details of the A-B and C-D data space region settings and simple statistics of the A, B, C and D distributions within the various regions. These statistics include the mean plus CV, median, mode and numbers of cells. The final processed file does not contain the individual coordinates of each cell in the A—B and C—D data spaces. These are not strictly necessary as long as you are content with knowing from which regions in each data space the E-F coordinates were obtained.
5.4
Data analysis
The data display and handling procedures described in the previous section enable us to obtain a readily appreciated visual record of even quite complicated data sets. This, as noted earlier, is one of the steps in transforming arrays of essentially meaningless numbers into information. In order to amplify
92
COMPUTING
DUMP/OUT:TTJ/ST:I VB VB4:PS3ll0.H00 BLOCK NUMBER 00001 000/ 000000 000000 000000 020/ 000000 000001 000000 040/ 000003 000001 000001 060/ 000004 000003 000004 100/ 000005 000004 000002 120/ 000004 000002 000005 140/ 000120 000242 000417 160/ 000775 000476 000303 200/ 000071 000074 000112 220/ 000072 000056 000071 240/ 000065 000051 000045 260/ 000064 000071 000046 300/ 000065 000056 000057 320/ 000117 000106 000074 340/ 000204 000240 000174 360/ 000103 000072 000042 400/ 000003 000002 000002 420/ 000001 000003 000002 440/ 000001 000001 000002 460/ 000003 000002 000000 500/ 000000 000000 000000 520/ 000000 000000 000000 540/ 000000 000001 000002 560/ 000001 000001 000002 600/ 000001 000001 000000 620/ 000003 000001 000000 640/ 000000 000001 000001 660/ 000001 000001 000003 700/ 000000 000003 000000 720/ 000003 000002 000000 740/ 000000 000001 000001 760/ 000002 000000 000000
000000 000001 000001 000001 000005 000012 000635 000215 000074 000065 000060 000054 000071 000115 000213 000040 000004 000001 000000 000000 000000 000003 000000 000000 000000 000002 000000 000000 000001 000001 000000 00000O
000000 000001 000002 000002 000003 000006 001036 000140 000077 000074 000070 000045 000101 000146 000157 000027 000006 000002 000003 000001 000001 000001 000001 000000 000001 000003 000000 000002 000000 000000 000000 000000
000000 000002 000003 000004 000001 000013 001327 000141 000053 000064 000050 000055 000072 000135 000154 000021 000006 000001 000001 000001 000000 000000 000001 000000 000001 000001 000001 000000 000003 000002 000001 000000
000000 000002 000004 000002 000003 000023 001336 000116 000103 000045 000043 000051 000063 000154 000146 000011 000001 000002 000001 000001 000001 000003 000001 000000 000000 000000 000000 000002 000000 000001 000001 000000
000000** * 000003 * * 000005 * * 000003 * * 0 0 0 0 0 0 *•••• * 0 0 0 0 4 5 *••••• %•* 001310 *P. U«~.H.* 0001.16 *> • > • C • . •x . a • N . N . * 000076 *9.<•J.<•?.+•C•>•* 000065 *i.,,9.5.<.4.%.5.* 000057 *5.).X*0»8. <•••/.* 000072 -*4.9.*.r.%.-•>.:.* 000103 *5.••/•9»A•:•3•C•* 000232 *0•F.<•M.f.3.1.•.* 000137 *•• • ! ••.o•1•f•_•* 000007 *C•t . ' * 000001 * * 000000 * * 000002 * * 000002 * * 000000 * * 000001 * * 000000 * * 000000 *• * 000003 * * 000000 * * 000000 * * 0 0 0 0 0 1 *••••• * 000001 * * 000001 * * * 000000 * * 000000 * *
Figure 5.13. One block of data (256 words) from a DNA histogram file as stored in the computer. this last point I am showing one block of data in figure 5.13. Data presented in this form will remain totally useless until they are placed in context and in a manner which can be appreciated. The data in figure 5.13 represent a DNA histogram, and those who are familiar with looking at data in this format could either have guessed this or worked it out; however, you would also have to be familiar with octal. It may seem a little daft to include this figure but one of the early commercial instruments actually presented the data hard copy just as a long string of numbers. Even when the DNA histogram is presented in the regular format (there are plenty later on) exhibiting the familiar Gl and G2 + M peaks with the S-phase trough between we still have to analyse the data to extract the proportions of cells in the three phases. This is the information we require and this section is concerned with the processes of extracting information which falls into five basic categories, counting within gates, distribution assessment, deconvolution of distributions, distribution shape analysis and background subtraction.
5.4.1
Counting within gates
This is the most simple, and time honoured, of all analysis procedures in flow cytometry. An example is shown in figure 5.14 in which a T-cell clone was
DATA ANALYSIS
488RS WDTH
93
520RF AREA
520RF AREA
Figure 5.14. Analysis of a T-cell clone stained for thy-1. Panel A is frequency versus 90° scatter and panel B is the green detector response for fluorescence control cells between the vertical bars in panel A. Panel C shows the specific green fluorescence for thy-1 staining; 23% of the population was above the control delimited set in panel B.
stained with a thy-1 antibody using a two step technique (see section 7.3.1). Panel A is the 90° scatter histogram and only cells between the two vertical lines were included for subsequent analysis. Panel B shows the green fluorescence histogram obtained with an irrelevant first antibody where the vertical line was set at the upper limit of the distribution. Panel C represents the results obtained with thy-1 labelling and a subset of the population exhibits specific binding signals manifest by a shift of part of the distribution to the right. The vertical line in panel C, which is drawn at the upper limit of the control distribution, is used as the delimiter between labelled and unlabelled cells. The fraction of the whole population above the delimiter can now be calculated and this gave an answer of 23%. This is far too low and the reason for this is covered in section 10.3, but these particular data sets were chosen to illustrate not only the procedure, but also the problems which might arise during the procedure. Multi-parameter gating has been considered in sections 5.3.4 and 5.3.5 and counting the numbers of cells in each of the various regions is one of the reasons for gating and is an integral part of these procedures. Figures 5.5 and 5.8 represent 2- and 4-parameter gating respectively and gating could also have been carried out in figure 5.9 which would have been 6-parameter gating.
COMPUTING
94
Mode \
Median ^Mean
o
or
Intensity Figure 5.15. The median, mean and mode of a skewed distribution.
5.4.2
Distribution assessment
Whenever we make any measurement, not just in flow cytometry, we have to expect some variation and many factors may contribute to this. If, for example, 10 different tailors measure the length of the same piece of cloth with the same old-fashioned linen tape-measure we will get 10 different answers. No-one will be surprised by this because it is quite obvious that each result will depend on how much tension each tailor places on both the cloth and the tape-measure. If each tailor now uses his/her own tape-measure the discrepancy in the results is likely to be even greater as the individual tape-measures are unlikely to be exactly the same length; older ones are longer. The sources of variation that can be readily identified in this particular assay are 'stretchiness' of both the cloth and the tapemeasure, the tensions placed on both plus the length of the tape-measure which is a calibration problem. If we now try to answer the question 'How long is the cloth?' we are in some difficulty. This can be resolved, at least to some extent, by taking the average which involves adding up the 10 individual measurements and dividing the result by 10 to give the arithmetic mean. This would be fine for the first scenario where each tailor used the same tape-measure as the over and under estimates are likely to cancel. But, this is not true for the second scenario where 10 different tapemeasures were used. In this case we have to take the length of the tape-measures into account. Older tailors have older tape-measures which are longer than they should be and hence measure 'short'. There are always relatively more younger tailors than older tailors as the probability of death is greater in the old ones. Similarly, there are always relatively more younger cells in an expanding population than older cells as the probability of division is greater in the older ones. If our tailors are drawn randomly from the population then there must be a larger chance of having relatively more long measurements of our piece of cloth and the distribution of the measurements will not be symmetrical. The arithmetic
DATA ANALYSIS
95
Median 178.5
Median 335.1
A
Mode
16.0
Aode
253.1
( \
Mean
246.3
Ban
410.4
'V.
A
B
Median 404.2
Median 9 9 1 .3
Mode 1024.0
Mode 1024 .0
Mean
Mean
473.9
8 6 1 .3
D
Figure 5.16. Examples of flow cytometric distributions for various cell surface determinant assays where the mean, median and mode are recorded on each individual panel.
mean is not an entirely appropriate measure of central tendancy for 'skewed' distributions of this type and the median should be used. The median is defined as that point in the distribution where half of the population lies on either side. With a symetrical distribution the mean and median as well as the mode (defined as the point of maximum frequency) are in the same place but in skewed distributions they are different and this is illustrated in figure 5.15. It is particularly important to make these distinctions in flow cytometry where some cells may exceed the dynamic range of the analogue-to-digital conversion step and be scored 'off-scale7 and appear in the last channel of the histogram. The problem is that we do not know how far 'off-the-end' they are, thus the true mean cannot be calculated and the median must be used as the measure of central tendancy. Figure 5.16 shows a number of flow cytometric distributions for various cell surface determinant assays in which all cells should have been labelled and where the mean, median and mode have been calculated and displayed on each individual panel. The potential problems are seen in panels A, C and D. In panel A some cells were scored with either zero or very little fluorescence and the mode was calculated as 16. In panels C and D there are very bright cells which are off scale at the right and in each distribution the mode is 1024, which is meaningless. Also, the means of these distribution are underestimated as it is not possible to know how far off-scale the off-scale cells would have been recorded if this had been possible. The only measure of central tendancy for the data shown in panels A, C and D is the median. As soon as more than 50% of the population is 'off-scale' there is no measurement of central tendancy which can be used.
96
COMPUTING
Fluorescence Figure 5.17. Hypothetical example of two reasonably symetrical distributions where satisfactory discrimination between the two can be obtained by just drawing a delimiter in the trough between the two as shown.
5.4.3
Deconvolution of distributions
All distributions contain components due to sources of variation, that is why they are distributions. However, we might also have two distributions which overlap each other and deconvolution means separating the overlapping components. These, obviously, cannot be physically separated but good estimates can be made using curve fitting procedures and statistical analysis. The DNA histogram is one such example where there are three distributions with two overlaps. These occur at the interface of Gl with early S-phase and at the late S-phase/G2 + M interface, and DNA histogram analysis will be considered in detail in section 11.4. A common problem in immunofluorescence work is encountered where attempts are made to determine the proportion of positive cells in mixed populations when the fluorescence is 'weak' and close to the background control with some overlap of the two. An 'easy' hypothetical example (we didn't have any easy real examples) is given in figure 5.17 where the shapes and separation of the distributions is such that satisfactory discrimination can be obtained by just drawing the delimiter in the trough as shown. Some real examples are shown in figure 5.18. In each of these a curve fitting procedure has been used which assumes that both the unlabelled and labelled cell data are normally distributed. The fitting procedure also takes into account the positive skewing due to the analogue-todigital conversion (section 4.3). The deconvoluted distributions predict that there are some positively labelled cells which have lower fluorescence signals than the control background signals from some of the unlabelled cells. This might seem a little difficult to accept at first sight but there is a perfectly reasonable physical explanation. Consider two cells where the first is unlabelled but with the potential for exhibiting a high background and the second is very weakly labelled but with a low background potential. If the first cell passes through the maximum light flux at the focus and the second passes through a lower light flux region then the unlabelled cell could exhibit a larger signal than the labelled cell. The geometry of this situation was considered in figure 338 of section 3.9.5.
DATA ANALYSIS
97
D
Fluorescence Figure 5.18. Real examples of data where curve fitting procedures are needed to compute the proportions of labelled and unlabelled cells. After the distributions have been deconvoluted we will have a mean and a standard deviation for each, and we may be asked to assess the differences between the distributions statistically using Student's-t. This can only be carried out rigorously if we know what type of distribution we are dealing with and this requires shape analysis, which is addressed in the next section.
5.4.4
Distribution shape analysis
The positive skewing effect of the analogue-to-digital conversion step on the shape of a distribution was described in section 4.3. What we see is the data output by the instrument and we may have to ask the question 'What is the real biological distribution from which the output data was obtained?7. Schuette et a\. (1983) addressed this problem to resolve closely spaced DNA histogram peaks with low CVs ( < 0.05) which may also be useful in chromosome analysis as well as in delineating aneuploid tumour components close to a diploid peak. Their method used an iterative computational procedure but, for CV values of 0.04 they required up to 1600 passes through the data to obtain satisfactory resolution. With CVs in the region of 0.2, which is typical for immunofluorescence, the number of passes through the data would increase astronomically rendering a purely iterative technique totally impracticable. The approach in our laboratory for the higher CVs seen with surface marker analysis has been to use a semi-analytic approach where
COMPUTING
98
we are testing the hypothesis of Gaussian distribution in the data (Watson and Walport, 1985). The various steps in the procedure are as follows. STEP (1) Assume a Gaussian distribution. STEP (2) Calculate the distribution for given mean and SD. STEP (3) Transform this to a distribution with constant CV as would be generated by the flow cytometer. This requires that each channel of the true distribution be redistributed according to the CV of that particular channel. The new distribution (defined as skewed-normal) is then obtained by a channel-by-channel summation of the redistributed data. In practice we have limited the spreading to + 4SD of a given channel although for some very extreme examples we have encountered some computational rounding down problems as predicted by Schuette et al. (1983). STEP (4) Compute the mean of the skewed-normal distribution which should be identical to the original as an equal number of cells are redistributed either side of the mean although the mode and the median will differ from the original. This estimated mean is satisfactory as long as only a small proportion of the total is redistributed to the first and last channels of the finite range into which the data must be confined in order to simulate the instrument's finite range. In extreme examples a systematic error was noted for which corrections could be applied. STEP (5) Calculate the variance and hence CV of the skewed-normal distribution. STEP (6) Apply systematic corrections for the CV found at step (5) and for the mean (if necessary) found at step (4) and generate the reconstructed normal distribution from these values.
o c
0) 3 O" 0)
Intensity Figures 5.19. Light scatter distribution from unstained red blood cells breaking through the 'green' fluorescence photomultiplier filters at high photomultiplier voltage. The continuous irregular line bounds the experimental histogram of frequency versus light intensity on the abscissa. The smooth dotted curve bounds the skewed-normal distribution which was generated from the reconstructed normal distribution.
DATA ANALYSIS
99
O
c 3
cr 0)
Intensity Figure 5.20. Fluorescence data from normal granulocytes stained with an antiCR3 monoclonal antibody. The smooth curve is the predicted skewed-normal distribution and the fit between this and the experimental data is compatible with the hypothesis that the experimental data derived from a normal distribution.
STEP (7) Take the reconstructed distribution and transform it according to the procedure at step (3) and compare it with the initial skewed-normal distribution generated at step (3). Figure 5.19 shows an experimental data set which was obtained from unstained red blood cells by measuring 488 nm light scatter (argon laser) breaking through the 'green7 fluorescence photomultiplier filters at high photomultiplier voltage. This data set was chosen to test the analysis as normally distributed data with a high CV were expected. The continuous irregular line bounds the experimental histogram of frequency versus light intensity on the abscissa. The smooth curve bounds the skewed-normal distribution which was generated from the reconstructed normal distribution. The mean of the latter was 99 with a CV of 0.39. The E# 2 calculated by comparing the experimental data with the predicted skewed-normal distribution was 199 with 248 degrees of freedom. This is associated with a probability p< 0.012 that the observed differences could have arisen by chance. Figure 5.20 shows comparable fluorescence data from normal granulocytes stained with an anti-CR3 monoclonal antibody. The mean and CV of the reconstructed distribution were 199 and 0.21 respectively. The £# 2 w a s 97 with 187 degrees of freedom for the comparison of the predicted skewed-normal distribution (smooth curve) with the experimental data. This value of E# 2 is associated with a probability p < 0.000 001 that this degree of fit could have arisen by chance. Thus, we may conclude that in both examples the biological information was normally distributed and that the skew was instrument in origin due to the constant CV derived from the ADC conversion. In the distribution shown in figure 5.21 (uninterrupted line) the analysis failed to substantiate the
100
COMPUTING
Intensity Figure 5.21. Light scatter histogram from a population of exponentially growing cells where the experimental data could not be fitted with a skewed-normal distribution.
hypothesis that the data were normally distributed. This data set is a light scatter profile from an exponentially growing tumour cell line stained for DNA using a nuclear isolation technique. Scatter was measured on a second detector and the histogram contains data from Gl, S and G2 cells and we would not expect these data to be normally distributed as the population was far from homogeneous. 5.4.5
Background compensation Some data sets exhibit a background continuum which overlaps a considerable section of the data. Examples include DNA histograms of nuclei extracted from paraffin wax embedded material (figure 5.22), a technique introduced by David Hedley and colleagues (1983), and flow karyotypes (figure 5.23). This type of background is usually due to bad preparation or starting material. It is very difficult to cope with even if you have a very large computer, and a number of algorithms have been developed to try to resurrect such data sets but none of these are entirely satisfactory. There are two basic problems here. Firstly, you cannot get good data out of a bad preparation, even though you might be able to apply some mathematical 'massage' to make the data look more presentable. It's been stated before and doubtless will be stated again, 'garbage in garbage out'. Secondly, mathematical massage is only really valid if you have some information about the mathematical nature of the type of distribution which is contributing to the background. This is really the same problem as that considered in section 5.4.3 where the background was modelled with the normal distribution. There is another, slightly more subtle, problem here. The data, to a very large extent, are obscuring the background so you don't know what type of distribution to model it with. Some time ago I used
DATA ANALYSIS
101
,? G2 peak DNA fluorescence Figure 5.22. Nuclei extracted from wax embedded material with a high background of rubbish.
9-12
DNA fluorescence Figure 5.23. A bad flow karyotype with high background. One of my preparations with my lymphocytes. I'm sure the cells were OK (it was 10 years ago and I'm still alive and kicking) and the instrument was performing well so the preparation was bad, I'm ashamed to conclude. to have a background compensating routine in my software which used a number of tricks to predict and subtract the background. Sometimes it seemed to work very well and produced very 'pretty' data but sometimes it didn't. As the Trojian sooth-say er Cassandra (one of Priam's many daughters, total not recorded, but 50 sons were recorded!!) warned 'Beware the Greeks bearing gifts'. From the outside the massaged data might look appealing, but looking good (or at least better) doesn't imply that the information content is increased. I've now withdrawn these routines from our software package as we get better, and more reliable, information by repeating experiments which is an option that is sometimes forgotten.
Appendix to Chapter 5
1) Asseiubler language bit-shifting routine for RT-11. SOURCE is the integer variable from which NBITS bits are to be shifted. SOURCESTARTBIT is the location of the first bit of the NBITS string in SOURCE. Bits are numbered from the right starting at zero. DEST if the integer variable to which the NBITS string is to be shifted. DESTSTARTBIT in the starting bit position in DEST. TITLE MVBITS ;CALL MVBITS(SOURCE,SOURCESTARTBIT ,NBITS,DEST,DESTSTARTBIT) MVBITS:: ;get source word MOV @2(R5),R0 MOV @4(R5),R1 ;source-start-bit ;prepare for RIGHT shift NEG Rl ;nbits MOV @6(R5),R2 ;make it a word-index ASL R2 ;right-justify data ASH Rl,R0 ;remove junk BIC SRCMSK(R2),R0 ;dest-start-bit MOV @12(R5),R1 MOV DSTMSK(R2),R3 ;get destination mask ASH Rl,R3 /position it BIC R3,@10(R5) ;make space in dest ASH Rl,R0 ;position new data BIS R0,@10(R5) ;insert it RTS PC ;0 bits (dummy) DSTMSK: BO ;1 bit B0000000000000001 B0000000000000011 ;2 bits B0000000000000111 B0000000000001111 B0000000000011111 B0000000000111111
Boooooooooiinm
B0000000011111111 B0000000111111111 B0000001111111111 B0000011111111111
Booooiiimiiini
B0001111111111111 B0011111111111111 B0111111111111111 Bllllllllllllllll
;16 bits
APPENDIX T O C H A P T E R 5 SRCMSK: BO BlllllllllllllllO B1111111111111100 B1111111111111000 B1111111111110000 BlllllllllllOOOOO B1111111111000000 BlllllllllOOOOOOO B1111111100000000 B1111111000000000 B1111110000000000 B1111100000000000 B1111000000000000 B1110000000000000 BHOOOOOOOOOOOOOO B1000000000000000 BOOOOOOOOOOOOOOOO END
103 ;0 bits (dummy) ;1 bit ;2 bits
;16 bits
104
COMPUTING
2) FORTRAN subroutines which pack and unpack 6-bit resolution data. NDIM is the number of dimensions in the data set. ICRD(s) are packed into IPDW(s) in BITPAK. The reverse operations are carried out in UNPACK. SUBROUTINE BITPAK(NDIM,ICRD,IPDW) C... FORTRAN "bit-packing" routine for 6-bit data resolution C... NDIM (3 through 8) is data set dimensionality C... ICRD is data input, 6-bit resolution C... IPDW is packed data word output IMPLICIT INTEGER*2 (A-Z) DIMENSION ICRD(9),IPDW(4) REAL RDUM
10 20 30
RDUM=FLQAT(ICRD(NDIM+1))*1024. IF (RDUM.GE.32768.) RDUM-RDUM-65536. IPDW(1)=IFIX(RDUM) .OR.(16*ICRD(NDIM)) .OR. (ICRD(NDIM-l)/4) IPEW(2)«0 RDUM»FLQAT( (ICRD(NDIM-1) .AND.3)) *16384. IF (RDUM.GE.32768.) RDUM=RDUM-65536. IPDW(2)«IFIX(RDUM) IF (NDIM.EQ.3) GO TO 10 IPDW(2)»IPDW(2).OR.(ICRD(NDIM-2)*256) IF (NDIM.EQ.4) GO TO 10 IPDW(2)=IPEW(2).OR.(ICRD(NDIM-3)*4) IF (NDIM.EQ.5) GO TO 20 IPDW( 2 )«IPDW( 2) .OR. (ICRD(NDIM-4 )/16) (3)0 RDUM=FLOAT((ICRD(NDIM-4).AND."17))*4096. IF (RDUM.GE.32768.) RDUM-RDUM-65536. IPDW(3)=IFIX(RDUM) IF (NDIM.EQ.6) GO TO 30 IPW(3)=IPDW(3).OR.(ICRD(NDIM-5)*64) IF (NDIM.EQ.7) GO TO 30 IPDW( 3)=IPDW( 3) .OR. (ICRD(NDIM-6)) IPDW(4)=ICRD(1) RETURN IPDW(2)=IPDW(2).OR.ICRD(1) RETURN IPDW(3)»ICRD(1) RETURN IPEW( 3 )=IPDW( 3) .OR.ICRD( 1) RETURN END
APPENDIX TO CHAPTER 5
SUBROUTINE UNPACK (NDIM, IPDW, ICRD) C... FORTRAN routine for "unpacking" data with 6-bit resolution C... NDIM (3 through 8) is data set dimensionality C... IPDW is packed data word input C... ICRD is 6-bit resolution data output IMPLICIT INTEGER*2 (A-Z) DIMENSION IPDW(4),ICRD(9) GO TO (110,90,70,30,20,10) NDIM-2 10 ICRD(1)=IPDW(4)+1 20 ICRD(NDIM-6)=(IPDW(3).AND."77)+l ICRD(NDIM-5)«((IPDW( 3) .AND. "7777 )/64 )+l GO TO 40 30 ICRD(1)=(IPDW(3).AND."7777)+1 40 JDUM=( IPDW( 3) .AND. "170000)/4096 IF (JDUM) 50,60,60 50 JDUM-16+JDUM 60 ICRD(NDIM-4)»(JDUM.OR.((IPEW(2).AND."3)*16))+1 GO TO 80 70 ICRD(1)=IPEW(3)+1 80 ICRD(NDIM-3)«((IPDW(2).AND."377)/4)+l GO TO 100 90 ICRD(1)«(IPDW(2).AND."377)+1 100 ICRD(NDIM-2)=((IPDW(2).AND."37400)/256)+l GO TO 120 110 ICRD(1)-(IPDW(2).AND."37777)+1 120 JDUM=( IPDW( 2) .AND. "140000 )/16384 IF (JDUM) 130,140,140 130 JDUM=4+JDUM 140 ICRD(NDIM-1)*(JDUM.OR.(IPCW(1).AND."17)*4)+1 ICRD(NDIM)=((IPEW(1). AND. "1760 )/16)+l JDUM=( IPDW( 1) .AND. "176000 )/1024 IF (JDUM) 150,160,160 150 JDUM=64+JDUM 160 ICRD(NDIM+1)=JDUM+1 RETURN END
105
6 Cell sorting
Sorting or separation of cells can be carried out using a number of physical and biological agencies. Perhaps the most extensively and frequently used, but least appreciated, is gravity. Red cells settle out to form the haematocrite layer in heparinized blood leaving the white cells in the buffy coat. Variations on this theme include density gradient sedimentation (Ficol and Ficol—Paque) and cell electrophoresis. The latter uses charge in combination with gravity in the separation process. Magnetism can also be used. Macrophages which have ingested iron particles fall prey to such manoeuvres. Biological procedures include complement lysis of specific antibody tagged unwanted cells leaving the cells of interest intact. Also, magnetic beads coated with antibody can be used to select positively for the cells of interest. Some of these procedures do not yield particularly pure sub-fractions and they will not be discussed further because this book is about flow cytometry. However, they should not be forgotten as they can, and frequently should, be used in conjunction with flow technology (see sections 63 and 6.4).
6.1
Ink-jet writing
Ink-jet writing (Sweet, 1965) was developed in the early and mid 1960s to attempt to cut down on the noise generated by 'classical' mechanical printing and to be able to write on fragile objects. One of the latter applications was date stamping individual eggs. This is notoriously difficult with traditional mechanical stamping devices which inevitably result in a significant proportion of breakages. In ink-jet writing the ink is forced at high speed through a fine nozzle and the jet breaks up into droplets. Normally, the droplet break-off point occurs at random distances from the nozzle and the droplet sizes are not constant. The trick is to make this break-off point a constant distance from the nozzle. This was achieved by introducing a high frequency pertubation into the jet by oscillating the whole nozzle assembly with piezo-electric diodes. With jets of 50 to 70 |im in diameter an oscillating frequency between 40 000 and 50 000 hertz will stabilize the droplet break-off point and form constant and regular sized droplets at the oscillating frequency. The stream of droplets can be guided in the X- and Y-axis planes by placing a variable charge on the droplets as they break-off from the jet. Down-
ELECTROSTATIC SORTING
107
stream from the droplet break-off point there are pairs of charged deflection plates at right angles to each other which deflect the charged droplets by defined distances proportional to the charge placed upon them. Thus, it is possible to guide the stream of ink droplets to trace out almost any geometrical shape including lettering.
6.2
Electrostatic sorting
Electrostatic cell sorting was developed from ink-jet writing and a typical layout shown in figure 6.1 was developed initially by Fulwyler at Los Alamos (1965) then by the Herzenbergs at Stanford University in the late 1960s and early 1970s in conjunction with Sweet (Hulett et al, 1969; Bonner et al, 1972; Herzenberg, Sweet and Herzenberg, 1976). The jet issues from the nozzle of the Crosland-Taylor type flow chamber and the laser intersects the jet just below the nozzle (the analysis point). The whole of the flow chamber assembly is oscillated at about 40 000 hertz with the formation of regular droplets which break off the jet at a constant distance from the analysis point at this frequency. Fluorescence and/or 90° light scatter is collected by the optics at 90° to the intersection of the jet with the laser, and solid-state detectors collect the forward scattered light. The system operates as follows. Cells are 'interrogated' at the analysis point and their fluorescence and light scatter characteristics are determined. The jet velocity is constant as is the distance between analysis and droplet break-off point. Thus, the time for a cell to travel from the analysis point to the break-off point, At, is also constant. If a given cell is analysed and is found to have characteristics in which the investigator is interested, then the jet containing the cell is charged at a time At Sample
First surface reflector Aperture
Laser beam
Fluorescence photomultiplier
Sample collection
Figure 6.1. Typical layout of an electrostatic cell sorter.
108
CELL SORTING
after it is analysed. Thus, the jet will be charged as the cell of interest is contained within the tip of the jet just before the droplet, which is about to surround the cell, breaks free from the jet. A 'split second' later the charged droplet containing the cell breaks off from the jet and is now isolated and in free fall. Further down-stream the stream of droplets passes between charged plates which deflect any charged droplets, either left or right depending on the sign of the charge, into suitable collecting vessels. Figure 6.2 shows a reproduction from Herzenberg et al. (1976) of a time-lapse photograph of the jet issuing from the nozzle which is located at the top with the
Figure 6.2. Time-lapse photograph of the jet issuing from the nozzle located at the top with the laser cutting across the jet just below the nozzle. The illuminating light for the exposures was stroboscopically flashed at exactly the same frequency as the droplet break-off frequency which 'freezes' the jet and droplets.
ELECTROSTATIC SORTING
109
laser cutting across the jet just below the nozzle. This and the following picture are quite remarkable as the illuminating light for the exposures was stroboscopically flashed at exactly the same frequency as the droplet break-off frequency. These photographs, therefore, represent multiple superimpositions (40 000 per second) of the jet and the droplets. As can be seen there is not a trace of 'fuzz' as each superimposition was, as far as it is possible to observe, exact and the droplet breakoff point is a constant distance from the laser intersection analysis point. The second picture (figure 63) shows the droplet stream between the deflection plates where three droplets are being deflected to both left and right. Again, there is exact superimposition of droplets on this multiple exposure photograph. Incidentally, data such as those in figure 6.2 can be used to calculate the surface tension of water
Figures 6.3. Down stream from the jet there are three droplets being sorted left and right.
110
CELL SORTING
from the shapes of the droplets as they break off from the jet, a technique originally suggested and used by Niels Bohr at Cambridge in 1909. The time it takes for a cell to travel from the analysis point to the droplet breakoff point, however, is never exactly constant as the velocity is not exactly constant. Very minor variation is possible as too is variation in the electronic timing, although this is also extremely small. Furthermore, the electrostatic charging of the jet cannot be absolutely instantaneous as it takes finite time (usually only nanoseconds) for the charge to build up to maximum. The timing of the charging must be to within + 10 (is at a droplet break-off frequency of 40 000 per second and it is possible, therefore, that the cell of interest may not be exactly at the droplet break-off point when the charge is applied to the jet. These various factors are determined (here it comes again) by Poisson statistics. Because of these potential sources of variation it is frequent practice to charge three droplets in succession with the timing arranged so that the cell is expected to reside in the middle droplet of the three which minimizes the chance of missing a cell of interest.
6.3
Cell sorting times
The flow rate and Poisson statistics considered in section 2.5 have considerable consequences for the time it takes to sort given numbers of cells, particularly for preparative as opposed to identification work. Not infrequently one is asked to sort 107 or even 108 cells so that, for instance, DNA can be extracted and manipulated. If we take a 'standard' concentration of 10 6 cells ml~ 1 with a core diameter of 10 |im we can calculate the time it would take to sort any given number of cells. This is shown in figure 6.4 where the time to sort 10 6 cells from a sample containing 106 cells ml" 1 with a 'standard' flow rate instrument (10m s" 1 core velocity) is shown on the ordinate versus core diameter on the abscissa. The three curves correspond to the situations where the population to be sorted comprises 100%, 10% and 1% of the total. In the extreme case where the minority population of 1% is required it would take 1.27 x 105 seconds to sort 106 cells, which is over 35 hours continuous running. Obviously, it would also take the same time to sort 107 cells from a population where the cells of interest make up 10% of the total. The requirement for 107 cells is not unreasonable for many applications for DNA preparative work in molecular biology and, frequently, the population of interest is a minority within heterogeneous samples.
6.4
Sorting purity and yield
We saw in section 6.2 that three-droplet charging can be used to minimize the chance of missing a cell; however, this has implications for the purity of the sorted population as any coincidence of unwanted cells in a droplet will contaminate and reduce the purity of the sorted fraction. In order to obtain some idea of the magnitude of this problem we will assume we wish to sort from a through-put rate of 5000 cells s" 1 with a jet velocity of 10m s" 1 using a cell
SORTING PURITY AND YIELD
111
1%
CO •o
104
o o
0) 0)
10 10
15
20
25
30
Core diameter, Figure 6.4. Time, on the ordinate, to sort 106 cells from a sample containing 106 cells ml~1 with a core velocity of 10 m s~ * versus core diameter on the abscissa. The three curves correspond to the situations where the population to be sorted comprises 100%, 10% and 1% of the total. concentration of 2 x 106 ml \ Looking back to section 2.5 we find that the core diameter would be about 17.5 |im; in fact it is 17.84 |im, which gives an area across the core of 250 |im 2. Using a similar calculation to that in section 2.5 we find that the cells are spaced at average intervals of 0.2 cm, which gives 5 cells cm" 1 . We need to know the length of core, and hence the number of cells, that will be included in each droplet. We obtain this by dividing the jet velocity by the frequency of droplet formation which gives (10 x 106 |im s~ 1)/40 000s~ l = 250 urn. We know that there are 5 cells per centimeter which is equivalent to 5 cells per 10 0 0 0 | i m = l cell per 2000 um. Thus each micrometer contains 1/2000 = 0.0005 cells, and 250 Jim (the length of the core which will be included in each droplet) contains 0.125 cells on average. We could also calculate the average number of cells per droplet by dividing the cell through-put rate by the droplet formation rate to give 5000 s~ 740 000 s~ 1 = 0.125. Whichever way we calculate the average expectation, this is the value of z to be used in the Poisson distribution for a single droplet sort to find the probabilities of 0, 1, 2, 3 etc. cells
112
CELL SORTING 100-1
o I
95 H
1 drop sort
0 U
'35 900)
a.
85 -
3 drop sort 82 2x10 5
5x10 5
10 6
Cell concentration, ml
2x10 6
-1
Figure 6.5. Proportions of sorted droplets containing single cells with varying cell concentrations, and hence varying sorting speeds, for a one- and a threedroplets sort.
being in any given droplet and for a three-droplet sort this value is mutiplied by 3 to give z = 0375 cells for each batch of three sorted droplets. Figure 6.5 shows the proportions of sorted droplets containing single cells with varying cell concentrations, and hence varying sorting speeds, for a one- and a three-droplets sort. At a concentration of 2 x 105 cells ml" * for a one-droplet sort over 99% of droplets will contain a single cell. This is a high purity but the instrument through-put speed is only 500 cells s ~ l and if our population of interest is 10% of the total we will be collecting the sorted fraction at 50 cells s" 1 . This would be fine for identification but hopeless for preparative work as, if 107 cells were to be needed, it would take over 55 hours. Raising the concentration to 2 x 106 cells ml" * increases the collection rate of the wanted cell fraction (10% of the total) to 5 0 0 s " 1 but with a three-droplet sort only 82.34% of the three droplets sorted will contain a single cell. A further statistical problem must be considered. If two cells are in a sorted droplet they could be two wanted cells or one wanted plus one unwanted. However, we cannot have two unwanted as the instrument is not programmed to sort this combination, there must be at least one wanted cell to trigger the sorting logic. If three cells are in a sorted droplet we could have three wanted, two wanted
SORTING PURITY AND YIELD
113
Table 6.1 Term
Combination
p4 4p3q 6p2 q2 4pq3 q4
4/7 3p+lq 2 p+ 2 q 1 p+3 q (4 q = {0.9)4=
Probability (O.I)4 =0.0001 4 X (O.I)3 X 0.9 =0.0036 6 X (O.I)2 X (0.9)2 = 0.0486 4 x O . l x (0.9)3 = 0.2916 0.6561 not applicable)
plus one unwanted or one wanted plus two unwanted. Again, we cannot have three unwanted. A cell can either be wanted or unwanted and it is a binomial distribution problem (it didn't appear in section 2.5 for nothing) to find the relative proportions with which the various combinations can occur. The form of the binomial distribution is {p + q)n = l. What does this mean? If n = 1 then p-\-q=l, and if p = 0.1 then q must be equal to 0.9. If we now take n = 2 and expand the expression (p + q)2 we get p2-\-2pq-\-q2=l. In flow cytometry terms n = 2 corresponds to two cells in a sorted droplet or group of droplets and the terms of the binomial expansion tell us the probabilities of obtaining two wanted cells (p2) and one wanted plus one unwanted cell (2pq) for any given value of p, the proportion of wanted cells in the sample. Remember, that if p is defined then q is also defined with a value oil—p, and that any term containing only q (e.g. q2) represents only unwanted cells which cannot trigger the system. For n = 3 we get p3 + 2>p2q + 3pq2 + q3 = l, where the respective terms give us the probabilities of finding three wanted cells (p3), two wanted plus one unwanted {3p2q) and one wanted plus two unwanted cells (3pq2) for given values of p. For n = 4 the expansion becomes p4-\-4p3q-\-6p2q2-\-4pq3-\-q4 = l. Let us take n = 4, i.e. four cells sorted simultaneously, as a worked example and list the probabilities of obtaining the various combinations of cells in table 6.1 for p = 0.1. The total probability in table 6.1 sums to 0.3439 as the q4 term, which is (0.9)4 = 0.6561, is not applicable as this represents only unwanted cells which are not sorted. The probabilities for the occurrence of each combination can now be calculated relative to the total, 0.3439. These relative probability values are now multiplied by the number of expected wanted cells to give their frequencies. These data are shown in table 6.2. The total frequency in table 6.2, 1.163 127, is the number of wanted cells per coincident four sorted which represents the fraction 0.2908. Similar calculations can be carried out for coincidence of both three and two cells to give 0.4022 and 0.5263 respectively. Table 6.3 shows the Poisson probability for N, the number of coincident cells sorted simultaneously, the total number of cells sorted relative to a nominal 100, the fraction within each sorted group that are wanted and the number of cells sorted that are wanted.
CELL SORTING
114
Table 6.2 Term p4 6p2 q2 Apq3
Total
Absolute probability
Relative probability
Frequency
0.0001 0.0036 0.0A86 0.2916 0.3439
0.000 290 78 0.010 46816 0.14132015 0.847 920 91 1.000 000 00
0.001163 0.031404 0.282 640 0.847 920 1.163 127
Table 63
N 1 2 3 4 Totals
Poisson probability 0.8243 0.1546 0.0193 0.0018 1.0000
Total number sorted 82.43 30.92 5.79 0.72 119.86
Fraction of wanted cells 1.0000 0.5263 0.4022 0.2908 —
Wanted cells sorted 82.43 16.27 2.33 0.21 101.24
We can now see that the proportion of wanted cells in relation to the total number of cells sorted is 101.24/119.86 = 84.46% which is marginally higher than the percentage of single events sorted, 82.43%. This small difference of 2% is due to the relative proportions of binomially distributed wanted and unwanted cells during coincidental sorting. The take home messages of the last two sections are that standard cell sorters are very efficient for sorting small numbers of cells with high precision and purity for identification purposes. However, they are not very efficient for sorting large numbers of cells for preparative work. Furthermore, purity has to be sacrificed to obtain a good yield (large numbers) but, the latter can sometimes be overcome by carrying out some bulk pre-sorting enrichment procedure of the types mentioned at the beginning of this whole section which would increase the proportion of the cells of interest in the sample before it is introduced into the cell sorter. If these are not practicable then it is still possible to use the cell sorter to obtain both purity and yield by running a 'fast' sort, 5000 cells s~ \ to obtain an 80% enriched sample of, for example, a 10% fraction which is then re-sorted at a slower rate to obtain the required purity on the second run. With this approach it is possible to sort 107 cells with > 9 5 % purity in about 7 hours as long as nothing goes wrong.
115
SORTING EFFICIENCY
6.5
Sorting efficiency
Sorting efficiency means that you do, in fact, collect the majority (should be > 95%) of the cells that you intended to collect in the pot you intended to collect them in. The way to determine that you have got what you want is to run a small sample from the sorted population through the instrument to check that all the cells/objects appear within the sorting selection window. An example of sorted chromosomes is shown in figure 6.6 where Davies et al. (1981) were sorting the X chromosome from the flow karyotype shown in the upper panel. The lower panel shows a sample of the sorted fraction which does confirm that the vast majority of the sorted fraction was chromosome X. In a long sorting run it is well worth doing this quality control check at intervals during the sort. The yield can be checked by haemocytometer or Coulter counting depending on which is
9,10,11,12
Fluorescence Intensity Figure 6.6. Chromosome sorting. The top panel shows the selection gate for the X chromosome. The bottom panel shows an analysis of the sorted fraction which confirms that the X chromosome was obtained. Data taken from Davies et al. (1981).
116
CELL SORTING
appropriate or available. However, if you have a cell sorter and you haven't got a haemocytometer then you shouldn't have a cell sorter. If the purity or yield is not what it should be, and from the data in the previous sections you should now be able to estimate this, then something is obviously wrong. The problem is most likely to be due to instability in the jet and droplet formation. This can be checked by looking at the droplet break-off point. The Beckton—Dickenson and Coulter sorters are equipped with either long focal length stream viewing microscopes or video cameras for this purpose. The illuminating light for the microscope is stroboscopically flashed at the droplet formation frequency and you should see patterns similar to those in figures 6.2 and 6.3. The Ortho instruments system 50 cell sorter (now taken over by Beckton-Dickenson) did not have this feature as standard but it is very straightforward to add this on. The most likely cause of jet and droplet formation instability is a partial blockage of the chamber outflow nozzle which is usually between 50 and 70 |im in diameter. It really doesn't take very much material in the nozzle to completely wreck the jet stability. The cause of the problem is usually cell debris (loose, spewed out DNA is bad) or clumps of cells in a badly prepared specimen. However, non-cellular nozzle blocking materials can be introduced at all stages in sample preparation. In my experience these include fibres from the plugging of plugged pipettes, short segments of hair or fur introduced during splenic removal from rodents and finally, little slivers of plastic which can arise from two sources. The first is from Petri dishes or wells where the cells have been harvested with a glass Pasteur pipette. Any scraping of the pipette tip over the plastic surface planes off little curls and slivers of plastic. These are very difficult to see not only because they are small, but also because the refractive index of plastic is fairly close to that of water which renders them almost invisible. The second source of plastic slivers is from polystyrene universal containers. In badly made batches (and they do vary) you can find very fine whispy threads of plastic still attached to the mould injection point. In some containers, where the injection mould sections have been forced slightly apart during manufacture there is a sharp ridge of plastic which can cut into the cap and shower flakes of plastic from the cap into the sample.
Preparation and staining
The objectives in preparation and staining are obviously to obtain a single-cell suspension with quantitative fluorescence staining of the molecule(s) of interest. Easy to say, but not always easy to achieve. In some tissues and cell types this is straightforward but, in others it can be very difficult. Preparation and staining procedures in flow cytometry are legion and it would require the majority of this book to give a comprehensive account. Hence, only a brief review of the principles involved are summarized in this chapter, but details of some techniques are given in the relevant sections later on.
7.1
Disaggregation
Disaggregation is clearly the first step in the process of obtaining singlecell suspensions. Some tissues need little or no disaggregation and the best examples of these are cells of the heamopoetic and lymphoid systems. Other tissues, e.g. skin and some elements of the musculo-skeletal system, are extremely difficult to disaggregate effectively without cell damage. Generally, the ease with which disaggregation can be carried out is related to the function of the tissue. Epithelial cells which form a 'barrier-layer7 at the environment interface have many types of intercellular connections, including desmosomes, which bind the cells of the epithelial surface tightly together. In contrast peripheral blood cells have no such connections. Two methods of disaggregation are available, namely mechanical and enzymatic, which can be, and often are, used in combination either with, or without, chelating agents. 7.1.1
Mechanical Mechanical disaggregation procedures can only be really effective in very loosely bound structures such as bone marrow and lymphoid tissue (Shortman, 1972). The sheer forces due to syringing through fine-gauge hypodermic needles (Pretlow, Wein and Zettergen, 1975) are sufficient to separate bone marrow cells. This type of process can also be used for other loosely bound tissues, e.g. spleen, liver and lymph nodes, where the tissue is first chopped with scalpel or scissors then successively syringed through increasingly fine needles (Harrison, 1953; Vann and Kettman, 1972; Archer and Wust, 1973). We have obtained very good
118
PREPARATION AND STAINING
yields of lymphoid cells from mouse spleen by simply applying compression to the organ under growth medium which splits the capsule and extrudes the cells followed by vigorous shaking of the 'squashed' product in a universal container. The suspension is then suspended in 10 ml growth medium to allow the larger 'bits' to settle out and the supernatant is pipetted off after 5 to 10 minutes, syringed then filtered. Mechanical disaggregation, by whatever means, can cause damage to cells (Rinaldini, 1958) and occasionally some selective loss and it should always be exercised with caution. 7.1.2
Enzymatic Enzymatic disaggregation techniques are directed towards disrupting intercellular protein connections and extracellular 'ground matrix' substances and proteins which bind cells together. Two classes of enzymes, the proteases and mucopolysaccharide (glycosaminoglycans) hydrolases, have been used in enzymatic disaggregation (Rinaldini, 1958) and the efficiency of disaggregation is dependent on a number of factors. These include pH, temperature, enzyme concentration, the ratio of the latter to the 'concentration' of target molecules, divalent cations, duration of exposure and size of the tissue pieces. The most commonly used proteolytic enzymes include trypsin, pronase, pepsin, collagenase and elastase and a brief resume of some of their properties, extracted from the books by McDonald and Barrett {1986a,b), is given below. Trypsin (EC 3.4.21.4) Trypsin has been the most commonly used disaggregating proteolytic enzyme. It is a serine protease which specifically catalyses the hydrolysis of proteins and polypeptides on the carboxylic side of the basic amino acids arginine and lysene. It is usually extracted from bovine pancreas and crude extracts are frequently contaminated with chymotrypsin, elastase, lipase, amylase and collagenase. The optimum pH is in the range 8.0—8.5 and inhibitors include soybean trypsin inhibitor, aprotinin and 0C2-macroglobulin. Ca 2+ ions confer some stability and chelation of calcium with ethylenediaminotetraacetic acid (EDTA) causes a slight reduction in activity. Pronase This is a 'trade-name' for a mixture of proteolytic enzymes extracted from Streptomyces griseus. The hydrolytic specificity is very wide and prolonged digestion will proceed to the single amino acid level. The optimum pH is 6.5-7.5 and there are no specific inhibitors. However, inhibition can be induced by dilution, cooling to 4°C, washing and resuspending cells in growth medium containing serum. Pepsin (EC 3.4.23.1) Pepsin in an acid protease with a relatively wide specificity which is extracted from porcine gastric mucosa. It cleaves preferentially bonds of phenylalanine, methionine, leucine and tryptophan residues in hydrophobic polypeptide domains but bonds involving tyrosine are resistant to hydrolysis. The pH optimum is between 1.5 and 2.5 and inhibitors include 4-bromoplenacyl bromide and pepstatin.
DISAGGREGATION
119
Collagenases (EC 3.4.24.3, 3.4.24.8) The collagenases are Zn-metalloproteases extracted from various bacteria. Their activity is directed towards proline residues in the sequence —Pro—X—Gly—Pro— where X is most often a neutral amino acid. Their activity is not specific for collagen and a number of polypeptides containing this motif will be hydrolysed. The pH optima lie between 6.0 and 8.0 and inhibitors include EDTA as these enzymes require Ca 2+ for their activity. Elastase (EC 3.4.21.36) This is a serine protease extracted from porcine pancreas. It hydrolyses peptide bonds on the carboxy terminus side of amino acids with uncharged non-aromatic side chains including alanine, valine, leudne, isoleucine, glycine and serine. The pH optimum is 8.5—9.0 and inhibitors include OC2-macroglobulin and 4-dinitrophenol diethylphosphate. Enzymes used in disaggregation which hydrolyse 'ground matrix7 substances include the hyaluronidases and the lysosyme group of enzymes both of which are widespread in nature. Hyaluronidases Hyaluronidases are found in cellular lysosomes particularly in salivary glands, liver and testis and in many bacteria but particularly in streptococci and clostridia (Meyer, 1971). It is one of the 'spreading factors' responsible for cellulitis and gangrene with streptococcal and clostridial infections. Testicular-type hyaluronidases (EC 3.2.1.35) hydrolyse glycosidic bonds to produce disaccharides of glucuronic acid and N-acetylglucosamine from both hyaluronic acid and chondroitin which is an isomer of hyaluronic acid. Commercial preparations are frequently contaminated with proteases and ribonuclease. The pH optima vary with enzyme type but are within the range of
3.5-5.5. Lysosyme Lysosyme is a term coined by Fleming (1922). It is derived from the words lytic enzyme' which he used to describe the bacteriolytic effects of what he surmised were enzymes in a number of body fluids, including saliva and tears, and cells, most notably leukocytes. These enzymes also cleave glycosidic bonds in polysaccharides but between N-acetylglucosamine and N-acetylmuramic acid. As with the hyaluronidases the lysosymes have pH optima which depend on enzyme type but these are usually between 5.0 and 9.0 (Imoto et al, 1972). The enzyme(s) chosen for disaggregation depend(s) on the starting material and the type of preparation that is required. If the starting material is solid tissue it is necessary to chop this into small pieces to increase the surface area before adding the enzyme solution. Wide ranges of enzyme concentrations are reported in the voluminous literature and this, at least to some extent, reflects the purity of different commercial preparations. It is always advisable to carry out pilot studies with a range of enzyme concentration titrated against time for an approximate given mass of tissue at a fixed temperature. The latter will usually be 3 7 °Cor room temperature. In general, a higher enzyme concentration for a shorter time will be equivalent to a lower enzyme concentration for a longer time (Bowman and
120
PREPARATION AND STAINING
Mclaren, 1970a,b). However, this must always be determined experimentally for every given system to check that the desired result, e.g. viability versus yield, which frequently are inversally related, is being achieved. At the conclusion of the incubation time the reaction must be stopped. This can be effected with cooling to 4°C, dilution and washing as well as with inhibitors. If yield is unimportant it is often possible to achieve increased viability by using an excess of tissue compared with enzyme as the latter is always 'used-up' to some extent in the reaction. If viable cells are required it is obviously impossible to use pepsin which has a pH optimum between 1.5 and 2.5 as the preparation must be kept close to neutral. Trypsin, pronase (also called neutral protease) or collagenase are used most frequently for this purpose. The pH optimum of trypsin is between 8.0 and 8.5 but it is still effective at neutral pH and it can also be used with EDTA. Ca2 + and Mg 2 + cations play some part in maintaining the integrity of intercellular binding (Waymouth, 1974). Hence, the addition of EDTA which chelates divalent cations will tend to destabilize intercellular connections. Increased yields with shorter incubation times are often obtained with the addition of EDTA to trypsin even though this tends to reduce the activity of the enzyme. Collagenase, however, must never be used with EDTA as Ca2 + ions are required for enzyme activity. The disaggregation efficiency of trypsin is well established and it is used as a routine in our department for the majority of animal tumours and for tissue culture cells which grow as monolayers. However, we tend to use pronase for human tumours as a good yield with higher viability is obtained compared with trypsin or collagenase. If all that is required from the disaggregation is a suspension of isolated nuclei for DNA staining then pepsin, which digests cytoplasm, is the enzyme of choice. Both fresh and fixed tissue can be dissociated. The pepsin concentration required for cytoplasmic digestion to release nuclei varies with tissue type but this usually will be between 0.01 and 1 mg ml" \ This is a very wide range and the optimum concentration and incubation time for particular applications can only be determined experimentally. The chopped tissue is incubated at 37°C in hydrochloric acid (HCl) at pH 1.5—2.5 containing the pepsin which must be made up fresh as required. A number of pepsins are available from various manufacturers, don't get the cheap stuff, it doesn't work. The preparation should be chromatographically purified, crystallized and lyophilized. This is the more expensive variety and Sigma (St. Louis, Missouri, USA) do a good one. The stock bottle must be kept at or below 0°C and it goes off very quickly if you get water in it. 7.1.3
Wax embedded material This technique was introduced by Hedley et al (1983) to assay for DNA content in nuclei extracted from archival clinical biopsies. However, it can also be used to assay for DNA and nuclear associated antigens simultaneously with very little modification (Watson, Sikora and Even, 1985; Bauer et al., 1986a; and see section 7.3.4, chapter 12 and section 15.2). Briefly, 40-50 |im sections are cut on a microtome and these are dewaxed and rehydrated by sequential treatment with
DISAGGREGATION
121
Embedded wax block
40 Jim slices
Dewax in Xylene and rehydrate
Pepsin digestion
Isolated nuclei Figure 7.1. Schematic of the dewaxing and pepsin digestion procedure for archival specimens.
washes in xylene then 100% ethyl alcohol followed by rehydration with washes in decreasing concentrations of alcohol. Many have their own minor modifications of this technique and our dewaxing procedure is carried out with a minimum of two washes in xylene. Approximately 5 ml of xylene are used for each thick section measuring about 1.5 x 2.0 cm. The section(s) is placed in a glass test tube (this is important as many plastics dissolve in xylene), 5 ml xylene are added and the test tube is aggitated. By looking obliquely through the test tube it is possible to see the wax dissolving in the solution by the refractive index changes which occur as dissolving takes place. After about 5 minutes the xylene can be poured off leaving the tissue section adherent to the test tube wall by surface tension. A further 5 ml xylene are then added as a washing procedure and this too is similarly poured off after a further 5 minutes. Water-free 100% ethanol is then added, the test tube is agitated for 1 to 2 minutes, the supernatant is poured off and a further 5 ml 100% ethanol are added for 5 minutes with intermittent agitation. During this step the tissue section will change from being translucent to opaque. The supernatant is again poured off and a further aliquot of ethanol is added for 1 to 2 minutes. Then 1.0 ml is removed with a pipette and replaced with 1.0 ml distilled water added drop-wise with inversion mixing. This gradually reduces the alcohol concentration to 80%. If the dewaxing process has not been complete the supernatant will become cloudy during this initial rehydrating step, in which case the alcohol is removed, replaced by 100%
122
PREPARATION AND STAINING
ethanol then by xylene to complete the dewaxing. If all xylene and wax have been removed the supernatant will remain absolutely clear during initial rehydration which can then proceed by sequentially pipetting off aliquots of supernatant and replacing this with equal volumes of distilled water thus gradually reducing the alcohol concentration. When the latter has reached about 10% it can all be removed and the section is washed in distilled water, then resuspended in phosphate buffered saline (PBS), pH 7.2. The rehydrated tissue is finally incubated at 37°C in 5 ml acid—pepsin as described in section 7.1.2 and a summary of the procedure is shown in figure 7.1. Most sections required a digestion time between 45 and 60 minutes with frequent agitation and mixing after which the solution will appear colloidal. One to four sections, depending on the size of the biopsy, are usually adequate to obtain sufficient nuclei. A small minority of sections fail to digest adequately even after prolonged incubation. These tend to be sections which are difficult to cut and contain very dense sclerotic fibrous tissue and calcification. Occasionally, these are more efficiently disaggregated with collagenase. Following partial digestion to release nuclei the material is filtered through a 35 (im nylon mesh, centrifuged at 200 G and resuspended in PBS, pH 7.2, at a concentration between 5 x 105 and 106 nuclei ml" 1 .
7.2
Permeabilization
Most highly polar dyes and large molecules, such as antibodies, do not cross functional external membranes of viable cells. Thus, in order for such ligands to gain access to intracellular components the external membrane has to be removed or permeabilized. 7.2.1
Fixation This term derives from the histopathologist's requirement that tissues be rendered sufficiently robust to withstand embedding and sectioning procedures. The process also preserves tissues from both external micro-organism attack and internal enzymatic lysis by destroying the functional capacity of enzymes. It is one of the processes used in flow cytometry, where live cells are not required, which enables highly polar fluorochromes to gain access to the cell's interior. The main effects of fixation include polymerization and cross-linking, which precipitate, denature and stabilize proteins. Classically, fixatives have been described as 'agglutinating' and 'non-agglutinating' which are terms derived from observations of the behaviour of plasma proteins to the various agents. The former group includes ethanol, methanol and acetone and the latter group includes acetic acid and the aldehydes namely formaldehyde, paraformaldehyde and gluteraldehyde. The mechanisms involved in fixation have been reviewed comprehensively by Hopwood (1985). Many different fixation protocols with methanol, ethanol, acetone, formaldehyde and paraformaldehyde have been used in flow cytometry and each has advantages and disadvantages. The aldehyde fixatives react with amine groups
PERMEABALIZATION
123
found within cells and can form fluorescent complexes. These fixatives should be avoided if the expected signals, for example in immunofluorescence work, are likely to be 'weak'. Gluteraldehyde in particular can cause considerable background green fluorescence. Paraformaldehyde, however, has been used very successfully for many such assays. The agglutinating fixatives, e.g. the alcohols, can produce considerable clumping as might be expected. For most purposes 50% methanol is adequate and our practice is to add an equal volume of 100% methanol one drop at a time to the single-cell suspension with continuous agitation as addition of fixative 'too quickly' can cause severe clumping of some cell types. The fixation process can also cause major problems in immunofluorescence staining with reduction or loss of antibody binding due to epitope modulation induced by the fixation (van Ewijk et al, 1984). These problems seem to arise most often with formaldehyde, particularly if this has not been buffered. Methanol (Elias-Jones et al, 1986; Jacobberger, Fogleman and Lehman, 1986; Levitt and King, 1987) and paraformaldehyde (Clevenger, Bauer and Epstein, 1985) have both been used for staining intracellular antigens using immunofluorescence techniques. Epitope modulation of cell surface antigens by fixation can be overcome by staining the cells prior to fixation (van Ewijk et al, 1984).
7.2.2
Hypotonic lysis
This technique, which was discovered by accident (Awtar Krishan, personal communication) as are many discoveries, was introduced by Krishan in 1975. Cells were centrifuged to a pellet, the supernatant was removed and the sample was resuspended in a solution containing 0.1% sodium citrate and propidium iodide at a concentration of 5 mg 100 ml~ \ Propidium iodide is a nonspecific nucleic acid fluorochrome (see section 11.1.2) which stains both DNA and RNA and in order to obtain an uncontaminated DNA histogram the RNA has to be removed. In fixed cell preparations this is effected by the addition of ribonuclease and the attraction of Krishan's method was that the majority of the contaminating RNA is located in the cytoplasm which was lysed by hypotonic treatment. The method works well for cells which are easily lysed by this treatment and which do not have appreciable quantities of nucleolar RNA. However, not all cell types can be lysed adequately by the method originally introduced by Krishan (1975), and Fried, Peres and Clarkson (1976) added triton X-100 to hypotonic citrate which improved the procedure. These same authors showed later (1978) that the hypotonic citrate/triton X-100 method was also capable of releasing nuclei directly from monolayers.
7.2.3
Detergent
Non-ionic detergents (NP-40 or triton X-100) can be used at low concentrations to permeabilize the external membrane to allow passage of polar fluorochromes and antibodies through to the interior of the cell. Concentrations within the range 0.01% to 0.1% in PBS will usually preserve the gross integrity of the external membrane (Hunt, Pini and Evan, 1987), but higher concentrations
124
PREPARATION AND STAINING
(0.1% to 1%) will cause cytoplasmic lysis (Taylor, 1980; Thornthwait, Sugarbaker and Temple, 1980). The rapid staining method developed by Taylor (1980) can be used with a number of fluorochromes and the technique involves using a stock solution containing 4.0% triton X-100 and either propidium iodide or ethidium bromide at concentrations of 40 mg 100 ml~ \ One part of this solution is added to 7 parts of growth medium containing the cells at a concentration of 106 ml~ 1 . This gives final concentrations of 0.5% and 5 mg 100 ml~ 1 respectively for triton X-100 and PI or EB. Ribonuclease can also be added to this solution to remove any nucleolar RNA (Tate et al, 1983). Some care needs to be exercised with this method if dual staining using antibody probes for nuclear associated antigens is undertaken as binding of some antibodies can be inhibited using relatively high concentrations of non-ionic detergents. Thus, pilot studies using a range of concentration and conventional microscopy should be undertaken as part of the work up.
7.2.4
Freeze-thaw
A freeze—thaw technique, adapted from the method described by Ganesan, Smith and van Zeeland (1981), has been developed in our laboratories (Smith, Nakeff and Watson, 1985) which can be used to study DNA as well as nuclear-associated antigens. It can be used for both monolayers and suspension cultures but it was primarily designed for the former. Monolayers are washed twice in phosphate buffered saline (pH 72), drained well and overlayed with low salt (LS) buffer. This contains 10 mM NaCl, 10 mM EDTA, l.Omgml" 1 bovine serum albumen in 10 mM Tris-HCl buffer pH 8.0. The quantity of-buffer added to each flask after removal of the medium depends on flask size and should be just sufficient to completely cover the monolayer. Flasks of 75 cm2 require between 1.5 and 2.0 ml and 150 cm2 flasks need about 3.0 ml. The flask is then frozen rapidly in a horizontal position by immersing the lower half in a dry ice/methanol bath. The frozen monolayer is then thawed rapidly in a water bath at 3 7 °C.Most cells detach from the plastic surface after the first freeze—thaw cycle but some will still be adherent and many will be in 'sheets' if the monolayer was relatively dense. A second freezing is then carried out after which the frozen cells can be kept at — 70 °C for up to six months (maximum time investigated to date) if necessary. A single-cell suspension suitable for immunofluorescence and propidium iodide staining can then be obtained by gentle syringing or pipetting after the second thawing. Inevitably, there are some clumps using this method so filtering through 35 |im nylon mesh is always advisable. Suspension cultures are treated similarly except that the pellet is resuspended in LS buffer after centrifugation and growth medium removal. Thereafter, the resuspended cells are then subjected to two cycles of freeze—thaw as above. This method was designed to avoid both detergent treatment, which might interfere with subsequent antibody binding, and fixation which can modify or destroy some epitopes rendering those samples useless. Moreover, it also enables samples to be stored. It depends on mechanical sheer stress to puncture the
STAINING
125
external membrane due to ice crystal formation during rapid freezing and most epitopes should be preserved. 7.2.5
Lysolecithin Lysolecithin is a naturally occurring lipid with profound actions on the external cell membrane. It probably replaces phospholipids in the membrane bilayer (Weltzien, 1979) and at high concentrations this leads to lysis. At low concentrations, which should be determined experimentally for each cell type, lysolethicin can be used to permeabilize cells sufficiently to allow access of large molecules whilst maintaining the gross integrity of the membrane. Schroff et al (1984) introduced this permeabilization technique in flow cytometry, but it had been used previously in transfection studies (Miller, Castellot and Pardee, 1979). Schroff et al (1984) used concentrations of 50 [ig ml" 1 which allowed access of anti-IgM antibodies to chronic lymphatic leukaemia cells and anti-intermediate filament antibodies to peripheral blood lymphocytes. Following lysolecithin treatment there was partial loss of light scatter signals with forward more affected than 90° scatter. However, a good discrimination was still maintained between lymphocytes and monocytes (see section 10.2). Dent et al (1989) have also used lysolecithin very effectively for analysis of intracytoplasmic and nuclear associated antigens.
7.3
Staining
As yet, there is no universally satisfactory or accepted classification for staining techniques. However, the methods can be divided into three operational categories. The first category includes fluorochromes which are coupled covalently to antibodies to probe specific molecules. Fluorescein and rhodamine, emitting green and orange/red fluorescence respectively have been most commonly used in these types of applications. More recently, phycoerythrin (blue light excited red fluorescence; Glazer and Stryer, 1984) and aminomethyl coumarin acetic acid, AMCA, (UV light excited blue fluorescence; Khalfan et al, 1986) have further increased the range of studies that can be contemplated using antibody (Watson et al, 1987b) and hybridization probes (Nederlof et al, 1989). Secondly, there are fluorescent ligands which interact with a cellular constituent, or the microenvironment within the cell, to release the fluorophore or modulate its emission. This category, which I will refer to as 'interactive7, includes noncovalently binding nucleic acid dyes, pH and calcium probes, and fluorogenic substrates for measuring enzyme activities. Finally, fluorescent dyes can accumulate within the cell either non-specifically or due to binding with a cellular component with an emission spectrum unaltered in either energy or intensity. Examples include fluorescein isothiocyanate (FITC) which binds to proteins, diphenyl hexatriene (DPH) which partitions in lipids, membrane potential and mitochondrial probes and I will refer to this group as 'non-interactive'.
126
PREPARATION AND STAINING
7.3.1
Surface antigens Immunofluorescence staining of surface antigens can be either direct or indirect. In the former, the antibody to the antigenic determinant is directly conjugated with the fluorescent probe, which is frequently fluorescein. In the latter, the specific antibody is not conjugated and a fluorochrome-conjugated second antibody is used to probe the first. Indirect immunofluorescence staining is preferable to direct for three reasons. Firstly, direct conjugation of some monoclonal antibodies with the fluorochrome interferes with their binding specificity. Secondly, it is not possible to carry out easily controls with an irrelevant antibody to determine the degree of non-specific binding with the direct method. Finally, a degree of signal amplification is obtained with the indirect method (see section 7.33). There are literally thousands of published variations on the theme of antigen labelling using antibody probes. However, a basic guide to the principles of indirect immunofluorescence procedures used in flow cytometry are as follows. Step (1) If there is likely to be an appreciable quantity of debris following disaggregation, if this was carried out, the preparation should be 'cleaned-up' using a Ficol—Paque density gradient. Don't ask me to define what 'an appreciable quantity of debris' might be, look at a sample under phase contrast microscopy and decide for yourself. Step (2) Wash the cells twice in phosphate buffered saline (PBS, pH 7.2) containing 1% bovine serum albumen (BSA). In general, viable cells (if that is what you've got) don't like being manipulated in PBS which does not contain some protein hence the reason for the BSA. After the first wash resuspend the cells in 1.2 ml PBS/BSA and split this into six aliquots each of which is placed in a 1.5 ml Eppendorf tube before the second spin. The reason for this will be apparent later. Step (3) Remove the supernatant from each of the six tubes which will then contain the cell pellet plus between 10 and 20 [i\ overlying PBS/BSA. Add 20 JLXI of four different concentrations of antibody solution to four of the tubes and resuspend. As stated earlier (section 25), we used antibody dilutions of 3.16 and 10 but, when the characteristics of a particular batch of antibody have been established only a single dilution is needed. Occasionally, we have found that more consistent results are obtained by adding more than the 20 |il stated above. Then 20 |il of PBS/BSA and an irrelevant antibody are respectively added to the remaining two tubes to act as controls and all six tubes are then incubated for 45—60 minutes. It should be noted that if you want viable cells for subsequent sorting and culturing don't use antibody containing azide. Step (4) At the end of the incubation period add 1.0 ml PBS/BSA to each of the tubes as a washing step, mix well, spin down and remove the supernatant. Step (5) Add 20 |il fluorochrome conjugated antibody to the four tubes which were incubated with the specific antibody and the control tube incubated with the irrelevant antibody. Then 20 |il PBS/BSA should be added to the remaining tube and all six are incubated for a further 60 minutes.
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127
Step (6) Following the second incubation 1.0 ml PBS/BSA is added to each tube to dilute the conjugated second antibody, the cells are spun down, the supernatant is removed and the preparation is finally resuspended in 0.5 ml PBS/BSA ready for analysis and/or sorting. The basic protocol outlined above can be modified at any step to suit particular needs and it should be regarded only as a general guide. It is, however, important to have the two controls where one (irrelevant first antibody) controls for nonspecific binding plus second antibody 'trapping7, and the second (PBS/BSA only) controls for any autofluorescence and light scattering into the fluorescence detector. 7.3.2
Antibody combination staining In order to understand how combinations of antibodies can be used in multi-colour staining methods it is necessary to consider their structure. Antibodies consist of two identical heavy chain polypeptides and two shorter light chains. The basic structure is shown in figure 7.2 where disulphide bonds link the four components to form the whole molecule. The epitope recognition site is at the amino-terminal ends of the heavy and light chains in the variable regions, V n and VL respectively. Light chains are subdivided into two subclasses, lambda (k) and kappa (K), depending on the structure of their constant region, CL. The structure shown in figure 7.2 is a very considerable simplification as, for example,
Figure 7.2. Simplified representation of antibody structure. The variable light and heavy chain regions containing the epitope binding site (BS) are denoted by VH and Vh respectively. The constant light chain region, CL, may be one of two subtypes, X and K. The heavy chain constant regions including the double disulphide bond to the carboxy terminus may be of five types (IgG, IgM, IgE, IgD and IgA) and this section of the molecule is called the Fc fragment.
128
PREPARATION AND STAINING
Fab'
Fc
Fab
Figure 7.3. Antibody digestion fragments. F(ab')2 are composed of both epitope recognition sites and heavy chain constant regions up to and including the double disulphide bond. Fab' fragments contain just one epitope recognition site and a small section of the Fc fragment region. Fab fragments include a single variable region epitope recognition site and the light chain constant region up to and including the single disulphide bond. Fc fragments are composed of the double disulphide bond of the heavy chain constant regions through to the carboxy termini.
the heavy chain is subdivided into a number of different regions and differences in these give rise to different antibody classes (e.g., IgG, IgM, IgA, IgD and IgE). Antibody structure was initially elucidated to some extent by partial enzymatic digestion and preparation from commercial organizations will be of four types depending on how they are prepared. By far the most common is the whole antibody molecule however, antibody fragments, F(ab')2, Fab' and Fab, containing the epitope recognition site produced by partial enzymatic digestion (Male, 1986) are also available and their structures are shown in figure 73 together with that of the Fc fragment. A number of strategies are available for multi-antibody probing. We have assayed for total DNA and the protein products of the c-myc and c-fos genes simultaneously (Watson et al, 1987b) as follows. The c-myc protein was probed with a mouse monoclonal anti-p61 c ~ mK antibody then secondarily stained with a sheep anti-mouse immunoglobulin (IgG) coupled to the UV fluorochrome aminomethyl coumarin acetic acid (AMCA). The c-fos protein was probed with a synthetic peptide induced rabbit anti-serum which was subsequently stained with a fluorescenated swine anti-rabbit antibody (FITC-SocR). Results of such staining procedures are given in section 12.3.4.
STAINING
129
Double antibody staining can also be carried out with K- and ^-Fab fragments recognizing the different epitopes which can then be individually probed with subclass-specific second antibodies each labelled with a different fluorochrome. Third and fourth molecules could also be probed with whole antibody molecules of different class (e.g. IgG and IgM) which would then subsequently be labelled with two further fluorochromes respectively coupled to the class-specific second antibodies. Horan, Slezak and Poste (1986) have produced an ingeneous method for identifying multiple lymphocyte subsets in a single sample using only two fluorescent probes, namely fluorescein and phycoerythrin which are both excited by the 488 nm argon line. The principles of this method are as follows. Two different cell surface molecules recognized by different antibodies can both be identified with a single fluorochrome (e.g. fluorescein) by suitable dilution of one or both of the antibodies so that one gives a weak signal and the other gives a strong signal. This principle can be extended to a two-dimensional procedure using two further antibodies both labelled with the second fluorochrome (e.g. phycoerythrin). Using this technique Horan, Slezak and Poste (1986) were able to identify five different lymphocyte subsets however, all antibodies must be directly conjugated with the fluorochromes. 7.3.3
Fluorochrome amplification Fluorochrome amplification is used to describe the situation where there are two or more fluorophores probing a single target molecule. The term is used almost exclusively in the context of antibody binding. However, it should not be forgotten that it also applies in enzyme reaction kinetics (see section 14.2) where, due to dynamic processes, there are many more fluorophores produced from the substrate than there are target enzyme molecules. The simplest amplification technique uses a non-fluorescent mouse (monoclonal) antibody to recognize the antigen which is then probed with fluorochromecoupled rabbit polyclonal anti-mouse antiserum raised by immunizing rabbits with purified mouse immunoglobulin of the relevant class. The rabbit anti-mouse antiserum will recognize a number of different epitopes on the primary antibody which is depicted in figure 7.4. The rabbit antibody molecules, with the asterisks representing fluorochromes, are shown here as binding just to the Fc fragment of the mouse antibody. But, epitopes on the Fab fragments may also be recognized unless of course the polyclonal antiserum was raised exclusively to the Fc fragment (see figure 7.3). Further amplification can be achieved using a triple-layer technique which is more time consuming as it requires an extra incubation. A primary non-conjugated mouse antibody is used as in the previous example which is then reacted with a non-conjugated rabbit polyclonal antiserum. This would give the same type of configuration as shown in figure 7.4 but without the fluorochromes. The rabbit antibodies would then be probed with a fluorochrome-coupled third antibody raised in sheep or goats and a number of these would bind to each molecule of rabbit antibody.
130
PREPARATION AND STAINING
Fc epitope
Second antibody
Epitope of specific antigei
Figure 7.4. Representation of indirect immunofluorescence labelling with two fluorochrome-conjugated second antibody molecules bound to the Fc fragment of the first antibody which is bound to the antigen being analysed. The fluorochromes are represented by the asterisks. High degrees of fluorochrome amplification can be achieved with the biotin-streptavidin labelling system. Biotin is a low molecular weight watersoluble molecule which can be bound to antibodies in relatively large numbers without modification of the antibody binding properties (Guesdon, Ternynck and Avrameas, 1979). Streptavidin is a protein, isolated from the bacterium Streptomyces avidini, with four high-affinity binding sites for biotin (Chaiet and Wolf, 1964). These biotin binding sites are identical to those in the egg white glycoprotein avidin but the latter suffers from high non-specific binding (Haeuptle et ah, 1983) due, in part, to the carbohydrate group (Green and Joynson, 1970; Green and Toms, 1970). Biotin binding to streptavidin can be inhibited when the former is bound to macromolecules due to steric hinderance; however, this has been overcome by using bridging spacer arms (Bonnard, 1984). The staining system using biotin-streptavidin illustrated in figure 7.5 is essentially the same as in figure 7.4 but the fluorochrome in the second antibody is replaced by biotin with its 'bridge7. The biotin is then probed with streptavidin coupled with a number of fluorochrome molecules. Only one of the four biotin binding sites in the streptavidin is filled in figure 7.5 and further amplification is possible using a biotinolated fluorophore carrier molecule. A fluorochrome amplification technique which gives enhanced sensitivity in flow cytometry has recently been introduced by Truneh and Machy (1987). This
STAINING
131
Fc epitope
Epitope of specific antige Biotin
Figure 7.5. The biotin-streptavidin system. Thefluorochromesof figure 7.4 have been replaced by a 'biotin-bridge'. The biotin is subsequently probed by the addition of fluorochrome-conjugated streptavidin where the fluorochrome molecules are again represented by the asterisks. Streptavidin has four biotin binding sites thus further amplification can be achieved by addition of biotinolated fluorochrome-carrier molecules. was based on work where Leserman et al. (1980) targetted fluorescent liposomes to cells by covalently coupling the liposomes with antibodies or protein-A. Truneh and Machy (1987) constructed two sizes of liposomes (Szoka and Papahadjopoulos, 1978) which respectively contained about 3000 and AOOOOO molecules of the fluorochrome carboxyfluorescein which, because of its polarity, remains trapped within the lipid vesicle. The liposomes were coupled to protein-A (Golding, 1978) and this conjugate was then reacted with the probing antibodies. Fluorescence amplification of greater than 100-fold was obtained with the larger of the two liposomes compared with conventional methods and Truneh, Machy and Horan (1987) have shown that a number of different fluorochromes can be used with this technique for multi-colour immunofluorescence labelling. 7.3.4
Intracellular antigens Intracellular antigens, including those that are nuclear associated, can be assayed with antibody probes after cells have been permeabilized by any of the methods described in section 7.2. Various combinations of fixatives have been used by both Clevenger et al. (1985) and Elias-Jones et al. (1986) in assays for nuclear-associated antigens. The best fixative for a particular antigen and assay
132
PREPARATION AND STAINING
system has to be determined experimentally. There is insufficient knowledge at present to make any generalizations. Clevenger et al. (1985) found that fixation with paraformaldehyde followed by treatment with triton X-100 gave the optimum results with Raji cells, HeLa cells and peripheral lymphocytes. A pellet of 1-3 x 106 cells was resuspended in 10 ml of 0.5% paraformaldehyde (Polysciences, Warrington, PA, USA) in PBS for 10 minutes. After centrifugation at 200 G for 10 min the fixed cells were resuspended in 0.1% triton X-100 (Sigma, St. Louis, Missouri, USA) in PBS for 3 minutes as a washing step, re-centrifuged and resuspended in 0.1% triton X-100/PBS in which all further washes and handling were carried out. Elias-Jones et al. (1986) found that fixation in 50% methanol/PBS for cervical brush biopsy specimens gave satisfactory results. After fixation the staining procedures are identical to those described in the previous section. However, indirect immunofluorescence techniques are recommended for the reasons given in section 7.3.1 as these enable the degree of any non-specific binding or intracytoplasmic or nuclear trapping in permeabilized cells to be determined. A certain amount of luck is needed when using the paraffin wax extraction plus pepsin digestion technique for nuclear-associated antigens. Pepsin has a wide specificity (see* section 7.1.2) but it cleaves proteins preferentially at leucine and phenylalanine residues in hydrophobic domains. It also cleaves at tryptophan and methionine residues again in hydrophobic domains but bonds to tyrosine are refractory to digestion. With antibodies raised to native protein there is no way of knowing in advance if the epitope recognized by the antibody contains residues which are digested by pepsin. If it does you will not see anything, and that is just bad luck. However, monoclonal antibodies can be raised to synthetic peptides corresponding to the primary amino acid sequence of the protein and are often raised to hydrophilic domains (Niman et al, 1983; Evan et al, 1985). Thus, by choosing for antibody production a peptide with amino acid sequences which are deficient in both leucine and phenylalanine and/or relatively tyrosine rich it is possible to minimize the chance that pepsin will digest the epitope. However, it is still possible for the epitope to be lost if bonds either side are cleaved and the epitope floats away into the sunset. So again, some luck is needed. We have also attempted to assay cytoplasmic antigens (in particular p21 N~rflS) from wax embedded material using a variety of proteolytic enzymes in the disaggregation step and have failed totally. Occasionally we seemed to get it to work but when we did we didn't know why. If anyone has managed to do this with any degree of reliability please let me know. 7.3.5
Interactive stains A variety of apparently unrelated dyes have been lumped together under this heading. This may not be the best way to attempt a classification but they have the common property of an alteration in their fluorescence emission on interaction with their target molecules. Most nucleic acid stains (see section 11.1) are highly polar and require
STAINING
133
permeabilization of the external membrane to gain access to the nucleus. Examples of permeabilization methods for the phenanthridinium dyes, which can also be used with the phenylindoles, were given in sections 7.2.3 and 7.2.4 and some of the properties of these groups of ligands are given in sections 11.1.1 and 11.1.2. The exception is the bisbenzimidazole group of dyes (see section 11.1.1) some of which are relatively lipophilic and can be used as vital DNA probes. Apart from the tricyclic heteroaromatic compounds (see section 11.1.3) all of these dyes exhibit a profound increase in the fluorescence emission intensity on binding to the nucleic acids. Intracellular pH and calcium measurements assess functional capability and obviously have to be carried out with intact viable cells. However, the probes for both pH and calcium are highly polar and both need to be preloaded into cells by incubating with the lipophilic acetoxy methyl ester derivatives. After traversing the external membrane the functional probes are released by intracellular esterases which hydrolyse the ester bond. The determinations then rely upon changes in either the intensity or energy of the emission spectrum which can be analysed on two photomultipliers simultaneously (see sections 8.4.1 and 8.4.2). Assays for functional enzyme capacity using a variety of substrates, most of which are fluorogenic (see section 14.2.1), must also be carried out with intact viable cells. Again, in order to gain access to the cell interior they have to be lipophilic. Care must be taken for assays involving membrane enzymes after any procedures involving enzymatic disaggregation to obtain the single-cell suspension as this may alter the functional capacity of the test system.
7.3.6
Non-interactive stains
The dyes included in this category are essentially unchanged when they enter the cell. Fluorescein isothiocyanate binds non-specifically to proteins and has been used to assay for total protein in fixed cells. It can also be used in viable cells but this just gives a measure of membrane proteins as FITC is polar and does not readily cross the intact external cell membrane. Lipid probes, such as diphenylhexatriene (DPH), partition non-specifically into lipids and these cannot be used after fixation with agents which dissolve fats, e.g. alcohols and acetone. Membrane potential stains (section 14.3) are charged symmetrical molecules with hydrocarbon side chains. These probes retain lipophilicity as the charge is not localized and the relative lipophilicity can be engineered by changing the length of the side chains. Assays can only be carried out in viable intact cells and changes in membrane potential allow influx or efflux of these ligands which are monitored by changes in the signals. Mitochondrial function can also be assayed in viable cells using the probe rhodamine-123 which crosses the functional external membrane (see section 14.5). It has been described as a specific mitochondrial dye but, this is not strictly correct as it partitions into any electro-negative environment. However, the interior of functional mitochondria is very electro-negative and hence the dye tends to accumulate within them.
134
PREPARATION AND STAINING
7.3.7
Stoichiometry
Stoichiometric binding in flow cytometry refers to the state where the quantity of fluorescent light emitted from a bound dye complex is directly proportional to the quantity of the target molecule. Ideally, all, or very nearly all, the free binding sites should be complexed with dye. Stoichiometry is defined in the Chambers Twentieth Century Dictionary (1976) as 'the branch of chemistry
that deals with the numerical proportions in which substances react' (Greek, stoicheion, an element; metron, measure). Such considerations are important in all fluorescence measurements but are particularly important when measuring DNA, for example. Flow cytometers measure fluorescent light from DNA and not DNA directly. The emitted fluorescence is directly proportional to both the number of dye molecules bound to DNA and the quantity of exciting light which is actually absorbed by those molecules in the dye/DNA complex. The most important processes are shown in figure 7.6 represented as one would represent a biochemical process such as an enzyme reaction. It may seem a little strange at first sight to represent the emission of fluorescence as one would normally represent an enzyme reaction. However, the two processes have similarities particularly if you allow your mind to consider them just as manifestations of energy transfer systems which is what they are. The various components represented in figure 7.6 and the processes which affect those components are as follows. Dye and DNA represent unbound molecules, which in DNA are the available and free binding sites. These may combine with rate constant kx to form the dye/DNA complex denoted by CX. Once CX is formed it could dissociate and revert to free dye and unbound DNA in the 'back-reaction' with rate constant k-v When light excites this system a number of processes can take place. CX can 'combine' with exciting light, Ex, with rate constant k2 to form the excited complex CX*. This can then emit fluorescence, EmC, which is what we want to measure, with rate constant k3. However, four possible quenching processes involving CX* can also take place. Firstly, the excited complex may revert to the non-excited state, CX, by non-radiative energy transfer within the bound molecular complex with rate constant k-2. Secondly, CX* may also dissipate energy to the microenvironment, ME, by non-radiative transfer with rate constant k4. Thirdly, resonant energy transfer (RET) may take place with rate constant k5 if there is an appropriate acceptor molecule (see section 3.8.4). Finally, CX* may disintegrate due to photolysis, P (absorbing further photons whilst in the excited state, section 3.8.4), with rate constant k6. Free dye may also be raised to the excited state, D*, with rate constant k7 and radiate energy as fluorescence, EmD, with rate constant fc10 giving rise to some 'background' light noise. Four quenching processes, directly analogous to those considered above, can also take place. Firstly, the excited dye may revert to the non-excited state by non-radiative energy transfer within the molecule with rate constant lc_ 7. Secondly, D* may dissipate energy to the microenvironment, ME, by non-radiative transfer with rate constant k8. Thirdly, RET may take place with rate constant k9 and finally, D* may disintegrate due to photolysis, P, with rate constant k^.
DNA DENATURATION
135
EmD EmC
Figure 7.6. Representation of the processes involved in dye to DNA binding, absorption of light, fluorescence emission and quenching (see text for explanation).
Although DNA has been used as the example here the same considerations apply to any fluorophore which binds to a cellular constituent. The process of binding and any attendent changes in electron configuration of the fluorophore or of the microenvironment can modulate the fluorescence emission. These factors must always be considered when interpreting fluorescence data quantitatively be this in flow cytometry or in more conventional analytical systems.
7.4
DNA denaturation
A number of techniques require DNA to be denatured. These include monoclonal antibody staining for bromodeoxyuridine incorporation and acridine orange staining to discriminate between interphase and metaphase cells. Antibodies to the bromodeoxyuridine/DNA complex generally only recognize the analogue in single-stranded DNA and techniques for the denaturation include formamide or HC1 plus heating (Dolbeare et al, 1983,1985; Moran et al, 1985; and section 11.5.5). Discrimination between interphase and metaphase cells using acridine orange relies upon the differential colour fluorescence from the dye bound to single- and double-stranded nucleic acids (Darzynkiewicz et al, 1977b; and section 11.1.3). Any method of denaturation can induce considerable disruption
136
PREPARATION AND STAINING
and disintegration of nuclei if it is 'overdone7 or if the nuclei are insufficiently fixed and caution must be exercised with these methods.
7.5
Filtering
It should not be necessary to state that most cell preparations should be filtered before they are run through the instrument; however, this does not seem to be general standard practice. Many preparative methods produce some clumping and debris and most flow chamber injection needles and nozzles are between 50 and 70 |im in diameter. Cells will range in diameter from 10 to 20 |im which means that there is not a large margin to play with. A clump of 4—6 cells each of 15 |JJTI in diameter will block many nozzles or, at best, cause a profound disturbance to the flow characteristics in the chamber thus degrading the data and large particles can profoundly alter the droplet break-off point in cell sorting (Stovel, 1977). It was previously stated in section 6.5, and is worth repeating, that little slivers of plastic scraped off from petri dishes during harvesting with a glass pipette can give rise to nozzle blockages. It is always worth the few seconds it takes to filter the preparation through a 35 |lm nylon mesh before introducing it into the instrument. Some systems incorporate 'in-line' filters but these are not always easy to change and they frequently become clogged up. We use a small plastic filter funnel where the majority of the spout has been cut off leaving a 1.0 cm 'stump' over which is wrapped the nylon mesh held in place by an 'O'-ring. It only takes a further few seconds to remove and wash the mesh between samples.
8 Miscellaneous techniques
The first two techniques described in this chapter, namely slit-scanning and multiangle light scatter, are very specialized and not yet available to the majority of users. Nevertheless, they are potentially important and beginners in flow cytometry should at least be aware of their existance and consequently I've included a brief summary of each. Rare-event and fluorescence emission spectrum analyses are also included in this section. The former presents particular statistical problems, although anyone could have a shot at it with a standard instrument and the latter can be performed on most instruments as long as they are equipped with the correct filter combination.
8.1
Slit-scanning
Slit-scanning is a term used to describe interrogation techniques where different parts of the object are sequentially illuminated and/or observed during their passage through the exciting beam. This can be achieved either in the object or the image plane and the recordings enable the shape of objects to be reconstructed. Progress in this area of flow cytometry has, to a large extent, been pioneered by Wheeless and colleagues in development of automated methods for cancer prescreening (Wheeless and Patten, 1973a,b; Wheeless, Hardy and Balasubramanian, 1975; Cambier and Wheeless, 1975; Cambier et al, 1976). 8.1.1
Object plane slit-scanning Object plane slit-scanning applies where the vertical dimension of the excitation beam is physically smaller than the object being illuminated. It was first encountered in section 3.9.6 where the differences in fluorescence intensity from crossed cylindrical lens pair focussed excitation was compared with that from spherical lens focussing. Object plane slit-scanning means that only part of the object is being illuminated at any given instant which is why we have to integrate the area under the pulse to obtain quantitation of the total number of fluorochromes being excited. Measuring pulse height (proportional to peak concentration), integrated area (total quantity) and pulse width (time-of-flight through the beam) simultaneously for each pulse requires fairly fast, but standard,
138
MISCELLANEOUS TECHNIQUES Cell
Laser beam
Direction of flow
Cytoplasm ^Nucleus*-
I
Time
Cell enters beam
Cell leaves beam
Figure 8.1. Slit-scan profile of a cervical epithelial cell stained with acridine orange (after Wheeless et al, 1984). electronics. Typically, the time-of-flight through the beam will be between 1 and 5 |is. With 'fast7 electronics, including the analogue-to-digital conversion step, it is possible to obtain a number of readings, or digitization steps, of the voltage heights above the base line from the photomultiplier during the time that the object is traversing the illuminating beam. A representation of a fluorescence slitscan profile from a cervical epithelial cell stained with acridine orange is shown in figure 8.1 where the points represent the digitizations of the voltages from the PMT. By joining up these points we obtain a 'fried egg' shape where the flatter portion corresponds to cytoplasm and the bump corresponds to the nucleus. The total width of the pulse from the cell shown in figure 8.1 is equal to the diameter of the cell plus the depth of the focussed laser beam and the 'bump', due to the nucleus, is equal to the diameter of the latter again plus the focal depth. Reconstruction of pulse shapes from data such as these has enabled Wheeless et al. (1984) to determine nuclear to cytoplasmic ratios for use in cervical screening (see
SLIT-SCANNING
139
section 15.1.2). Further examples are shown in figure 82 which are chromosome profiles where the 'dips' represent the centromeric region from which there is less fluorescence. Using data such as these Joe Gray and colleagues at the Lawrence Livermore Laboratories are developing automated methods to determiner centromeric indices (Lucas et al, 1983; Lucas and Gray, 1987; and see chapter 13). Dividing up each pulse into say 128 numbers means that the electronics must be able to digitize at a maximum rate of 10 8 Hertz whilst the object is traversing the beam. This is once every 10 ns and modern electronics can cope with this very adequately. However, for higher resolution work where more recordings are made per object, and there are potential applications for this in high resolution chromosome scanning, we must start paying particular attention to the response time of the photomultiplier as well as the electronics. The response time of a photomultiplier is expressed as the time taken for the voltage to build up to half its maximum height (the half-rise time) and in most regular PMT tubes this is between 1 and 5 ns. This is fine for a maximum digitization rate of 108 hertz but not if we want to digitize an order of magnitude faster and take 1024 readings per object where we would have to have very fast photomultipliers (they are expensive). Potential applications of high resolution chromosome slit-scanning include gene and restriction enzyme mapping and the latter could possibly be used for automated restricted fragment length polymorphism (RFLP) analysis. So far we have considered scanning in the object plane from only one direction, at 90° to the intersection of the cell stream with the beam. The 'beam' in all these types of application must be a laser because of its focussing characteristics; it is impossible to focus a non-coherent light beam down to such small dimensions. Wheeless et al. (1984) have also developed techniques to slit-scan in the axial
A r\
v \ / 5
h I\
\ 6
7
Figure 8.2. Slit-scan profiles of chromosomes (after Lucas and Gray 1987).
8
140
MISCELLANEOUS TECHNIQUES Cell image on CCD array Hydrodynamic focussing
Flow chamber
Laser beam
Figure 8.3. Axial slit-scan setup with CCD array placed horizontally across the direction of flow in the forward direction (Wheeless et al., 1984, redrawn from original diagram supplied by Professor Leon Wheeless, with thanks). The cell and CCD array are not to scale, and a band-pass filter has been omitted for clarity.
direction, which is along the axis of the beam. The detector in this technique is a linear array of charged-coupled devices (CCDs) located at a distance from the analysis point. This is arranged horizontally across the flow direction and the magnified image of the object is focussed and imaged on to the detector array. Figure S3 shows the set up where we can see that fluorescent light emitted from only a specific Vertical slice' through each cell will fall on each element of the CCD array. As the cell passes through the beam the charge builds up in each element of the CCD array which can then be digitized after the cell has passed out of the beam. The direct analogy to this in classical fluorescence microscopy would be to draw a number of vertical grid lines through the image of a cell and measure the quantity of light emitted between each set of lines. Wheeless et al. (1984) have combined axial with 90° slit-scanning where the former gives shape information by virtue of detector position and the latter gives shape information by virtue of resolving measurements in the time domain.
8.1.2
Image plane slit-scanning
In image plane slit-scanning the illuminating focal volume is larger than the object and this technique is used with spherical lenses where the fluorescence or light scatter image is focussed onto a slit. This can be best explained using another microscope analogy where there is a slit placed horizontally across the image plane so that only a narrow section of a cell can be seen at any one time. In order to view the whole of the cell the stage of the microscope would have to be moved vertically enabling sequential 'slices' of the cell to be seen in the slit. The
MULTI-ANGLE LIGHT SCATTER
141
Object plane
T
S
Figure 8.4. Imaging onto a slit demonstrating the principles involved in image plane slit-scanning.
principles involved are illustrated diagramatically in figure 8.4 where only light emitted from the cell along the central optical axis (horizontal dotted line) passes through the slit on the right.
8.2
Multi-angle light scatter
The combination of forward and 90° light scatter can be used to distinguish between a number of different cell types without staining (see chapter 10). Successes using two-parameter light scatter prompted the development of multiple-angle measurement to investigate the possibility of gaining increased discriminatory capacity and two techniques have been developed.
142
MISCELLANEOUS TECHNIQUES Jet containing cells Scattered light
Detector Mask with aperture
Figure 8.5. Sweep-scan system of Loken et al. (1976) with an expanded laser beam where the light scattered through the slit is from increasing angles as the cell passes through the illumination source.
8.2.1
Sweep-scanning
This is essentially slit-scanning in the image plane which was introduced by Loken, Sweet and Herzenberg (1976) and their setup is shown in figure 8.5. The cells were illuminated by an expanded laser beam at an angle to the cell stream. As the cells travelled through the beam they scattered light at different angles through the slit towards the detector. On entering the beam the scattering angle towards the slit was approximately in the forward direction but, on exit from the beam the scattering angle was approximately at 50°. The detector voltages, reflecting the changing light intensity scattered at increasing angles as the cell travelled through the beam, were digitized and the results enabled discrimination to be made between a number of different leukocytes without staining (see chapter 10).
8.2.2
Multi-detector
Multi-angle light scatter measurements were made on individual cells in brain white matter preparations in a static microscope based system by Meyer et al. (1974) where discriminatory scatter patterns were obtained for red cells, debris and oligodendroglial cells. Similar detectors, consisting of radial arrays of solid-state devices were used by Salzman et al (1975a) to obtain light scatter data at 32 angles between 0° and 19° in the forward direction and at angles between 175° and 177° in the back scatter direction. Two major difficulties, namely orientation dependent scatter and data handling, arise with multi-angle light scattering measurements and these also are discussed in chapter 10.
RARE-EVENT ANALYSIS
8.3
143
Rare-event analysis
Rare-event analysis constitutes a considerable problem even for flow cytometry and there are two basic problems which have been addressed by Cupp et al (1984), Ryan et al. (1984) and Corsetti et al. (1987). The first is a statistical problem concerned with the number of cells that have to be counted which depends on how rare the rare-event is. The second is a discriminatory problem between the rare-events and the remainder.
8.3.1
Statistics
In the introduction to the book an example of manual cell counting was given where 5% of the population was positively labelled. It was stated that due to statistical factors the precision of the estimate depended on how many cells the investigator was prepared to count. Cells are arranged at random on the haemocytometer and statistics governing their dispersion are described by the Poisson distribution. The precision of the estimate of how many cells are labelled is dependent on the Poisson variance which is equal to the number of cells counted and this applies whatever the measurement system, be this a flow cytometer or a haemocytometer. The standard deviation of any distribution is equal to the squareroot of the variance, hence we can calculate the coefficient of variation of the estimate, CVe, for a given number of cells counted, N, where CVe = *JN x 100/N. This is shown in figure S.6 where CVe is plotted on the ordinate versus number of 35
n
30
25 -
20 4> O
15
O O
O
10
10
100
1000
10000
Number of cells counted Figure 8.6. Plot of coefficient of variation of estimate (CVe) versus number of cells counted.
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MISCELLANEOUS TECHNIQUES
cells counted on the abscissa. If 10 cells are counted the CVe is 31.6% but this falls to 1% if 10 000 cells are counted. Let us suppose that the 'rare' event we are attempting to analyse is not too rare and comprises 1 cell in 1000, i.e. 0.1% of the population. If we are prepared to work with a CVe at the 5% level we would have to count 400 rare cells (see figure S.6). However, this number increases to 3000 at a CVe level of 2%, and to 10 000 at a CVe level 1%. Thus, 4 X 105, 3 x 106 and 107 cells would have to be analysed in total to obtain CV of estimates at the 5%, 2% and 1% levels respectively. It's not too difficult to do the calculation if the rare-event is even rarer, say at a frequency of 1:10 000 (0.01%).
8.3.2
Discrimination
The ability to discriminate between the distributions of rare events and the remainder depends on the relative numbers of cells in each distribution, the magnitude of the difference between the mean values and the standard deviations of the two distributions. This is a statistical as well as a biological problem. If we take an example where the CVe has been chosen as 5% we can see from figure S.6 that we will have to count 400 rare cells. Let us also suppose that the CV of the positive and negative distributions are both 30% and that the mean of the negative distribution is in channel 20. We can now calculate the proportions of cells scored as positive by simulating these distributions, varying the mean channel of the rareevent distribution and placing a discriminator between the distributions set 'by eye' as would be carried out with a mono-dimensional fluorescence histogram. This is shown in figure 8.7 where the proportions of cells scored as positive by this procedure are plotted against the ratio of the means of the distributions for the fractions 0.001 and 0.0001 of rare-events in the population. We can see that in order to score 95% of the true positive cells as being positive the mean of the rareevent distribution has to be a factor of 5.0 greater than the remainder, i.e. it must be in channel 100 or higher for the example cited here. However, if the biology is such that the mean of the rare-event distribution is only a factor of 2 or 3 greater than the mean of the remainder we're in trouble. Hence, it is essential in such studies to reduce any non-specific antibody binding signals to an absolute minimum and if necessary amplify the specific signal so that the ratio of the means of the two distributions is greater than about 5 or 6. Furthermore, multi-parameter analysis including light scatter measurements can often help in discrimination (Ryan et al., 1984). The time taken for analysis of populations containing rare-events can be considerable particularly if large numbers of samples need to be analysed. If the rare event is at a frequency of 1:10 000 it will take 1000 seconds running the instrument at 4000 cells s ~ l to accumulate 400 positive cells and obviously a total of 4 x 106 cells would have to be analysed. This would be sufficient for an analytical run but a sorting run where a large number of rare cells are needed for subsequent biological manipulation could take 'for ever' with standard flow rate instruments. In these types of applications very specialized high speed sorters
FLUORESCENCE SPECTRUM ANALYSIS
145
0.001
80-
(0
o a. tn (0 •D
2 60 o o V)
I 40 V) o a
20-
1
2 3 4 5 Ratio of distribution means
6
Figure 8.7. The ratio of the proportion of cells scored as positive to the actual proportion positive plotted against the ratio of the means of the distributions for the fractions 0.001 and 0.0001 of rare events in the population. These data were calculated from simulated monodimensional distributions with a discriminator set 'by-eye' between the distributions.
(Peters et al.r 1985) are required unless a pre-sorting enrichment procedure can be carried out.
8.4
Fluorescence spectrum analysis
We saw in section 3.8 that both light absorption and fluorescence emission are dependent on a number of factors. These include the microenvironment which can change the electronic configuration of a molecule to alter its light absorption spectrum or modulate the emission. The latter may be shifted to different wavelengths or different regions of the emission spectrum may be quenched differentially. Relative changes in the absorption spectrum can be exploited in flow cytometry by using two light sources with different wavelengths (see below); however, this is usually expensive. Changes in the emission spectrum can be assayed much more easily by measuring on two or more detectors
146
MISCELLANEOUS TECHNIQUES
simultaneously where the band-pass filters are designed to coincide with the maximum change in the emission. These approaches have been used to assay intracellular pH, calcium and to study how cells handle vital dye binding to their DNA.
8.4.1
pH
Positive ions can bind to a number of fluorochromes with a resulting modification of their electronic configuration which can lead to changes in either the absorption or emission spectrum. This property can be exploited in flow cytometry to give a measure of intracellular pH due to binding of H + ions. The absorption spectrum peak of one such probe, 6-carboxyfluorescein (6-CF), is close to the 458 nm argon line at low pH but increases to close to the 488 nm line at higher pH (Thomas et al., 1979); however, the position of the peak of the fluorescence emission shows little change with pH (Martin and Linquist, 1975). Hence by using two argon lasers tuned to these lines at the same power output and analysing the same cell sequentially we can obtain a ratio of the fluorescence emission at the two excitation wavelengths which is proportional to pH. Two major problems arise with this approach. Firstly, 6-CF is highly polar and does not readily traverse the external cell membrane and secondly, the expense of two lasers tunable to the required wavelengths is considerable. The first problem is resolved by loading cells with the di-acetate derivative, 6-CFDA, which is highly lipophilic and readily crosses the cell membrane. Intracellular esterases then release the 6-CF which remains trapped in the cell due to its polarity. Secondly, although the position of the peak of the emission spectrum of 6-CF does not change with pH, the relative magnitudes of the emission at 520 nm and 620 nm do show changes (Musgrove, Rugg and Hedley, 1986). Valet et al (1981) developed a similar technique using the di-acetyl derivative of 2,3-dicyano-l,4dihydroxybenzene (DCDHB) which shows an emission spectrum shift from about 450 nm to 480 nm as pH increases (Kurtz and Balaban, 1985). A measure of pH is obtained as follows. Cells for a calibration curve are preloaded with the lipophilic acetoxy derivative of the pH probe and are then treated with the ionophore nigericin in buffers of varying pH. The ionophore allows equilibration of the internal and external H + concentration. Fluorescence measurements for each cell are obtained at two wavelengths simultaneously, the ratio is calculated and a histogram of the latter is obtained which varies with pH. The test cells are then similarly analysed in PBS at physiological pH without the addition of nigericin which maintains the pH differential across the cell membrane. The ratio histogram for the test cells can then be compared with those obtained for the calibration curve. Examples of this type of assay are shown in figure S.S. In panel A the di-acetyl derivative of the probe DCDHB (Valet et al, 1981) was used and the histograms were obtained as the ratio of the emissions at 425 nm and 540 nm using UV excitation. 6-CFDA with 488 nm excitation was used in panel B and the histograms were obtained as the ratio of the emissions at 520 nm and 620 nm. The
FLUORESCENCE SPECTRUM ANALYSIS pH 8.0
147
pH 6.0
7.6
C
o O O
Fluorescence Ratio Figure 8.8. Fluorescence ratio histograms at the buffer pH indicated in the presence of the ionophore nigericin, non-stippled histograms. Panel A, 425nm:540nm ratio for cells treated with DCDHB; panel B, 520 nm:620nm ratio for cells exposed to 6-CF. Stippled histograms obtained without nigericin. These data form the basis of a calibration curve for non-ionophore treated cells which are then loaded with the acetate derivatives of the compounds. The position of the ratio histogram of the test sample, e.g. the stippled histograms, gives the intracellular pH and the range within the population. Data taken from Musgrove et a\. (1986) with permission from the editor of Cytometry.
stippled histograms in each panel were obtained from the test cells without nigericin and the unstippled calibration histograms were obtained with nigericin at varying pH as indicated against each histogram. 8.4.2
Calcium Calcium participates in the regulation of many cellular functions including signal transduction across the external membrane (Campbell, 1983), and a number of fluorescent probes which chelate calcium with high affinity have been developed. As with pH probes, the addition of positive Ca2 + ions causes shifts in either the absorption or emission spectra which can be detected using similar techniques to those described above for pH measurement. These probes are all highly polar and are again loaded into cells using the acetoxy derivatives which rely upon esterases to release the probe. Quin-II (Tsien, 1980) and its analogue Fura-II (Grynkiewicz, Poenie and Tsien, 1985) exhibit absorption shifts on binding calcium. As with pH measurements this is not ideal for FCM; however, Indo-1 (Grynkiewicz, Poenie and Tsien, 1985) shows an emission spectrum shift on binding Ca2 + which can be monitored by simultaneous analysis at 400 nm and 480 nm. The ratio of the emission intensities at these wavelengths is proportional to the quantity of Ca2 + chelated.
148
8.4.3
MISCELLANEOUS TECHNIQUES
DNA The fluorescence emission from nucleic acids stained with acridine orange is metachromatic with single and double strands giving rise to red and green fluorescence respectively (see section 11.1.3). This is a somewhat gross example of a binding-dependent change in the fluorescence emission spectrum of the dye—nucleic acid complex. A suspicion that other fluorescent DNA ligands might give rise to similar, or related, phenomena was raised when Alex Nakeff spent a sabatical in our laboratories in 1982. He is interested in megakaryocytopoiesis and we were involved in experiments designed to study megakaryocyte maturation and kinetics using the vital DNA stain Hoechst 33342. A sample of bone marrow was extracted, stained and run through our instrument but we did not see the expected histogram profile. The experiment was abandoned and repeated the next day but again, we saw the same 'abnormal' pattern. After a little thought we realized that there were three differences between the analysis system in our instrument compared with a B-D FACS 440 which Alex had used previously. First, we were using krypton UV (337 + 356nm excitation) as opposed to argon UV (356 + 363 nm). Secondly, the 'abnormal' profile was obtained with the sample analysed in the flow chamber as opposed to stream-in-air, and finally the filter combinations were different. Our analysis was being performed with a blue/green (490-560 nm) filter combination compared with indigo/blue (420-490 nm) used previously. We switched photomultipliers to analyse on the 390-460 nm bandpass (violet/indigo) and obtained very nearly the expected profile. A dual parameter assay was then carried out using both the green and violet channels and these results are shown in figure 8.9 where a number of subsets are apparent. Initially, we had some difficulty believing this result even after it had been repeated and we decided to run some instrument checks firstly with microbeads (which didn't show anything wrong) and then with chicken thymocytes. We don't normally use chickens and know very little about them, but someone in another department was using a chicken that day and in the interests of economy we asked for its thymus which we thought would give us a nice homogenous biological control. Surprise, surprise, we didn't see a single peak. Luckily, a DNA chemist and repair specialist, Paul Smith, had recently been appointed to our unit and he suggested repeating the experiment with two dye concentrations as a time course to follow the changes in fluorescence with time on the two wavelength bands simultaneously. These results demonstrated that the fluorescence emission spectrum of Hoechst 33342 stained cells changed with time and these and further results will be discussed in section 11.8.
FLUORESCENCE SPECTRUM ANALYSIS
10UM H34-2 MBM 15MNS 7 JAN 83
149
BM0701. 002 PI
1 4
I0UM H3+2 7 JftN 83
BM0701.002 P1
Figure 8.9. Mouse bone marrow stained with Hoechst 33342 and analysed on both the green (560RF AREA) and violet (440RF AREA) photomultipliers which reveals seven different subsets, three of which are S-phase cells. The major 'Gl' spike is composed of two clusters (top panel) and there is also a smaller 'Gl' population clearly discernable in the top panel. The seventh cluster is seen in the rotated bottom panel just to the left of the major spike.
Instrument performance
The performance of any quantitative instrument depends absolutely on the signalto-noise ratio. A star in the night sky can be seen, and its intensity measured with a suitably equipped telescope, but during the day it is invisible within the noise of the high background light intensity. The signal-to-noise ratio is zero in day light due to the noise. The terrestrially based astronomer is also in trouble at night if there is cloud about. In this case, the signal will be zero and its doesn't matter how low the noise is, you simply will not see anything. If the sky at night is absolutely clear and the telescope is functioning perfectly to its design specification you will be disappointed if you are trying to observe below the detection limit. However, failure to see anything doesn't necessarily mean that there is nothing there. These analogies are not only readily appreciated but also very close to flow cytometry where performance depends on the correct and integrated functioning of all the constituent parts of the instrumentation, light sources, fluidics, mechanics, optics, photodetectors, electronics and computers. Performance also depends on the biological preparation and the question you are trying to answer. The latter is particularly pertinent if the assay involves working close to the detection limit. Even if all these components are functioning correctly and you are well above the detection limit with a 'good' cell preparation the performance may still be suboptimal due to design specification or software deficiencies which do not allow the user either to collect or extract from the data base all the information/that may be needed. One very good example of such a deficiency is the failure of some manufacturers to incorporate adequately the computer time stamp within the data base. In some instruments time is fully implemented in the data base, in others it is not and in some it is only included at the beginning and end of data collection for each sample but not during collection. Hence, if you want detailed kinetic information you have to assume that the biological process being studied behaves linearly during the time that data are being collected. However, if it varies, and that is usually what is interesting, you will never know.
9.1
Noise
Background noise can, and frequently does, occur at every stage in the flow cytometric process in the instrumentation, cell preparation and biology.
NOISE
151
Noise in the instrument may arise in light sources, fluidics, mechanics, optics, photodetectors, and electronics. In turn, each of these components may be dependent on other critical components. These include power supplies for light sources, photodetectors, electronics and computers; pressure control valves for the fluidics; cooling water supply for high power lasers; mechanical adjustments for beam alignment and stability of mountings for lasers, optical components and flow chamber. Some of the commoner sources of noise will be considered here. 9.1.1
Electronic Noise in electronic circuitry is not usually a problem except perhaps in 4-decade log amplifiers where the triggering threshold is set too low. Similarly, noise from power supplies is not usual unless there are components which are 'burning out'. This frequently means that a catastrophic failure is imminent and when it happens it is easy to diagnose as everything stops. The most common electronic noise encountered on a day to day basis is due to photomultiplier high tension voltages being set high in an attempt to score very low fluorescence signals. An example is given in figure 9.1 which shows traces from the photomultiplier monitoring oscilloscope. Cells were being analysed for a surface determinant and these data were obtained from the fluorescence control sample labelled with an irrelevant first antibody and the fluorescenated second reagent. The inverted bottom traces in each panel were from the 90° light scatter detector (488 nm) and the top traces were from the green photomultiplier. The system was being triggered by the scatter detector in the top panel and by the green detector in the bottom panel. In the top panel only green signals, which represented background fluorescence and light scatter, associated with each scatter pulse were recorded by the instrument. The difference between the top and bottom panels is the horizontal 'base-line' under the superimposed scatter pulses in the bottom panel. These represent zero scatter pulses associated with green photomultiplier noise exceeding the triggering threshold when this detector was triggering the system and there were no cells in the sensing volume. The two-dimensional frequency contour plots of 90° scatter versus green 'fluorescence', with their associated histograms adjacent to the respective axes, corresponding to the traces of figure 9.1 are shown in the top and bottom panels of figure 9.2. In the top panel we have the expected 90° scatter histogram from cells and its associated background histogram on the green channel. In the bottom panel, where we were triggering on the green detector (mainly noise), there was a major proportion of 'events' on the 90° scatter channel which were being scored as zero or close to zero. These correspond to the 'base-line' event traces under the scatter pusles in the lower panel of figure 9.1. The shape of the green 'fluorescence' histogram is exponential in form in the lower panel of figure 9.2 which is characteristic of photomultiplier noise. Also, there was a greater proportion of smaller events on the green channel in the lower panel compared with the upper panel in figure 9.2. In the upper panel only green signals associated with real events, i.e. cells, were being recorded due to the triggering on the scatter channel
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INSTRUMENT PERFORMANCE
Figure 9.1. Oscilloscope traces illustrating photomultiplier noise. The bottom traces in each panel are from the 90° scatter detector and the top traces are from the green fluorescence photomultiplier. The system was triggered by the scatter detector in the top panel and by the green fluorescence detector in the bottom panel. Note the zero scatter pulses under the lower trace in the bottom panel. and these were associated with scatter and autofluorescence from cells. In the bottom panel, where the green detector was being used as the trigger, we were scoring a greater proportion of random noise events. This resulted in a greater proportion of smaller events being recorded and these are predominantly associated with zero 90° scatter signals. Photomultiplier noise is very easy to diagnose if you have an oscilloscope to monitor the voltage output from the detectors. However, if you haven't and you are worried that you might be running into this problem you should collect two data sets triggering first on the scatter channel and then on fluorescence. If you obtain patterns corresponding to those in figure 9.2 you know that you have a
NOISE
153
Green
Green
Figure 9.2. The contour plots of 90°scatter versus 'fluorescence', with associated histograms adjacent to the respective axes, corresponding to the traces of figure 9.1. The top panel shows the expected 90° scatter histogram from cells and the associated background noise histogram on the green channel. In the bottom panel, where we were triggering on the green detector (mainly noise), there is a considerable proportion of 'events' on the 90° scatter channel which is being scored as zero or close to zero. These correspond to the 'base-line' event traces under the scatter pulses in the lower panel of figure 9.1. potential photomultiplier noise problem and its high tension voltage supply may be turned up too high. Electronic noise can also arise from the most unlikely sources on occasions. Our system uses crossed cylindrical lens pair focussing to give partial slit-scan excitation and the electronics digitize pulse height, width and area. When we were commissioning the system over a decade ago we occasionally obtained pulses which had height but no width or area. This was somewhat puzzling until it was
154
INSTRUMENT PERFORMANCE
noted that this was intermittent and only occurred in the evening between 5 p.m. and 8 p.m. on Tuesdays and Thursdays. Clearly, there had to be some systematic causation and it then didn't take very long to trace the problem to electrical interference from a floor scrubbing machine with faulty suppression. It is also pertinent to add that some publications (not referenced) have claimed to obtain a discrimination between positive and negative fluorescent cells within the first decade of a 4-decade log amplifier using non-laser illumination. I do not believe this is possible as the instrument is being asked to discriminate between positive and negative in an amplified signal range of a few tens to a few hundreds of micro volts. No regular electronic circuitry can hope to make these distinctions as the electronic noise will also be within this range (see section 4.2.2).
9.1.2
Mechanical
Mechanical vibration arising from any source will give rise to a degree of degradation in the data and an increase in the coefficient of variation. As long as this is not gross it constitutes little or no problem for analytical work where the coefficient of variation within the biology is relatively high. Examples of the latter include surface immunofluorescence and enzyme kinetic studies. However, for assays requiring the highest resolution (which is discussed in section 9.6) where coefficients of the variation within the 1% to 2% range are needed, e.g. flow chromosome analysis, then any mechanical vibration is too much. The most likely sources are very slightly loose mountings for beam steering mirrors or prisms, focussing lenses and particularly of the flow chamber or its components. The optical benches of most instruments these days are vibration isolated. However, vibration can be transmitted to the laser plasma tube in the cooling water supply. This usually arises in the pump in the secondary cooling circuit and if you are about to purchase an instrument you should obtain written confirmation from the supplier that the cooling system recommended has been tested and that it is vibration noise free. Building vibration can also be a problem for high resolution work on occasions and these instruments should not be mounted on a wooden floor, but on concrete. If you have a choice it is better to have the instrument as near to the foundations of the building as possible, but if you are half way up a tower block then site the instrument as close to a load bearing structure as possible. This can be a very real problem. Our instrument was initially sited in the middle of a laboratory on the fourth floor of the building and on windy days the building vibration was simply too great for chromosome analysis. Having moved down in the world to the third floor and sited our instruments in two adjacent laboratories next to the load bearing wall we have had no problems.
9.1.3
Fluidic
Junk in any sample or sheath fluid feed lines or in the sheath reservoir are common causes of noise and are usually picked upon on scatter detectors particularly those at 90° if UV excitation is being used. Some micro-organisms can
NOISE
155
grow in distilled water or phosphate-buffered saline and these have been known to cause contamination. Sheath fluid should always be filtered through a 0.22 |lm millipore filter even if it is supposed to be distilled water from the building supply. Pressure and flow rate control regulators can sometimes give rise to noise due to oscillations from the pressure control diaphragm. This is often due to contamination of the compressed air supply with sealing oil used in the compressor which tends to block up the jets within the regulator. All compressed air lines should contain an in-line filter and this should be checked every month or so and cleaned when necessary.
9.1.4
Stray light
The probability of any unwanted photons entering a photomultiplier must be reduced to an absolute minimum as any stray light will raise the base-line d.c. current of the detector. Photomultipliers have a finite output range and their response is not linear over the whole of the range (see section 9.7.2). If the d.c. base-line current is high the range of the device will be restricted. This is depicted diagramatically in figure 9.3. In the left panel the d.c. base-line occupies about 10% of the potential output range but in the right panel this occupies 40% of the range and would be due to a relatively high background light intensity. Clearly, this is highly undesirable and should be avoided as far as possible. Unwanted light from the ambient lighting of the laboratory can enter the detectors, and if the instrument has a 'lid' over the analysis point then use it. Ideally, the analysis point from which fluorescence is emitted should be completely enclosed. This is not always possible particularly if you are looking at, and positioning, the droplet break-off point in cell sorting but under such conditions common sense dictates that the ambient light should be reduced to the minimum.
Available range for signals PMT output range
DC base line current Figure 9.3. Depiction of the effects of background light entering a photodetector. In the left panel the d.c. base-line occupies about 10% of the potential output range but in the right panel, with a high background light intensity, this occupies 40% of the range.
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INSTRUMENT PERFORMANCE
Dirty optics are extremely good at scattering exciting light into the collecting lens and hence raising the base-line d.c. current of a photomultiplier. This is particularly important when the analysis takes place in a cuvette. It must also be remembered that there are four interfaces in the latter. The first is where the exciting beam enters the cuvette. Scattered light from this point should not enter the 90° light collection optics unless the design is awful but a dirty air/cuvette interface will reduce the amount of light getting to the cells and will increase the quantity of light scattered into the forward detector. In extreme conditions, particularly if very high light powers are being used, it is possible to absorb enough light at the dirty air/cuvette interface to generate sufficient local heating to produce cracking in the cuvette material. The second interface to be considered is inside the cuvette at the cuvette/capillary junction from which scattered light from any material stuck to the walls of the capillary bore can enter the light collection optics. The inside of the cuvette is just as, if not more, important than the outside but it is not as easy to see if the internal interface is dirty. If you have any doubt take the chamber out and look at the capillary bore with a long focal length phase contrast microscope. The last two interfaces are the internal and external interfaces at right angles to the laser beam in the light path to the collection optics. Any dirty surfaces here will decrease the fluorescent light transmission to the collecting lens. Moreover, as we are dealing with fluorescent material for the majority of the time it is possible to get inappropriate fluorescence signals from material stuck to the capillary walls that is left over from a previous assay. Cuvette material tends to be non-fluorescent quartz but on occasions you will get a chamber in which there are impurities or colour centers. These not only scatter light very efficiently but also generate local heating which will eventually produce cracking. If the latter occurs close to the capillary with extension to the capillary bore then the crack can fill up with the various fluorescent dyes that are being used. This is usually difficult to see under 488 nm excitation but with UV it is very obvious. Also, it should be remembered that some optical filters contain fluorescent material which can give rise to optical noise.
9.1.5
Light sources
Lasers are generally very stable and will usually emit light to within + 0.5%. However, as the tube gets older it will require longer to warm up and reach a steady output. They can also be operated in either current or light stabilized modes. The latter should be used in flow cytometry as the light output is kept constant with the current being varied automatically to keep the output constant. The light output from high pressure mercury arc sources can vary considerably especially towards the end of the arc life time which is about 200 hours. Instruments using mercury arcs should contain a base-line correcting circuit controlled by a feed-back loop from part of the light from the source.
NOISE
9.1.6
157
Preparative
The cell preparation and/or staining procedure can produce obscuring noise under some conditions. This may arise in 'weak7 immunofluorescence staining where dead cells non-specifically trap a greater quantity of fluorochromeconjugated second antibody than the truly positive cells express on the cell surface. Combinations of light scatter signals can help in this problem which is discussed fully in section 10.3. Noise can arise from the carrier fluid surrounding the cells. This is also particularly likely to occur in cell surface immunofluorescence work where there are relatively few molecules of interest on the external membrane and the washing steps have been inadequate. A schematic of this is shown in figure 9.4, which depicts a cell in the core within the illuminated sensing volume. The dots represent the fluorochrome molecules and there is a greater concentration of these in the carrier fluid than in the volume occupied by the cell although there are fluorochromes associated with the cell membrane. If the instrument is being triggered by the scatter detector (which it should be) then all fluorochrome molecules in the core surrounding the cell as well as those on the cell surface will be 'seen7 by the fluorescence detector. In this scenario the cell is effectively 'displacing' fluorochrome molecules from the volume which is seen by the instrument and you will not be able to detect the specific binding within the high non-specific background. This is directly analogous with an attempt at astronomical observations of stars with a telescope during the day.
Hydrodynamic core-
Instrument will "see" all fluophore molecules in this volume
Cell with surface immunofluorescence
Figure 9.4. Depiction of cell surface fluorescence where there is a greater concentration of fluorochromes (represented by the dots) in the carrier fluid than in the total volume occupied by the cell which is, therefore, displacing fluorochrome molecules.
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INSTRUMENT PERFORMANCE
9.1.7
Biological
The two main sources of biological noise arise from auto-fluorescence and light scatter. Many biological molecules can fluoresce, in particular tyrosine and NADH, and on occasions these can give rise to significant 'intrinsic' noise. Also, cells fixed with gluteraldehyde emit considerable fluorescence and this fixative should be avoided. Highly granular cells or those with multi-lobed nuclei, e.g. polymorphonuclear leukocytes, eosinophils and basophils, always scatter considerable quantities of light to 90° and heavier filtration of excitation light may be needed for assays involving such cells.
9.2
Calibration
Calibration is about finding out how many molecules correspond to each digitization step from the A to D converters and two methods have been applied in flow cytometry. The first used a ligand double labelled with fluorescein and 125I so that radioimmunoassay results can be compared directly with those from flow cytometry. Hulett et al. (1973) used the binding of double-labelled concanavalin A, and Loken and Herzenberg (1975) used a similar method by double labelling a Fab (R oc M Fab) fragment. Titus d al (1981) quantitated the average number of Fc receptors per cell using radiolabelled rabbit IgG dimers. Cells were then counter-
o
y
200-
Rad ioactiv
cpm:
T-
/'
100-
O-i
y
r
'
I
200
'
l
400
'
600
Mean fluorescence
Figure 9.5. Calibration curve obtained with a double labelled antibody comparing radioimmuno assay results with those from flow cytometry where the above background values for both the 125I counts and mean fluorescence are plotted respectively on the ordinate and abscissa. The regression line has a slope of 42.4 cpm per fluorescence channel with a correlation coefficient of 0.99.
MEASUREMENT RANGE
159
labelled with fluorescenated anti-rabbit antibody and sorted on their different fluorescence intensities. The latter were correlated with radioactivity counts to give a calibration curve. The second approach is to use Sephadex beads conjugated with known quantities of fluorescein (Visser, Haaijman and Trask, 1978) to give a non-biological absolute standard. Le Bouteiller et al. (1983) have used this method but they did not attain linearity of instrument response until there were over about 400 000 fluorescein molecules per microbead. Our group has used the first method where the E l l murine monoclonal antihuman complement receptor type 1 (CRJ antibody (IgG-k; Hogg et al, 1984; Walport et al, 1985) was double labelled with 125I and fluorescein isothiocyanate (Watson and Walport, 1986). Normal human granulocytes were labelled with the same overall concentration of antibody where the labelled: unlabelled ratio was varied. Figure 9.5 shows the calibration curve which compares the radioimmuno assay results with those from flow cytometry where the above background values for both the 125I counts and mean fluorescence are plotted respectively on the ordinate and abscissa. The regression line has a slope of 42.4 cpm per fluorescence channel with a correlation coefficient of 0.99. The mean number of anti-CR-! molecules bound per neutrophil was calculated to be 25 000 from the known 125I specific-activity and the counts per minute. A count rate of 24 000 cpm (undiluted labelled antibody) from the radioimmune assay was equivalent to 25 000 CRj molecules. Thus, each fluorescence channel was equivalent to 44 CR! molecules with a linear response.
9.3
Measurement range
In the early days of commercial flow cytometers, which is only 15 years ago, most instruments had a dynamic range of 2 8, i.e. 0—255. If the assay you wanted to perform could be encompaced within this range all was well. This was then perfectly adequate for most DNA histogram work where the maximum range required was a factor of 2. The Gl peak could be set at channel 100 and the G2 + M peak would then be recorded in channel 200. It was also perfectly adequate for simple immunological studies which were designed to determine the proportion of cells labelled with a specific probe to a cell surface determinant. It didn't matter if large proportions of the population were scored 'off the end' of the range, as long as they were recorded, as it was still possible to determine the labelled fraction. However, this limited range was not adequate for assays in which multiple subsets within a heterogeneous sample needed to be quantitated simultaneously, be this for surface immunofluorescence work or for measurement of dynamic cellular processes where the range required might span a number of orders of magnitude. 9.3.1
Log amplifiers Log amplifiers (see section 4.2.2) were introduced to overcome this problem and an example is shown in figure 9.6. This shows a bivariate distribution of lymphocytes double labelled with 0C-CD4 and 0C-CD8 antibodies respectively
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INSTRUMENT PERFORMANCE
CD8—•
Figure 9.6. Bivariate distribution of lymphocytes double labelled with 0C-CD4 and 0C-CD8 antibodies respectively tagged with fluorescein and phycoerythrin using logarithmic amplification. tagged with fluorescein and phycoerythrin. The results shown in figure 9.6 required a dynamic range of three orders of magnitude which is close to the maximum that can be attained with log amplification for the reasons given in section 4.2.2. In order to increase the dynamic range still further we have to use the methods described in the next two sections.
9.3.2
Neutral density filters
The dynamic range was increased to five orders of magnitude by Hecht et al (1981) with a combination of log amplification and neutral density filters to study the DNA content of uni- and multi-cellular systems. Neutral density filters attenuate the quantity of light entering the photodetector by a defined quantity (see section 3.5.2). Thus, the sample containing cells with the largest signals is run first with a neutral density filter in the light path to the detector. When the required number of events has been recorded the filter is removed and the cells with the smallest signals are recorded. This technique can use a number of different neutral density filters (see next section) and it requires that two (or more) different data files be collected. Thus, cells with the largest and smallest signals are not recorded within the same data file, but the light scale' differences between the files are defined by the filter attenuation which allows direct comparisons to be made.
9.3.3
Variable gain
With log amplifiers the data are 'compressed7 in the upper region and, 'expanded' in the lower region of the range (see section 4.2.2). Hence, there is some
MEASUREMENT RANGE
161
loss of resolution of the larger signals which is proportional to signal magnitude. There are many instances where a large dynamic range, without loss of resolution, is required. This can be achieved by designing the pre-amplifier so that the gain, within a specific range, can be varied by defined quantities. This technique is directly analogous to the volume control of a radio and can be used with either log or linear amplifiers in combination with neutral density filters. The combination of variable gain with linear amplifiers and neutral density filters has been used on our instrument to obtain a dynamic range equivalent to seven log-orders (Cox, Munn and Watson, 1987). Three neutral density filters with optical densities of 0.5, 1.0 and 2.0 (Melles Griot Ltd. Arnhem, Holland) were placed in holders which were constructed so that any two filters could be placed in the light path to the PMT without exposing the latter whilst the high tension voltage was switched on. Figure 9.7 shows the section of the instrument with the green and red PMT mounting block, their band pass filter holders (515—560 nm and > 630 nm respectively) and two holders for each PMT which contain the neutral density filters. The push rods for the latter enable the filters to be inserted or withdrawn from the light paths. Figure 9.8 shows a typical calibration run where the OD 0.5 and 1.0 filters were used separately. Initially, the OD 1.0 filter was placed in the light path to the PMT, the pre-amplified gain was set to the maximum of 140 and the PMT high tension
Figure 9.7. The green and red PMT mounting block with their band-pass filter holders (515-560 nm and > 630 nm respectively) and two holders for each PMT containing neutral density filters which can be placed in the light paths to the PMTs with the push rods.
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162
1344 at gain 140 900
OD 0.5
OD 1.0
0
20
40
60
80
100 120 140
PRE-AMPLIFIER GAIN
Figure 9.8. Calibration run using the OD 0.5 and 1.0 filters separately with varying pre-amplified gain.
voltage was adjusted to record the median of the fluorescence distribution from the microbeads in channel 120. The pre-amplifier gain was then progressively decreased in increments of five units and the medians of the fluorescence distributions were plotted against gain. The two other similar calibrations shown in figure 9.8 were carried out in the same experiment with the same PMT voltage settings for OD attenuations of 0.5 and zero. The slopes of the regressions were 9.6, 3.28 and 0.89 for OD attenuations of zero, 0.5 and 1.0 respectively. In all three there was a linear relationship between fluorescence and gain, and in no case was the regression coefficient less than 0.996 or the Y-axis intercept significantly different from zero. The dynamic range of the instrument can now be calculated for the setup from which the data shown in figure 9.8 were obtained. Theoretically, the calibration for zero attentuation will extrapolate to 1344 at a gain of 140 and the ratio of the slopes for the attenuation of zero to OD 1.0 is 10.8. Hence, the dynamic range is about 14 500 for this particular setup. Taking the data at a gain of 70 (mid gain range) in figure 9.8 as a practical illustration we can see that had the microbeads been a factor of 10.8 brighter they would have been recorded in channel 675 with
MEASUREMENT RANGE
163
the OD 1.0 filter in place. Hence, their true fluorescence could be calculated to be
675X10.8 = 7290. A further example is shown in figure 9.9 where the OD 0.5 and 1.0 were used in combination to give a maximum attenuation OD of 1.5. Both filters were used in the setup, the gain was set to 140 and the PMT voltage was increased to record the median of the fluorescence distribution in channel 130. As in figure 9.8 the gain was then varied for OD combinations of 1.5, 1.0, 0.5 and zero. Again, all the regressions were linear with correlation coefficients not less than 0.998 and the Y-axis intercepts did not differ significantly from zero. The regression slope for zero attenuation versus gain was 21.5, which extrapolates to 3010 at a gain of 140, and the slope ratio for the attenuation of zero to OD 1.5 was 23.1, which gives a dynamic range of 69 500. A number of similar runs were carried out with various combinations of the neutral density filters including 1.0 + 2.0. With this OD combination of 3.0 the high tension voltage on the PMT was increased to record the fluorescence distribution in channel 60 with a gain of 140. The gain was then reset to 3, the filters were removed and the fluorescence distribution was recorded in channel 726. Only two more points, at gains of 2 and 4, could be obtained in the absence of
i 3 0 1 0 at gain 140 900
/ OD 0.0
OD 0.5
OD1.0
OD 1.5 (0.5+1.0)
20
40
60
80
100 120 140
PRE-AMPLIFIER GAIN
Figure 9.9. Similar calibration run to that shown in figure 9.8 but where the OD 0.5 and 1.0 were used in combination to give a maximum attenuation OD of 1.5.
INSTRUMENT PERFORMANCE
164
filtration at this PMT voltage but six were obtained with the filters in place before the pulse size dropped below the triggering threshold. This was the maximum OD difference that could be attained at a given PMT voltage and the slopes of the respective regressions were 245 and 0.431 giving a slope ratio of 56S. The slope of 245 extrapolates to 34 300 at a gain of 140, hence, the maximum dynamic range of the instrument at a given PMT voltage is 1.94 x 107. From figures 9.8 and 9.9 we can calculate the ratio of the slopes for various combinations of optical density difference. There is one ratio in figure 9.9 for an OD difference of 1.5 (0.0 with 1.5), two ratios for a difference of 1.0 (0.0 with 1.0, and 0.5 with 1.5) and three ratios for an OD difference of 0.5. As the optical density scale is logarithmic we should obtain a linear relationship by plotting the OD difference against log e of the slope ratios for these OD differences. This is shown in figure 9.10 for all the combinations of slope ratios from a number of experiments and regression analysis gave a slope of 0.463 with a correlation coefficient of 0.994. As the abscissa scale is in natural logarithms and the OD scale is in log 10 the expected slope (dashed line) is Iog10(e) = 0.4343. Although the difference between observed and expected appears to be small (0.463 compared with 0.4343) this was significant at p < 0.05. For a given optical density (Y-axis) the log e of the slope ratio was 6.6% less than the theoretical value and two factors have contributed to this discrepancy. Firstly, the OD filters were calibrated individually at 550 nm by the manufacturer and our system uses a 515—560 nm band-pass filter. Although the optical densities are not very different at lower wavelengths there were some deviations from the nominal value particularly for the higher ODs, but this would not account for all of the observed difference. Secondly, there was an air gap between all filters and a thin Perspex guard over the coated surface of the OD 2.0 filter which is normally used to ^ o
3.0
UJ
O
2.0
Calculated result slope 0.463 correlation coefficient 0.994
UJ
cc S! u.
5 o
1-5
to
Expected result slope 0.434
o 0.5 0
1.0
2.0
3.0
4.0
5.0
LOG OF SLOPE RATIOS
Difference significant at p<0.05 6.0
7.0
(log e )
Figure 9.10. Slope ratios for all combinations of OD differences gave a regression slope of 0.463 and correlation coefficient of 0.994.
COEFFICIENT OF VARIATION
165
attenuate the forward scatter signal in our instrument. This particular filter was used to obtain the results for OD differences of 2.0, 2.5 and 3.0. Hence, additional light losses of about 1.5% at each interface would account for the discrepancy shown in figure 9.10. However, these factors are of no importance once the calibration has been carried out under operating conditions, and we have found this simple technique to be a very useful addition to our instrument.
9.4
Coefficient of variation
The coefficient of variation (CV) is defined as the ratio of the standard deviation of a distribution to the mean. Thus, the CV is the relative standard deviation of the distribution and it is frequently used as an overall indicator of the performance of flow cytometers but few seem to question exactly what the measurement represents. Every histogram generated by flow cytometry contains a number of sources of variation. These include variation due to the biology (including staining variability), the background excitation light entering the fluorescence detector and the inherent variation in the instrument due, amongst many other things, to noise. When combined these factors give rise to a distributed response from the population being studied. We have also seen (section 4.3) that the analogue-to-digital conversion (ADC) step in the electronics gives rise to an artefactual positive skew in all distributions. If we want to know what the true distribution of molecules per cell is within the
0.2>
\!
o
- 8 - 8 - 8 — Q-o-e-©
8
0.1 -
0 O
o
200
400
600
800
Mean channel of distribution from fluorescence detector
Figure 9.11. Coefficients of variation plotted against the means of the associated distributions. Experimentally determined data are shown by the closed circles and the predicted values are shown by the open circles. The triangles show similar determinations obtained with microbeads.
166
INSTRUMENT PERFORMANCE
population we have to take into account all these sources of variation. As an example I will take the CR1 data cited in section 9.2. The variance of the distribution (calculated from the mean and CV) at each 'hot' antibody concentration was obtained from the skew-histogram analysis (section 5.4.4). This is equal to the sum of the variances due to the background, biological and instrument variation. The CV of the background was calculated to be 21% from analysis of the zero point (cells stained with non-labelled antibody) and the CV of the instrument was taken to be 3% at maximum from analysis of fluorescent microbeads (see figure 9.11). Hence, the only unknown is the biological variance which must be constant in these experiments as the same cells were used throughout. Thus, we can calculate the biological variance and hence CV which was 19.1%. The measured CVs (closed circles) are shown in figure 9.11 plotted against the means of their associated distributions. Also shown are the predicted values (open circles) calculated from the measured CVs of the instrument and background plus the calculated CV of 19.1% for the biological variation. The agreement is good. This value of 19.1% for the biological CV is equivalent to a standard deviation of 4775 CR-! molecules for cells within the population.
9.5
Sensitivity
The sensitivity of an instrument determines the point above which it is possible to perform an assay. A number of factors including noise, exposure time, excitation light flux, bleaching, light collection efficiency, optical filtration and fluorochrome amplification all contribute to sensitivity. Noise was discussed in detail in section 9.1 and will not be considered here. 9.5.1
Exposure time Fluorescence is emitted in nanosecond time following excitation (section 3.8). This is a random process, governed by exponential decay and we will assume that the average fluorescence life time is 10 ns (this is not the same as the fluorescence half-time but is related to the half-time by the factor 0.6931 which is log e 2). If an instrument has a 'high' flow rate of 1 0 m s " 1 each cell of 10 |lm in diameter will be contained within the beam for 1.0 |ls. Thus, each fluorochrome molecule has the average potential for 100 excitations and fluorescence emissions. With a low' flow rate instrument of say 2 m s " 1 this obviously raises the potential for 500 excitations and emissions. If, therefore, we are attempting to measure very low fluorescence intensities we should use a flow rate which is as low as possible but still compatible with flow stability for that particular instrument.
9.5.2
Excitation intensity
Light flux at the excitation point was considered in section 3.9. In general a higher light flux will give a greater probability of exciting all available fluorochrome molecules as these pass through the focus. However, there is no point in increasing the light flux beyond the point at which there is a gross excess
SENSITIVITY
167
of photons compared with the number of fluorochrome molecules to be excited. This can give rise to bleaching (see next section) and an increase in the scattered light which has to be filtered out (see section 9.5.5). 9.5.3
Bleaching Bleaching was considered briefly in section 3.8.4 and occurs when a second photon is absorbed by the fluorochrome before it has discharged the excess energy from a first photon. This can give rise to a number of molecular changes ranging from minor electron configuration disturbances to total disruption of the molecule. The higher the light flux the greater is the chance of bleaching and this is a more important consideration in low' flow rate compared with 'high' flow rate instruments. If the light flux is 'too high' in a low flow rate instrument the advantage of the large number of excitations per fluorochrome will be lost due to the increased chance of bleaching. 9.5.4
Light collection efficiency Light collection efficiency was considered in detail in sections 3.6 and 3.7 and, clearly, collecting greater quantities of light would seem to be universally desirable. However, as with exposure time and excitation intensity there are two sides to the coin. Collecting more light necessarily means that more scattered and background light as well as fluorescence will be collected and in order to obtain an increased signal-to-noise ratio the extra scattered light has to be eliminated completely (which is usually not possible) or reduced to a minimum. If the light collection efficiency of a system is increased by a factor of three we have to reduce the probability of background light entering the fluorescence detector by this same factor to obtain a threefold increase in the signal-to-noise ratio. 9.5.5
Optical filtration The performance of any filter system depends on some form of probability function and there is always some chance that an exciting photon will enter the fluorescence detector and be scored erroneously as fluorescence. This phenomenon is frequently used in setting up an instrument with non-fluorescent control cells by increasing the photomultiplier (PMT) high tension voltage until the exciting light from each cell 'breaks-through' the filter system and can be seen by the fluorescence detector. The sample containing labelled cells is then run and the two data sets are compared. Modern photomultipliers and electronics are capable of amplifying a signal by many orders of magnitude and this has important consequences for the measurement of very low levels of fluorescence and determination of sensitivity and detection limits. This applies particularly when the excitation light is close to the lower wavelength limit above which fluorescence is measured and where the latter is less intense than the excitation light scattered towards the fluorescence detector. Hence, a major component which is scored as fluorescence could in fact be scattered light. Perhaps the best example is fluorescein excited with the blue
168
INSTRUMENT PERFORMANCE
Table 9.1. Probability of photonentry Green detector
50:50 splitter 510 dichroic
90° scatter detector
blue light
green light
blue light
green light
5 X 10 " 6 10 " 6
0.45 0.72
0.45 0.81
5xlO"4 2X 10~4
488 nm line from an argon laser where green fluorescence is measured above about 515 nm. The problem tends to be compounded by the compulsion to increase the laser power for the detection of low intensity fluorescence as the yield of the latter tends to saturate due to bleaching but the quantity of scattered light continues to increase linearly. Consider two optical filtration systems containing a 50: 50 beam splitter and a dichroic mirror respectively. Both of these types of optical filtration system have been used in commercial instruments. Let us assume that we are exciting fluorescence with the 488 nm argon line (subsequently referred to as blue) and analysing light, some of which will be fluorescent, above 515 nm (subsequently referred to as green). A 515 nm long-pass filter (LP 515) guards the green 'fluorescence' detector which has a blue transmission probability of 10 ~5 and a green transmission probability of 0.9 above about 525 nm. The blue 90° scatter detector is guarded by a 500 nm short-pass filter (SP 500) which has blue and green transmission probabilities of 0.9 and 10~ 3 respectively. When the 50:50 beam splitter is in place there is a 0.5 probability of both blue and green light being transmitted and reflected but, if this is replaced by the 510 nm dichroic mirror (DC 510) there are transmission probabilities of 0.1 for blue and 0.S for green with reflection probabilities of 0.9 and 0.2 respectively. A summary of the overall probabilities of green and blue photons entering the two detectors is shown in table 9.1 for both filter systems. We can now see that the probability of the green detector seeing a green photon using the dichroic mirror is 7.2 X 105 greater than its chance of seeing a blue photon. However, with the 50:50 beam splitter this is reduced to only 9 x 104. Thus, the system containing the dichroic mirror is 800% more efficient in discriminating between blue and green compared with the system containing the 50:50 beam splitter. Most, if not all, modern instruments contain dichroic mirrors and not 50:50 beam splitters. However, many of the older instruments containing the latter are still around and functioning, but obviously, their sensitivities are limited. In very high light collection efficiency instruments a second 510 dichroic mirror can be introduced into the filter system which gives probabilities of 10 ~7 and 0.5 7 respectively for blue and green photons entering the fluorescence detector. This gives a 5.7 x 106 greater chance of seeing a green photon in the green detector than of seeing a blue photon; a further gain factor of just under 800%.
SENSITIVITY
169
9.5.6
Fluorochrome amplification A number of techniques are available for tagging each molecule of interest with a number of fluorochrome molecules (section 733). These include two or three layer immunofluorescence methods where a number of fluorochromes are attached to the second antibody with a number of these being bound to the single antibody probing the target molecule. The biotin-strapavidin technique is also being used quite extensively and fluorochrome-tagged liposomes can achieve a 100-fold amplification (Truneh and Machy, 1987). These methods were discussed in section 733. 9.5.7
Sensitivity measurement Exposure time, excitation light intensity and light collection efficiency are all two edged swords and must be balanced one against the other to obtain optimum results. A number of groups have defined the detection limits of their systems and hence the sensitivity. Loken and Herzenberg (1975) obtained a detection limit between 3000 and 5000 molecules with double-labelled Fab (R a M Fab), a similar value to that of Hulett et al. (1973), Visser et al. (1978) and Le Bouteiller et al. (1983) using fluorescein-conjugated Sephadex beads and obtained detection limits between 2500 and 3500 molecules. Referring back to figure 9.5 we can see that the regression line cuts the abscissa at 16.6 channels which is significantly different from zero (P> 0.05) and from this we calculated the detection limit in our system to be 730 CR! molecules per cell with a resolution of 44 molecules per channel (see section 9.2). Furthermore, the response was linear over the range of 700—25 000 molecules in contrast to the results reported by Le Bouteiller et al. (1983) where linearity was only achieved above about 400 000 fluorescein molecules per microbead. Fluorescence from FITC bound to protein is 80% quenched compared with free fluorescein in aqueous solution (Tengerdy, 1965) and each antibody molecule in the results shown in figure 9.5 was labelled with 0.9 FITC molecules on average. Hence, in terms of the fluorescence from free fluorescein in solution, the detection limit of the instrument was about 130 molecules per cell with a resolution thereafter equivalent to less than 10 molecules per channel. A detection limit of 22 000 molecules of rhodamine-6G in aqueous solution has been achieved and the possibility of single molecule detection has been considered using laser induced fluorescence (Dovichi et al., 1983, 1984). These studies were also conducted with a flow cytometer but the measurement system was very different from the regular type of instrument. Dovichi et al. (1983, 1984) were integrating over a one second interval from fluorochrome in solution and the dilution was such that there was less than one dye molecule in the sensing volume at any instant. In our studies there was, on average, less than one fluorescein per antibody molecule and the detection limit equivalent to 130 free fluorescein molecules per cell was achieved with each cell traversing the sensing volume in 5 |is. Thus, in our studies the light flux was very much greater when a cell was being illuminated than in the system used by Dovichi et al. (1983,
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INSTRUMENT PERFORMANCE
1984). Hence, any comparison of the relative sensitivities of the two instruments is not strictly valid. Our instrument has already been used to quantitate CRX density in the range of 100—1200 molecules per cell in erythrocytes using an amplified technique with a polyclonal antiserum (Walport et al, 1985). Even without any further improvements in the instrument we should be able to achieve a detection limit of a few tens of receptor molecules per cell using fluorochrome amplification with biotin— streptavidin.
9.6
Resolution and discrimination
The term resolution can have slightly different meanings in different contexts. In the previous section this expression was used as a means of specifying the minimum number of molecules equivalent to each fluorescence channel, or digitization step, of a near continuous distribution. The more common usage in flow cytometry is analogous to its meaning in microscopy where it describes the minimum distance between two lines that can be seen to be two. Due to diffraction effects the maximum resolving power of a good microscope objective is about 0.5 |lm, which means that if two lines are less than this distance apart they will be seen as one. In flow cytometry resolution is frequently used to describe the ability of the instrument to distinguish between closely spaced peaks on a histogram, particularly in chromosome analysis. As all population measurements in flow cytometry have a dispersion (see section 9.4) the ability to distinguish between closely spaced peaks depends critically on the coefficient of variation and, clearly, the smaller the coefficient of variation the greater will be the resolving capacity. This relationship is demonstrated in figure 9.12 where Student's-T is plotted on the ordinate versus the channel number of the mean of two distributions which both have the same CV and where one was fixed in channel 100. You can find out all about Student's-T in Fads from Figures by M. J. Moroney (1951) and, if you have got this far you really should buy that book as well. The CV was varied between 1% and 4% and each distribution was generated with 5000 cells and the two distributions were summed. The figure is divided into three regions by the stippled area above which the combined distribution could be seen to have two distinct peaks. With a CV of 1% the means of the two distributions had to be separated by 23 channels in order to be able to see two definite peaks. However, with a CV of 4% the separation had to be 8.5 channels. Within the stippled area it was obvious that the combined distribution had a shoulder but below this the combined distribution looked essentially symmetrical. This type of diagram can be generated for various proportions of the whole population contained within the two individual distributions and these can be a useful guide to the CVs that are required to resolve closely spaced peaks. Resolution is sometimes confused with sensitivity. It is quite possible to have a very sensitive instrument which is deficient in resolving capacity particularly for 'weak7 signals. The converse is also true; a less sensitive instrument can have good
RESOLUTION AND DISCRIMINATION 160
3%
2%
1%
171
1%
2%
3%
140 4%
•o
4%
120
CO
100
80 90
95
100
10000 cells
105
1 10
50:50
Figure 9.12. Resolving capacity between two closely spaced Gaussian distributions. Student's-T' is plotted on the ordinate versus the channel number of the mean of two distributions which both have the same CV and where one distribution was fixed in channel 100.
resolving capacity for weak signals. The best example is weak immunofluorescence with a relatively wide CV where there is a mixture of labelled and unlabelled cells. A sensitive instrument with linear amplification will have poorer resolving capacity than a less sensitive instrument with log amplifiers (section 4.2.2). This is illustrated in figure 9.13 which is a magnified version of figure 4.1 where the X-axis has been 'expanded' to show the responses of both log and linear amplifiers on the same graph over the range zero to 0.5. Incidentally, log amplifiers do not have a log response over the whole of their range. They tend to linearity in the very initial phase as shown by the dashed line in figure 9.13. In this example there are inputs of 0.05 and 0.1 on the abscissa. With the linear amplifier these inputs translate to outputs of 10 and 20, a difference of 10. The same inputs to the log amplifier give outputs of 2>2>2> and 433, a difference of 100. Thus the log amplifier has a 10-fold greater resolving capacity than the linear amplifier over this range as the slope of the log amplifier response curve is greater by a factor of 10 than that of the linear amplifier. However, if we move to the right and consider inputs of 0.45 and 0.5 the resolving capacity of both amplifiers is about equal as the response slopes are approximately equal. With inputs greater than about 0.5 the resolving capacity of the linear amplifier is greater than that of the log as the slope of the response curve of the latter is less than that of the former.
172
INSTRUMENT PERFORMANCE 700-1
0.5
Figure 9.13. Magnified view of figure 4.1 showing both log and linear amplification responses on the same diagram.
9.7
Precision
Precision of measurement in any instrument is concerned with the deviation of the answer obtained from the instrument compared with the reality. In flow cytometry if we have a linear amplifier and the G l peak of a DNA histogram is recorded in channel 200 then the G2 + M peak should be recorded in channel 400 as we have an a priori reason for believing that the G2 + M DNA content is double that of Gl. Similarly, if the Gl peak had been recorded in channel 400 the G2 + M peak would be expected to be appear in channel 800. These examples describe a linear response of the instrument where the G2 + M : G l ratio is constant at 2.0 and independent of signal magnitude. However, if we had used log amplifiers the G2 + M : G l ratio would not be constant and for Gl peaks in channels 10, 100 and 200 we should get G2 + M.-G1 ratios of 1.301, 1.150 and 1.131 respectively. Nevertheless, even though the G2 + M.-G1 ratio is not constant with log amplification the instrument is still behaving in a precise and predictable manner if we obtain these values when the Gl peak is placed in those respective channels. A 'non-linear' response, and by that I mean a response which either deviates from linearity with linear amplifiers or from a log response with log amplifiers, is most commonly due to ADC offset or to an attempt to work outside the linear range of detectors or amplifiers. These potential problems are discussed in the next two sections.
PRECISION
9.7.1
173
ADC offset
We saw in section 4.3 that the analogue-to-digital converter can be set up so that the arbitrary 'zero' is not the first digitization channel. It may be that the first digitization channel that can be scored is, for example, 10 or even 100 units. This may seem a little strange until you consider that the whole of the measurement system is essentially arbitrary and depends to a large extent on the amplification and high tension voltage on the photomultiplier. Let us suppose that we have a 10-bit (0-1023) ADC and there is a 50 channel offset to the right which is the most likely artefact of this type to be encountered. The 'true zero' will in fact be — 50 channels. Thus, if the Gl peak of a DNA histogram is recorded in channel 200 the G2 + M peak will appear in channel 450 giving a G2 + M : G l ratio of 2.25. In reality, channel 200 is 250, and 450 is 500 (giving the expected G2 + M: Gl ratio of 2.0) as we should add on the ADC offset of 50 channels to the peak positions of 200 and 450. It is very easy to check if there is such an offset in your instrument by running microbeads at different laser powers where the medians of the distributions are plotted against their respective laser powers. This procedure is identical in principle to that used in figure 9.8 which was a calibration 800-1
600o c 0)
o
(0 0)
o 3
200-
offset
200
400 600 800 1000 Light power, mW
Figure 9.14. ADC offset shown by analysing microbeads at different laser powers. Distribution means are plotted on the ordinated versus light power on the abscissa.
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INSTRUMENT PERFORMANCE
curve of fluorescence versus pre-amplifier gain. Many instruments do not have the capability of defined pre-amplifier gain variation, but everyone can vary the laser power. If there is no ADC offset the regression line of fluorescence intensity versus laser power will extrapolate through the origin just as in figure 9.8. If there is an ADC offset the regression will cut the Y-axis at the value of the offset and this is illustrated in figure 9.14 where the regression line was calculated using the solid symbols. The open symbols show some deviation from linearity which is due to photobleaching at the higher light powers. Having established the value of the offset it is now possible to correct the data accordingly. This is important for DNA histogram work where aneuploidy is being assessed to give estimates of DNA index and confusion has arisen because some users were not aware of this potential offset problem. The offset should not be more than about 20 channels with 10-bit (0—1023) resolution and if it is, you should complain to the supplier.
9.7.2
Non-linear response
Both photomultipliers and linear amplifiers have a finite range over which their response is truly linear. A representation of the general shape of photomultiplier (PMT) response curves are shown in figure 9.15 where voltage output is plotted on the ordinate versus photon input on the abscissa for three different PMT high tension voltages. This figure is not data, it is a cartoon, but it is, at least, reasonably representative. Each curve is characterized by an initial nonlinear response where there is increasing output with photon input followed by a linear response directly proportional to input as indicated above the dashed line. Saturation is reached at the upper end of each curve followed by a decrease in output. The latter condition should never occur as this is indicative of gross
800 volts
600 volts
200 volts
3
a.
Photon Input
Figure 9.15. Representation of the general shape of photomultiplier response curves where voltage output is plotted on the ordinate versus photon input on the abscissa for three different PMT high tension voltages.
PRECISION
175
photon overexposure of an energized phototube, but it can occur if the energized tube is accidentally exposed to ambient light and it's usually not much good thereafter. The linear section of the response is a plane in the three-dimensional space of voltage output, photon input and high tension voltage on the PMT. From figure 9.15 you can see that at any given PMT high tension voltage it is possible for conditions to exist where you are not working within the linear response section. The reason for the two vertical lines, labelled A and B, will become apparent later. A practical example is shown in figure 9.16 where ethidium bromide stained nuclei, with some (useful) clumping, were being analysed for DNA content on two photodetectors simultaneously. Fluorescence was being elicited by the usual 488 nm argon line at a light power of 200 mW and a 580 nm dichroic mirror was used to split the emission spectrum. The 'green7 and 'red7 PMTs were additionally guarded by a 515—560 nm band-pass and a 590 long-pass filter respectively, and the signals from the red detector were scored on the ordinate versus the signals from the green detector on the abscissa. The high tension voltages of the PMTs were adjusted to place the Gl peak at a scale reading of 200 on both channels (the 'green' PMT high tension voltage was very much higher than the 'red') and in the left panel there is clearly non-linearity. The response on the red channel is increasing more rapidly with signal magnitude than on the 'green' channel. This problem was only encountered after we increased the light collection efficiency of our flow chamber (see section 3.73). What was happening here was that we were not on the linear segment of the red photodetector response curve. A very considerable quantity of fluorescence is emitted from ethidium bromide stained nuclei at an excitation power of 200 mW and we had just increased the light collection efficiency by 300% when this particular experiment was performed. Thus, the high tension voltage on the red detector had to be reduced to very low levels to place the Gl peak in channel 200. We were working, therefore, in the region of the vertical line 'A' drawn on figure
A
B
•o
j
Green
Green
Figure 9.16. Illustration of non-linear PMT response obtained from ethidium bromide stained nuclei with a high light collection efficiency flow chamber. Analysis was carried out on two PMTs simultaneously, note the distinct curve in panel A which was corrected in panel B by inserting an OD 1.0 neutral density filter and increasing the red PMT high voltage.
INSTRUMENT PERFORMANCE
178
0)
o> (0
o > I-
o.
T2 T1
9.17. Double threshold electronic threshold triggering system to identify closely spaced pulses. recording is not completed. The difference between the upper and lower panels is that the voltage drops below Tl in the lower before it rises again through T2. In this case a recording is made and the width of the pulse is timed when the voltage drops below Tl and pulse height, width and area are digitized and input to the FIFO buffer (see section 4.4.1). This system is similar to traffic lights controlling vehicle flow at a road junction. If only the amber light is showing you know that red is coming up next and you must stop. If red and amber are showing then green is coming up next and you can prepare to accelerate. With the double threshold system the sequence Tl, T2, T2, T2 means stop, events are too closely spaced. In contrast, the sequence Tl, T2, T2, Tl means go and the data are acquired. The analogue-to-digital conversion step plus dumping the data into the FIFO takes a finite interval of time and the acquisition system is disabled until this is completed. In the lower panel of figure 9.17, which is approximately to scale, there would not be sufficient time in our system to complete these operations quickly enough to be able to start recording the second pulse and this would be lost. There is a third possibility shown in figure 9.18 where the threshold sequence would be Tl, T2, T2, Tl and the data would be recorded although, clearly, this is a double event. However, this can be excluded after acquisition using pulse shape analysis as described in the next section.
QUALITY CONTROL
177
some form of standardization of quality control. The commonest reasons of poor quality data are poor preparation and partial nozzle blockages and the latter is often due to the former. A number of techniques are available to monitor the preparation and hence quality of the data. 9.8.1
Inspection It seems frequently to be forgotten that you can look at your preparation. Just because you have a sophisticated and expensive instrument it doesn't mean you should abandon the fluorescence microscope and newcomers to flow cytometry should always be encouraged to carry out a quick check before presenting the sample for flow analysis. If the preparation looks bad with shredded cells and clumps under the fluorescence microscope it will look much worse in the cytometer. These instruments are very sensitive but they have no inherent intelligence or recognition capability in spite of their apparent complexity. If you are triggering on light scatter and a small chunk of garbage floats through it will always be seen and recorded. In contrast the human eye and mind has the capacity to recognize rubbish and clumps (pity we don't yet know how we do it) and to exclude them automatically. This editorial capacity of the human mind will always lead the observer to believe that the preparation is better than it is. So, if it looks bad under the microscope it really is bad and isn't worth running through the instrument and if you do you will usually plug up the tubes and nozzle.
9.8.2
Coincidence correction
Even if the preparation looks perfect under the microscope there is always a chance that two cells will pass through the focus either very close together or simultaneously. The probability of this occurrence was considered in sections 2.5 and 6.4 and clearly efforts in quality control should take this eventuality into account. Two methods are available, and both use time in slightly different ways. The data acquisition computer can be programmed to calculate the average time interval between arrival of cells at the analysis point from the rate at which the digitized signals are being presented to it for storage. It can then calculate the Poisson probability of coincidence and set the data acquisition logic so that only events spaced at greater than specific intervals are recorded. Thus, if events are arriving 'too close' to each other they are both ignored. The second method uses a double electronic threshold triggering system. Figure 9.17 shows pulses from two closely spaced cells passing through the beam. Threshold 1, Tl, is set lower than threshold 2, T2, and nothing at all will happen unless the voltage from the photodetector exceeds Tl. This 'enables' the electronic acquisition system, which begins to integrate the area under the pulse, starts timing the width of the pulse and records the peak height when this is reached. In the top panel the voltage drops below T2 as the first cell passes out of the beam but does not drop below Tl before rising again to cross T2 as the second cell enters the beam. This aborts the data acquisition logic which is then reset and the
INSTRUMENT PERFORMANCE
178
0)
o> (0
o > I-
o.
T2 T1
9.17. Double threshold electronic threshold triggering system to identify closely spaced pulses. recording is not completed. The difference between the upper and lower panels is that the voltage drops below Tl in the lower before it rises again through T2. In this case a recording is made and the width of the pulse is timed when the voltage drops below Tl and pulse height, width and area are digitized and input to the FIFO buffer (see section 4.4.1). This system is similar to traffic lights controlling vehicle flow at a road junction. If only the amber light is showing you know that red is coming up next and you must stop. If red and amber are showing then green is coming up next and you can prepare to accelerate. With the double threshold system the sequence Tl, T2, T2, T2 means stop, events are too closely spaced. In contrast, the sequence Tl, T2, T2, Tl means go and the data are acquired. The analogue-to-digital conversion step plus dumping the data into the FIFO takes a finite interval of time and the acquisition system is disabled until this is completed. In the lower panel of figure 9.17, which is approximately to scale, there would not be sufficient time in our system to complete these operations quickly enough to be able to start recording the second pulse and this would be lost. There is a third possibility shown in figure 9.18 where the threshold sequence would be Tl, T2, T2, Tl and the data would be recorded although, clearly, this is a double event. However, this can be excluded after acquisition using pulse shape analysis as described in the next section.
QUALITY CONTROL
179
T2 T1 Figure 9.18. Illustration of two closely spaced pulses which would not be recognized by the double threshold system.
9.8.3
Pulse shape analysis
Some types of preparations, e.g. nuclei extracted from paraffin wax embedded archival material, inevitably contain a variable quantity of debris, clumps and nuclear fragments as well as intact single nuclei. After DNA staining with propidium iodide (red fluorescence) any small debris and large clumps can be gated out on a combination of forward and 90° scatter signals. Large fragments of nuclei and small clumps not identifiable in the forward versus 90° light scatter data space can be identified and gated out using the shape of the pulse from the red (DNA) photomultiplier which is usually the master triggering detector in these types of assays. This involves analysis of the pulse height, width and area under each pulse (PAW analysis) where the ratio of width x height/area should be constant to within narrow limits. The method is illustrated in figure 9.19 which shows individual pulses from a single cell (left panel) and a clump of two cells (right panel) which is similar to figure 9.18. The boxes surrounding each panel represent the area obtained by multiplying the height of each pulse by the width, time of flight through the beam. Naturally, this analysis can only be used in partial slit-scan systems using crossed cylindrical lens pair focussing where peak pulse height,
Width
Width
Figure 9.19. Pulse shape analysis of height, width and area under each pulse (PAW analysis) where the ratio of width X height/area should be constant to within narrow limits which can be used to discriminate between fragments and clumps not identified by the double threshold system.
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INSTRUMENT PERFORMANCE
width and area are digitized. We can see by inspecting the two panels that the integrated area under each pulse, which is shaded, occupies a different proportion of the boxes defined by multiplying height by width. As the beam illumination intensity is Gaussian distributed (section 3.9.5) then nuclei which are approximately spherical will give single cell pulse shapes which approximate to a Gaussian profile no matter what the size. Thus, single cell events will give a constant for height x width/area. Doublet clumps (right panel of figure 9.19) and fragments of
Figure 9.20. Practical illustration of pulse shape analysis in a data set obtained from nuclei stained for DNA from an archival carcinoma of colon specimen. Panel A shows the raw data. Panel B shows the same data set after gating on forward and 90° scatter to exclude small debris and large clumps. Pulse shape analysis has been additionally applied in panel C. Panel D shows the final result in which the mean and SD of the diploid peak in panel C were computed and any signals less than 2.5 SDs below the mean were excluded.
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181
nuclei will not give a constant value for this derivative but a spread in values which are unlikely to be the same as the values from intact nuclei. Thus, if the majority of the population (i.e. > 50%) is composed of single nuclei these can be identified and the abnormal pulse shapes excluded. Figure 9.20 illustrates this pulse shape analysis in a data set obtained from nuclei stained for DNA from an archival carcinoma of colon specimen. The product of pulse height x width/area of the red (PI) signal for each cell is plotted on the ordinate against area under the pulse (abscissa). Panel A is the non-gated raw data plotted as a contour map with the mono-dimensional histograms adjacent to the respective axes. Clearly, the derivative (ordinate) is essentially constant but there is a negative skew due to pulses with abnormal shapes. Panel B shows the same data set after gating on forward and 90° scatter to exclude small debris and large clumps. Many of the signals above 600 on the abscissa have now been gated out as have some of those at less than 180. There is also a dip appearing to the immediate
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10 20 30 40 50 Section thickness, microns
Figure 9.21. Indirect relationship between predicted proportion of rubbish (clumps, nuclear fragments and debris) versus histological section thickness.
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INSTRUMENT PERFORMANCE
right of the major spike which is the diploid DNA peak. Pulse shape analysis has been additionally applied in panel C. This was effected by computing the mean and variance (hence standard deviation, SD) of the Y-axis distribution in panel B. Only those pulses falling within +1.5 SDs of the mean of the Y-axis distribution of panel B were included in the display shown in panel C. There is now very clearly a bimodal DNA distribution (abscissa) with the diploid spike at about 200 and an aneuploid component peaking at about 290 which has a much wider distribution. There is still, however, a component being scored at less than about 180 on the abscissa. Panel D shows the final result in which the mean and SD of the diploid peak in panel C were computed and any signals less than 2.5 SDs below the mean were excluded. The original data set in panel A contained 20 000 events; the final data set in panel D contained 6500 events. Thus, only about 33% of the original raw data set was composed of isolated single nuclei which conformed to a specific size and shape distribution. In a number of experiments with various types of samples where the section thickness was varied between 5 and 50 |im the predicted proportion of 'debris' was inversely proportional to section thickness. These data are shown in figure 9.21.
9.8.4
Time
Continuous time recording was introduced as a flow cytometry parameter by Martin and Schwartzendruber (1980) to follow the kinetics of fluorescein diacetate (FDA) hydrolysis in populations of intact cells. Kinetic aspects of flow cytometry will be considered in detail in chapter 14 but time can also be used as a quality control parameter by continuously monitoring versus time an independent parameter which does not vary with time (Watson, 1987). A sample of isolated nuclei stained for DNA with ethidium bromide was introduced into our instrument and the red fluorescence associated with each event was digitized and the time at which each event occurred in relation to the start of each run was also recorded from the computer time clock with 50 ms resolution. A total of 10 000 cells was sampled for each run at a throughput rate of about 200 cells per second and the data were collected list-mode for subsequent display. During some of the runs a number of artificial perturbations were introduced into the system in order to demonstrate the quality control potential of the time parameter. In each figure DNA fluorescence intensity is plotted on the ordinate versus time as a dot-plot where each abscissa scale division represents about 5 seconds. The DNA histogram associated with the whole of each data set is shown adjacent to the Y-axis. Figure 9.22 shows the results of an unperturbed run where the even distribution of cells in Gl and G2 + M with time is apparent. The coefficient of variation of the Gl peak was 3.4%. Figure 9.23 shows the results obtained when the sheath feed tubes were partially occluded on three occasions, once at 5 seconds for about 1.0 seconds and twice for about 0.5 seconds at approximately 13 and 14.5 seconds into the run. The perturbations are readily appreciated where on each occasion
QUALITY CONTROL
183
Figure 9.22. DNA content plotted versus time in an unperturbed run where the even distribution of cells in Gl and G2 + M with time is apparent. there was the expected 'smearing' of the fluorescence data and consequent loss of definition particularly noticeable at the base of the Gl peak of the DNA histogram. These data were redisplayed from the list-mode data file commencing at 15 seconds (beyond the disturbance) to give a histogram indistinguishable from that in figure 9.22. It was also gratifying to note that the instrument stability returned immediately the constriction was removed. Figure 9.24 shows the expected effect due to defocussing the laser and the severe data degradation is obvious. However, by redisplaying the list-mode file from disk and excluding the data between 15 and 45 seconds it was possible to obtain a histogram which was almost identical to that in figure 9.22, although it contained only 395 7 cells. The CV of the Gl peak for the 'resurrected' data from figure 9.24 was 3.7% compared with 3.4% for that in figure 9.22. Partial blockage was not attempted in these experiments for the obvious reason that nobody in their right mind would actively set out to induce such a perturbation. However, the data in figures 9.23 and 9.24 partially simulate this condition, and it can be seen that by including the time parameter in the list-mode data base it is possible not only to see if a perturbation has occurred and for how long, but also to extract useful information from a data set by being able to 'excise' degraded information recorded during the perturbation. As a consequence of these studies we now routinely incorporate the computer time stamp into all data files.
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INSTRUMENT PERFORMANCE
Figure 9.23. Perturbation induced by partial occlusion of the sheath feed tubes on three occasions at 5 seconds for about 1.0 sees and twice for about 0.5 seconds at approximately 13 and 14.5 seconds into the run. This was responsible for the loss of definition particularly noticable at the base of the G l peak of the DNA histogram.
9.9
Instrument hygiene
Keeping any instrument clean is obviously a pre-requisite for obtaining good performance and a dirty instrument will always produce a considerable quantity of noise arising from a number of sources which were discussed in section 9.1. It is also extremely important to keep the sample feed tube scrupulously clean. Obvious sources of noise include cells left over' from a previous assay and this is particularly likely to occur if there is a partial blockage in the feed tube or any of its connections. Not so obvious is the problem of fluorochromes becoming adsorbed into plastic or silicone rubber feed lines. The lipophilic substrate fluorescein diacetate (FDA) is particularly bad in this respect and spuriously positive immunofluorescence results have been obtained in our laboratory as well as in others when surface marker stained cells have been run immediately after FDA analyses. We have also encountered this problem after Hoechst 333A2 staining which is also lipophilic. Another fluorochrome which tends to 'hang around' in the tubes is acridine orange and, furthermore, the phenanthridinium dyes can interfere with the red/green emission of acridine orange for simultaneous RNA and DNA analysis.
INSTRUMENT HYGIENE
185
Figure 9.24. Laser defocussing to simulate unstable flow generating gross degradation of the data. The latter were excised to give a resurrected histogram indistinguishable from that in figure 9.22.
Apart from automatic 'back-flushing', which will get rid of the cells from the previous sample, there are a number of remedies that can be used. Saturated urea dissociates proteins and as the majority of junk in the tubes is likely to be protein you can help to keep things running by flushing through with urea. A word of warning. Some flow cells are stuck to their hydrodynamic focussing cones with a cement which is dissociated by urea, so check with the manufacturer before you perform this manoeuvre. We have also run through acid—pepsin which very effectively gets rid of any accretions of protein. Flushing through a dilute solution of bleach usually is very effective at removing fluorochromes adsorbed to sample feed-tube, but make very sure that you get rid of the bleach before the next sample is run. If, however, you have any doubts the best solution to these problems is to replace the sample feed-tube. This doesn't take very long with the majority of instruments.
10 Light scatter applications
10.1
Forward scatter
Forward light scatter (also referred to as TALS', forward angle light scatter) is very rarely specified adequately and almost invariably is equated directly with cell size. Forward scatter is proportional to particle size at narrow forward angles. The operative word here is narrow, and the relationship is strictly only valid over collection angles between about 0.5 and 1.5°. At wider angles the correlations tend to break down. This is illustrated in figure 10.1 by the work of Mullaney et al. (1976) where total light scatter intensity at 62>2.S nm (helium-neon) is plotted on the ordinate versus diameter for particles with two different refractive indices. The latter were 1.533 and 1.373, which correspond approximately to fixed and unfixed cells respectively, and the collecting angle was between 3 and 5°. It will be noted that the scatter intensity between these particular angles is very insensitive for diameters of 7 to 13 |im which is the range of most interest in biology. Another problem encountered with all scatter measurements, irrespective of the collection angle, is the dependence on cellular orientation. A spherical cell with a centrally placed spherical nucleus constitutes no problem as the light scatter pattern will be orientation independent. However, cells which are not radially uniform in all orientations, e.g. nucleated disks such as chicken red blood cells (CRBCs) or elongated fibroblasts, can give rise to artefactual light scatter distributions. Loken, Parks and Herzenberg (1977) found a bimodal distribution with light scatter measurements from fixed CRBCs. The two peaks were sorted and each was rerun through the instrument and the same bimodal pattern was obtained indicating that the bimodality of the distribution was 'instrument generated 7 and due to different cellular orientation during interrogation. Sharpless, Bartholdi and Melamed (1977) have investigated the size and refractive index dependence of forward scattered light in both the vertical and horizontal directions using Sephadex beads with crossed cylindrical lens pair focussing. Their set up is shown in figure 10.2. The laser beam (488 nm) was focussed to a sheet of light across the stream flowing in a cuvette from bottom to top. As each bead entered the illuminating beam the lower detector exhibited a large signal but the upper detector exhibited a small signal. On emerging from the
FORWARD SCATTER
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Figure 10.1. Light scatter intensity (ordinate) versus diameter for particles with refractive indices of 1.373 ( # ) and 1.533 ( • ) at a collection angle between 3 and
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188
LIGHT SCATTER APPLICATIONS Upper detector
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Figure 10.3. Cartoon of oscilloscope traces from the vertical detectors shown in figure 10.2. The upper and lower traces are from the upper and lower detectors respectively with particles effectively flowing from left to right. As each bead entered the illuminating beam the lower detector exhibited a large signal but the upper detector exhibited a small signal. On emerging from the beam the particles elicited large signals in the upper detector but small signals in the lower. beam the particles elicited large signals in the upper detector but small signals in the lower. This is illustrated in figure 10.3 where the upper and lower panels depict the signals in the upper and lower detectors respectively and the particle in this diagram is effectively 'flowing' from left-to-right. The authors concluded that light was being scattered into the detectors from the surface of the particles, probably due to refraction, and representations of the physical processes involved are depicted in figure 10.4. Panels A and B show the scattering geometry of a particle entering and leaving the beam respectively and the numbers of photons intercepted by each detector are represented by the numbers of arrows. It might appear that the lower detector in panel A (beam entry) and the upper detector in panel B (beam exit) were receiving scattered light at narrower angles than the respective upper and lower detectors. However, this diagram is not to scale and the laser beam 'thickness' would be relatively much smaller than shown and the scattering angles into the detectors would not be sufficiently different to account for the effect. It is much more likely that light was being scattered by refraction from the surface into the lower detector on beam entry (panel A) and into the upper detector on beam exit (panel B). The conclusion by the authors that the signals were due to scattering from the surface of the particles was vindicated by the observation that not only the amplitude, but also the time interval between the signals in the lower and upper detector, were proportional to size. This is shown in
FORWARD SCATTER
189
B
Upper detector
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Lower detector
Figure 10.4. Scattering geometry for vertical detectors where the particle enters the beam in panel A and emerges from the beam in panel B. figure 10.5 where the summed signals from both detectors are reproduced for a small and a large particle. An accurate measure of cell size can be obtained by quantitating the width (time-of-flight) of the large pulse in either the upper or lower detector (figure 10.3). A measure of particle size plus laser beam focussing depth can be obtained from analysis of the distance between pulses for different sized particles (figure 10.5). With Very small' objects the distance between peaks of figure 10.5 will approximate to the depth of the focussed light sheet. In contrast to the results from the vertical detectors Sharpless et al. (1977) found
190
LIGHT SCATTER APPLICATIONS
O O)
Time —• Figure 10.5. Summed signals from the vertical detectors where the larger signals from the larger object are spaced further aparc than the smaller signals from the smaller particle.
that the pulses from the horizontal detectors depicted in figure 10.2 were uniform and single, which was to be expected. This is the more usual configuration for measuring forward light scatter and the results of this particular study serve to illustrate the importance of detector position in relation to the geometry of focussing and cell stream. Loken et a\. (1976) found five peaks in mouse bone marrow on forward light scatter analysis integrated over the angular range of 2 to 8°. Each of the peaks was sorted, fixed and stained with Wright-Giemsa stain. The lowest intensity peak contained debris. The next most intense peak contained mainly mature red cells and the next peak contained small lymphocytes and some normoblasts. The second most intense peak contained polymorphonuclear leukocytes, large lymphocytes and normoblasts. The most intense peak, which was effectively a shoulder of the previous peak contained very large blast cells with some of the cells found in the second most intense peak. Each of the peaks contained a heterogeneous mixture of cells and it was evident that scattering intensity was not just related to cell size. This was particularly noticeable in the second most intense peak which contained the polymorphonuclear leukocytes which are larger than normoblasts but which scattered light of the same intensity at this particular angle. This result was not unexpected in view of the work of Mullaney et al. (1976), which was reproduced in figure 10.1, where there was considerable insensitivity of forward light scattering to size over a collection angle of 3 and 5° which is a fairly commonly used acceptance angle. Otten and Loken (1982) have studied forward light scatter at two different wavelengths (argon UV, 351 nm +363 nm, and 488 nm) simultaneously and found that the two signals were not equivalent. Small T- and B-lymphocytes from peripheral lymph nodes as well as mitogenically activated large T- and Blymphocyte blasts were discriminated at both wavelengths. Moreover, there were also light scattering differences between Lyt-2 positive and negative Tlymphocytes. Dual colour analysis of bone marrow revealed that differences were also apparent between small bone marrow cells and peripheral B-cells with an increase in UV forward scatter coinciding with the appearance of surface immunoglobulin on the former.
DUAL-ANGLE SCATTER
191
The most important single function of forward (or indeed any angle) light scatter measurement is to provide an independent variable. There are many fluorescence assays in which there are subpopulations of cells with little or no fluorescence. Thus, if we have two populations, only one of which is fluorescent, and we want to know the proportions of positive cells in the sample then it is absolutely pointless using the fluorescence channel as the master triggering channel (see section 4.2.4) as the non-fluorescent cells will not trigger the system and the answer you will get will be 100%. To answer this type of question you must trigger on an independent parameter such as light scatter which will allow all cells, not just those with fluorescence, to be 'seen' by the system.
10.2
Dual-angle scatter
A number of dual-angle light scatter studies have been carried out in a number of different systems. Jovin et al. (1976) have studied the light scattering properties of different diameter polystyrene beads simultaneously at two angles, which were variable. A ratio function of the scatter intensity at the two angles was developed where the experimental results agreed almost exactly with theoretical predictions from Mie theory (1908). Sorting was carried out with a binary mixture of 0.794 and 1.011 |lm beads using the ratio function in the sort decision logic and sorted purity of over 95% with a recovery of about 90% was achieved. A mixture of 0.794, 1.011 and 2.02 (im beads was also analysed and these results are reproduced in figure 10.6 where the top and middle panels show the scatter intensity histograms at 12° and 19° respectively. Clearly, there is considerable overlap between distributions but when the ratio function was applied the results in the bottom panel were generated and the three bead sizes were clearly delineated. Steinkamp, Hansen and Crissman (1976) used a combination of fluorescence pulse width analysis of propidium iodide/FITC stained cells to obtain nuclear and cytoplasmic diameters respectively and hence they were able to calculate nuclear/cytoplasmic ratios. These results were also duplicated with the combination of scatter for cytoplasmic size and mithramycin—DNA staining for nuclear size and applied to gynaecological samples. J. M. Thompson et al. (1985) have used forward and 90° scatter both individually and in combination plus anti-monocyte antibody staining to discriminate between lymphocytes and monocytes in Ficol—Paque prepared blood samples. These authors concluded that 90° scatter alone gave the most efficient discrimination between the two cell types and they also pointed out some of the difficulties encountered with morphological identification of monocytes. In previous studies by Salzman et al. (1975b), where forward and 90° scatter were used to discriminate between, and sort, lymphocytes and monocytes, a proportion of 80% of the monocyte peak was identified morphologically as being monocytes with a 15% 'contamination' of lymphocytes. However, it is not possible to distinguish between monocytoid lymphocytes and lymphocytoid monocytes
LIGHT SCATTER APPLICATIONS
192
4)
128 256 Scatter 12°
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128 256 Ratio 12°:19° Figure 10.6. Scatter intensity histograms from a mixture of 0.794, 1.011 and 2.02 Jim at 12° (top panel) and 19° (middle panel). The bottom panel shows the histogram after applying the ratio function where the three bead sizes were clearly delineated.
purely on morphological criteria (Zucker-Franklin, 1974) and the study of J.M. Thompson et al. (1985) made this distinction more comprehensively with the addition of the anti-monocyte monoclonal antibody. J. M. Thompson et al (1985) also reported that gating out the monocyte cluster in the forward versus 90° light scatter data space tended to result in exclusion of some lymphocytes; however, this is possibly partly dependent on instrument configuration and geometrical set up. They were not using crossed cylindrical lens pair focussing, but with the latter we have found the discrimination between lymphocytes and monocytes to be good using this combination of parameters where the two clusters exhibited distinctly different biochemical properties (see section 14.2.4). A typical 90° versus forward light scatter data set obtained from
DUAL-ANGLE SCATTER
t 0>
193
Granulocytes /
Monocytes Lymphocytes Forward scatter — • • Figure 10.7. Typical dual parameter 90° versus forward light scatter data obtained from peripheral blood white cells in the Cambridge MRC instrument.
peripheral blood leukocytes with our instrument is shown in figure 10.7. The lymphocyte, monocyte, granulocyte and debris clusters are superficially well defined. The debris cluster contains fragments, red cells and platelet aggregates. S. C. Thompson, Bowen and Burton (1986) also obtained a good discrimination between lymphocytes and monocytes in rats using the forward and 90° scatter combination. They were using crossed cylindrical lens focussing, but they also report subtotal discrimination between the two cell types. Similar conclusions were drawn by Fleisher, Marti and Hegengruber (1988) using 90° scatter and volume measurements. The latter parameter presumably was an impedence Coulter-type volume measurement but this was not explicitly stated in the paper, an omission which should have been spotted by the referees. Visser, van der Engh and van Bekkum (1980) used forward versus 90° scatter to analyse mouse bone marrow and their results are reproduced in figure 10.8. A number of clusters are apparent which are similar to our results shown in figure 5.4 (Dive, 1988). Importantly, Visser et al. (1980) sorted the various populations and found that only the blast cell regions contained pluripotent bone marrow stem cells which generated spleen colonies in irradiated mice. The combination of 90° plus forward scatter revealed two subsets in T8positive cells (Terstappen et al, 1986), discriminated between small lymphocytes and blasts in stimulated mixed lymphocyte cultures (MacDonald and Zaech, 1982) and identified pancreatic B-cells (Nielsen et al, 1982). This combination of parameters has also been shown to change with chemotactic stimulation of neutrophils after treatment with peptide addition (McNeil et al, 1985). Initially, 90° scatter decreased and forward increased but, after about 180 seconds the
194
LIGHT SCATTER APPLICATIONS
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reverse was noted. Hence, the ratio of 90°: forward scatter exhibited an initial decrease then a sustained increase. The initial phase was attributed to membrane 'ruffling' of stimulated cells and the later phase to polarization of neutrophil morphology. Also, 90° scatter has been used by van Bockstaele, Berneman and Peetermans (1986) to analyse peripheral blood subsets in hairy cell leukaemia. Epstein, Watson and Smith (1988) used a combination of 90° pulse width and area to distinguish between mitotic and G2 cells. The latter authors used this to analyse drug-induced cell-cycle delay in a subset of a human breast tumour cell line recruited into the cell cycle by oestrogen stimulation. Also, 90° light scatter has been found to be reduced in mitotic cells by Zucker et al. (1988), and has been used to discriminate between myogeriic cells in embryonic skeletal muscle (YablonkaReuvein, 1988).
10.3
Viability determination
The combination of 90° and forward light scatter can assist in making a discrimination between viable and non-viable cells in some cell types. This is illustrated in figure 10.9 which shows four clusters in the forward versus 90° light scatter data space obtained from EMT6 mouse mammary and H69 tumour cells. In these experiments the cells had been held in PBS without added protein for about two hours which reduces their viability. The preparations were then incubated
VIABILITY DETERMINATION
195
with propidium iodide (PI) and fluorescein diacetate (FDA) and analysed with the red (PI) and green (FDA) photomultipliers as well as with the two scatter detectors. Viable cells exclude the highly polar PI but retain fluorescein after the lipophilic fluorogenic substrate FDA is hydrolysed by intracellular esterases. Thus, viable cells are scored as green-positive but red-negative. Non-viable cells cannot exclude PI and hence fluoresce red but they cannot either retain fluorescein or hydrolyse FDA and consequently are green-negative. The A clusters in figure 10.9 were clumps of two or more cells identified by pulse shape analysis (see section 9.8.3). The B clusters contained a majority (>90%) of red-negative but greenpositive cells and these represent the viable fraction. The C clusters contained the non-viable red-positive but green-negative cells ( > 85%) and the D clusters were composed of green-negative and red-negative/events' compatible with fragments. Note that the fragments have very little forward scatter as this is not a particularly sensitive measurement on our instrument but they do have considerable 90° scatter. In this particular example the viable fraction constituted 46% of the total which compared with an estimate of 54% using trypan blue exclusion. With EMT6, H69 and some lymphoblastoid cells we obtain good agreement between trypan blue exclusion and light scatter viability estimates, but this should not be taken as being a universal phenomenon. Each cell type must be evaluated individually. Furthermore, we have always observed some non-viable (red-positive, greennegative) cells in cluster B and some viable cells (red-negative, green-positive) in cluster C. Thus, dual parameter light scatter estimates of viability do not, repeat
90° Scatter
90° Scatter
Figure 10.9. Partial viable/non-viable cell discrimination using forward and 90° light scatter for EMT6 and H69 cells. The A clusters are composed of clumps. Cells in the B clusters exclude propidium iodide (red-negative) and retain fluorescein (green-positive). The C cluster cells do not exclude propidium iodide (red-positive) and do not retain fluorescein (green-negative). The D clusters are rubbish.
196
LIGHT SCATTER APPLICATIONS
not, give an absolute discrimination. Nevertheless, we have found this technique in conjunction with propidium iodide to be very useful in enzyme kinetic studies (Dive, Workman and Watson, 198 la, b, 1988; Dive, 1988) as a means of excluding the majority of non-viable cells from the analyses. Moreover, the discrimination between live and dead can sometimes be enhanced by substituting carboxyfluorescein diacetate for fluorescein diacetate as the former releases carboxyfluorescein, which is more polar than fluorescein and is retained more efficiently by the live cells. This has recently been used in studies with membraneactive cytotoxic agents and revealed that green fluorescence (FDA) is lost before red (propidium iodide) fluorescence is gained (Dive, Workman and Watson, 1990). The discrimination between live and dead cells using light scatter can be more difficult than in the example illustrated by figure 10.9 and the following problem came to light when characterizing a T-cell clone for thy-1, CD4, CD5 and CD8 immediately after removel from liquid nitrogen (Wing et a\., 1990). Trypan blue exclusion revealed a viability of less than 20% and propidium iodide (final concentration 5 mg 100ml" 1 ) was added and both forward and 90° light scatter were collected together with red propidium iodide fluorescence and green immunofluorescence elicited with a double layer technique. Figure 10.10 shows the fluorescence control data set obtained with an irrelevant first antibody plus fluorescenated second antibody. It was these data which were used in the illustration of mono-dimensional gating in figure 5.14. Panel a shows the contour plot of forward versus 90° scatter which is very similar to figure 10.9 and two regions Rl and R2 were defined. The latter represents debris and the arrowed population corresponds to cluster C of figure 10.9. Panel b shows red fluorescence versus 90° scatter for region 1 cells (Rl) of panel a. This secondary data space was now gated into red-negative (Si) and red-positive (S2) clusters respectively. Panel c plots green fluorescence versus 90° scatter for the red-negative region (Si) of panel b. This clearly identifies both a green-negative and a green-positive cluster,
if
1
90° scatter
T2
S2
m sr
90° scatter
/
T1 90° scatter
Figure 10.10. Initial analysis of fluorescence control data set from T-cells immediately after removal from liquid nitrogen. Panels a, b and c respectively show forward scatter, red fluorescence and green fluorescence all versus 90° scatter.
197
VIABILITY DETERMINATION
4) O C 4> U (A
4) C 4>
luore
esc
B2
o 3 "O 4> CC
0*
C2
c
?\ fpTfpuv
90° scatter
/
/
4> 4>
O
0
C1 90° scatter
E2
E1 90° scatter
90° scatter
Figure 10.11. The same data set as shown in figure 10.10 but with an additional region set in the forward versus 90° light scatter data space, see text.
Tl and T2 respectively. It should also be noted that the green-positive cluster (T2) exhibits slightly less 90° scatter than the Tl green-negative cluster. These data were a little disturbing as a significant fraction of the red-negative, apparently viable, cells in the control were exhibiting green fluorescence which should not have been present. The contour plot in figure 10.10a was then inspected more carefully and a distinct shoulder could be seen to be included in the gated region Rl and the data set was then regated. This is illustrated in figure 10.11a where region A2 includes the shoulder. Panel b shows red fluorescence versus 90° scatter for region A l which is directly analogous to panel b of figure 10.10 and this was similarly gated into red-negative and red-positive regions, Bl and B2 respectively. Panel c shows that the red-negative Bl region of panel b contains almost no green-positive cells. A similar procedure was then carried out for region A2 cells of panel a. These results are given in panels d and e which show that there are very few red-positive cells, panel d region D2, and that the rednegative fraction, Dl, contains the non-specifically labelled green-positive cells, panel e region E2. In summary, these various data were interpreted as follows.
198
LIGHT SCATTER APPLICATIONS
Some cells in region A l were non-viable and could be excluded from subsequent analysis on their red fluorescence, region B2, leaving the Bl cells as the fluorescence controls. 'Events' within region A2 consist primarily of large debris which are essentially red-negative (panel d) and a proportion of these are greenpositive, panel e, region E2. Thus, a combination of forward and 90° light scatter plus propidium iodide exclusion enabled immunofluorescence characterization to be performed in cells extracted directly from liquid nitrogen where there was known to be a large fraction of dead cells and debris.
10.4
Multi-angle scatter
Multi-angle light scatter measurements have not yet enjoyed widespread use for two main reasons. Firstly, there are no regular commercial flow cytometers available which can perform such measurements and secondly, the data handling problems are considerable. These types of measurements can only be seriously investigated in highly specialized laboratories and a group at Los Alamos has carried out the majority of work in this area. The problems arise not with collecting the data but with interpreting and presenting it when it has been acquired. Most commercial instruments could be adapted to function with a multi-angle detector (see section S.2) but 32-dimensional data handling requires very considerable main-frame computer power with cluster analysis capability. A number of cluster analysis algorithms have been developed since Goad (1978) specifically addressed this type of flow cytometric data handling problem using similar techniques to those of Ludlam and Slansky (1977). However, these require considerable expertise for their correct operation and interpretation and they have not yet reached sufficient maturity for non-expert use and there is a move now towards using expert systems (Waterman, 1986; Harmon, Maus and Morrissey, 1988) to assist with such problems. In spite of these data handling problems it is possible to use multi-angle scatter to distinguish between a number of different cell types some of which are very similar morphologically. Price et al (1976) and Price, Kollman and Salzman (1978) have discriminated between two physically similar organisms Chlamydemonas reinhardii and Chlorella pyrenoidosa in mixed cultures using such measurements. Initially, each cell type was analysed separately to establish the characteristic multi-angle scatter 'finger-print' and they were then run as a mixture. These data are shown in figure 10.12 which is redrawn from the data of Salzman, Mullaney and Price (1979). Light scatter intensity is plotted on the ordinate versus scattering angle on the abscissa where the data from chlorella are cross hatched from bottom left to top right and those from chlamydemonas are cross hatched from top left to bottom right. The light scatter intensity limits at each angle for each organism are drawn at the + 1 standard deviation level calculated from the cluster analysis algorithm. This analysis system was used to classify unstained leukocytes (Salzman et al, 1975b) and extended to gynaecological specimens by Salzman et al. (1976) where squamous cells were distinguished from both lymphocytes and granu-
199
MULTI-ANGLE SCATTER
0.9
1.9
3.5 6.5 11.6 Scatter angle
19.3
Figure 10.12. Multi-angle light scatter patterns from chlorella (cross hatched from bottom left to top right) and chlamydemonas (cross hatched from top left to bottom right). locytes on their cluster patterns. These data are reproduced in figure 10.13 where the display is similar to that of figure 10.12 and where the patterns for the three cell types are readily apparent. Loken et al. (1976) used their sweep-scanning system to investigate the multiangle scattering properties of a number of synthetic particles and obtained characteristic patterns for 2.02, 6.0 and 11.0 |im plastic microbeads and they were also able to distinguish two separate subsets of mouse thymocytes by their multiangle light scatter 'finger-print'. Very little work has been carried out in multi-angle light scattering over the past decade for a number of reasons, some of which, namely, the problems of data handling and the measurement orientation dependence, have already been considered. There is also a further reason; the advent of monoclonal antibody technology, which allows very much greater identification specificity to be achieved. However, the new generation of 32-bit micro-processors and the development of expert systems and more reliable pattern recognition procedures (Murphy, 1985) may enable multi-angle light scattering techniques to be reevaluated as a generally useful adjunct within the flow cytometry armamentarium.
LIGHT SCATTER APPLICATIONS
200
©
-
(0
Sea tter int ensity
o
-
•.
i
i
10
i
J
15 20 Scatter angle
•"
••
i
25
Figure 10.13. Multi-angle light scatter patterns from leukocytes, top panel, and gynaecological exfoliated squamous cells, bottom.
11 Nucleic acid analysis
It seems almost ridiculous to start this chapter by stating that there are two nucleic acids, ribo- and deoxyribo-nucleic acids, RNA and DNA respectively, as everyone knows this. However, I had to start somewhere. DNA is the custodian of all the fundamental data (but not all the information, it's that distinction again) required to construct most biological entities be these E. coli, amoebae, daffodils, elephants or humans. It is the 'Encyclopaedia Biologica' which has the inherent capacity within its structure to be replicated exactly (Watson and Crick, 1953). The retro viruses are the exceptions in which the genetic material is RNA, and these organisms use the DNA of a cell in their replicative process.
11.1
Nucleic acid stains
A large number of fluorescent ligands bind to the nucleic acids. Each is fluorescent in its own right but the fluorescence is modulated or enhanced very considerably after binding to RNA or DNA. These fluorescent stains fall into four categories namely, DNA specific, nucleic acid specific, non-specific poly-anion and RNA 'part-specific' stains.
11.1.1 DNA specific The fluorochromes in this category which are most useful in flow cytometry include the antibiotics chromomycin A3, olivomycin and mithramycin, DAPI (4/,6-diamidino-2-phenylindole), its analogue DIPI (4',6-bis(2'imidazolinyl4H,5H)-2-phenylindole) and the bisbenzimidazole group of dyes which are identified by their Hoechst 'telephone numbers'. Chromomycin, olivomycin and mithramycin are similar tricyclic agents. They have the common structure shown in figure 11.1 and they differ in sugarcontaining side chains (Ward, Reich and Goldberg, 1965; Kersten, Kersten and Szybalski, 1966). Studies of supercoiling properties of DNA bound with these ligands suggest that they do not intercalate (Waring, 1970) and all three bind preferentially to G-C rich DNA (Kersten et al., 1966; van de Sande, Lin and Jorgenson, 1977). Mithramycin can be used very effectively as a fluorochrome for DNA histograms (Crissman and Tobey, 1974; Tobey and Crissman, 1975; Crissman, Oka and Steinkamp, 1976; Taylor, 1980) and chromomycin A3 has been
202
NUCLEIC ACID ANALYSIS Tricyclic antibiotics
Figure 11.1. Common structure of the fluorescent DNA binding antibiotics, chromomycin A3, olivomycin and mithramycin, which differ in their sugar side chains, Rl and R2.
DAPI
DIPI
Figure 11.2. Structures of DAPI and DIPI.
used extensively in conjunction with Hoechst 33258 for chromosome analysis (see chapter 13). All three fluorochromes have similar spectral properties with maximum absorption in the violet at about 400 nm and a peak emission in the green at about 540 nm (Crissman et al, 1979). The phenylindoles were introduced by Dann et al. (1971) and the structures of DAPI and DIPI are shown in figure 11.2. They were first used in flow cytometry as DNA dyes by Stohr et al {1977) and have very similar spectral properties to the Hoechst dyes (see below). They bind non-intercalatively to repetitive A—T rich regions, another similarity with Hoechst ligands. Both dyes can be used in rapid nuclear isolation techniques (Taylor, 1980; Taylor and Milthorpe, 1980; Thornthwaite et al, 1980) and the fluorescence from the phenylindoles bound to DNA is very intense. Otto and Tsou (1985) have compared them with Hoechst 33258 and 33342 as chromosomal DNA stainds and found that they are about 15% brighter than the Hoechst dyes; furthermore, DAPI gave a lower CV than the Hoechst dyes, 2.2% compared with 2.8%. Hoechst 33258, see figure 11.3, was the lead bisbenzimidazole compound and was used as a DNA stain in the late 1960s (Herzog and Schutze, 1969; Lammler
NUCLEIC ACID STAINS
203
Bisbenzimidazole dyes
R - N
33258
HOECHST
R
-
R1 =
C Ho "OH
Figure 11.3. Structure of Hoechst 33258.
and Schutze, 1969; Hilwig, 1970). A large number of related compounds were developed by Loewe and Urbanietz (1974) in a search for drugs active in filariasis and many of these were investigated as probes for DNA synthesis (Latt and Stetton, 1976). The physicochemical properties of the bisbenzimidazoles are consistent with the hypothesis that they bind tightly to DNA in the external grooves of the helix (Mueller and Gautier, 1975; Bontemps, Houssier and Fredericq, 1975) and that this binding is preferentially to repetitive A—T sequences (Weisblum and Hanessler, 1974). The optical properties are pH-dependent (Latt and Wohlleb, 1975; Hilwig and Gropp, 1975) and are consistent with two modes of binding (Bontemps et al., 1975; Latt and Wohlleb, 1975) and see section 11.8. Hoechst 3325S also binds very weakly to RNA, particularly at moderate ionic strength (Latt and Stetton, 1976; Hilwig and Gropp, 1975) but the fluorescence emission is considerably less than with DNA and has not constituted a problem in our hands. The Hoechst dyes are particularly interesting on two counts. Firstly, some can be used as vital DNA stains (Hoechst 33342) yielding viable cells after staining and sorting (Arndt-Jovin and Jovin, 1977; Hamori, et a\., 1980; Lydon, Keeler and Thomas, 1980). Secondly, the emission spectrum is dependent on dye/DNA phosphate ratios, pH and chromatin structure (see section 11.8). Although the DNA specificity of this group of fluorochromes is an advantage they do have the disadvantage of needing UV, violet or low-blue excitation. This necessarily means that laser-based flow cytometers must be equipped with either a high power laser capable of being tuned to UV and blue lines or with an additional small helium-cadmium laser for a 'dedicated' UV-line. 11.1.2 Nucleic acid specific The major fluorochromes under this heading, the phenanthridinium dyes, are ethidium bromide (2,7-diamino-9-phenyl-10-ethylphenanthrinidinium bromide) and propidium iodide (3,8-diamino-5-diethylmethylamino-propyl-6phenylphenanthridium diiodide). You can see why they are usually just called EB and PI, and their structures are shown in figure 11.4. These dyes bind to both RNA (Gatti, Houssier and Fredericq, 1975) and DNA in two binding modes. The first
204
NUCLEIC ACID ANALYSIS
ETHIDIUM BROMIDE
\ — /
PROPIDIUM IODIDE
Figure 11.4. Structures of ethidium bromide (EB) and propidium iodide (PI).
involves intercalation with double-stranded helical structures and results in considerable enhancement of fluorescence from the dye/DNA complex compared with free dye (Le-Perq and Paoletti, 1967; Waring, 1970) and dye-dependent unwinding of the helix can be induced by ethidium bromide (Waring, 1965). The primary intercalating binding mode is essentially independent of base pair sequence although Mueller and Crothers (1975) have reported a very weak preference for G-C sites. Secondary electrostatic binding of ethidium bromide to the external domains of double-helical structures can also take place and this is associated with a decrease in fluorescence yield. However, this phenomenon can be reduced by using relatively low ionic concentrations (le-Perq and Paoletti, 1967). Chromatin-associated proteins may reduce the accessibility of the dyes to binding sites either by physically covering the sites or by modifying nucleic acid conformation (Angerer and Moudrianakis, 1972; Brodie, Giron and Latt, 1975). Propidium iodide was introduced by Hudson et al. (1969) in a procedure to distinguish between the dye-dependent density of linear and closed circular DNA. These phenanthridinium dyes are polar, highly soluble in water and do not readily cross functionally intact external cell membranes. Reliable estimates of DNA content requires that cells be permeabilized or the nuclei isolated. Thereafter, both types of preparation should be treated with ribonuclease, including isolated nuclei as nucleoli can contain considerable quantities of RNA in some cell types. Both dyes are excited by the 488 nm argon line and a small 5 mW laser is more than adequate, which is a considerable saving on capital expenditure if all you want to do is DNA histograms. There is nothing to choose between PI and EB just for DNA histograms except that EB is cheaper. Both dyes emit in the orange/red region of the spectrum. However, the emission from PI is more towards the red which means that this is the fluorochrome of choice for any double staining of a second cellular constituent using fluorescein (Crissman and Steinkamp, 1973).
11.1.3 Non-specific poly-anion stains A group of basic (cationic) dyes, the tricyclic heteroaromatic family, bind to poly-anion complexes including RNA and DNA. Not only these dyes, but also
NUCLEIC ACID STAINS
205
many others, have been used in 'classical' histochemical studies for over a century. The structure of the tricyclic heteroaromatic compounds is shown in figure 11.5 and the X, Y, Rl, R2, R3 and R4 groups are given in table 11.1 for the dyes most likely to be used in flow cytometry. Acraflavine was developed therapeutically by Ehrlich as an antibacterial agent and this was used in conjunction with methyl and crystal violet as a bacteriostatic cocktail by Churchman (1927). Pyronin (there'll be more about this in the next section) was also used by Ehrlich in conjunction with methyl green, methylene blue and acid fuchsin in cell morphological studies in anaemia (Ehrlich and Lazarus, 1898). It was also known by the turn of this century that some cells exhibited pronounced cytoplasmic basophillia with the tricyclic heteroaromatic dyes (Ehrlich et al.f 1903), and this was later appreciated to be nucleic acid (RNA) associated (Brachet, 1940a,b). Work in the 1940s established that many of these dyes have metachromatic fluorescence properties (Metcalf and Patton, 1944), and Strugger (1948) demonstrated that UV excitation of acridine orange stained soil samples elicited green fluorescence from bacteria and red from humus particles. Metachromatic fluorescence from acridine orange stained eukaryotic cells was discovered by a Russian scientist, Meissel (1951), who noted that green and red fluorescence were emitted from the nucleus and cytoplasm respectively. This was confirmed in the mid 1950s by von Bertalanffy and Bickis (1956), Armstrong (1956) and Schummelfeder, Ebschner and Krogh (1957). In 1959 Bradley and Wolf proposed that intercalation of the dye molecules between the bases in doublestranded nucleic acids gives rise to green emission and that electrostatic stacking of dye molecules along single-stranded species gives rise to red fluorescence. Mueller and Crothers (1975), Mueller, Bunemann and Dattagupta (1975) and Mueller and
Tricyclic heteroaromatic dyes x
NR 3 R 4
Figure 11.5. Structure of the tricyclic heteroaromatic dyes.
Table 11.1. Tricyclic heteroatomic dye structures Dye Acridine orange Pyronine Y Oxanine 1
CH CH N
Y
Rl
R2
R3
R4
NH O O
CH3 CH3
CH3 CH3 CH3CH3
Ch3 CH3 CH2CH3
Ch3 CH3 CH2CH3
CH2CH3
206
NUCLEIC ACID ANALYSIS
Gautier (1975) confirmed not only that heteroaromatic compounds intercalate with double-stranded nucleic acids, but also showed that they bind preferentially to G—C sequences. Polymer formation (Sculthorpe, 1978) as a consequence of dye molecule stacking with single-stranded nucleic acids, which can be with either RNA and DNA, leads to aggregation and precipitation (Kapuscinsky, Darzynkiewicz and Melamed, 1982) and is probably responsible for metachromasia. A major contribution to the application of flow cytometry in cell biology has been made by Darzynkiewicz and colleagues at the Sloan Kettering Memorial Hospital in New York who have developed a number of techniques using acridine orange. These include methods for selectively denaturing any double-stranded RNA to single-stranded forms whilst maintaining the double-stranded integrity of DNA (Darzynkiewicz et al, 1975, 1977a; Traganos et al, 1977). Hence measurements of RNA and DNA can be made simultaneously in each cell with a single dye and with a single excitation source as both forms of AO/nucleic acid complex are excited by the 488 nm argon line. Moreover, the fluorescence emission of both complexes is bright and extremely good results can be obtained with a low power, 5 mW, air cooled argon laser. This technique has also been used to study the sensitivity of chromatin in different cell cycle phases to heat denaturation enabling distinctions to be made between G2 and mitotic cells (Darzynkiewicz et al, 1977b) and to define a number of subsets in Gl on their RNA content (Darzynkiewicz, Traganos and Melamed, 1980). A word of caution must be sounded, however. None of the tricyclic heteroaromatic dyes are specific for the nucleic acids, they bind and fluoresce with many poly-anionic structures. These particularly include the mucopolysaccharides (now referred to as the glycosaminoglycans, e.g. heparin and chondroitin sulphate) which are found in basophils and mast cells both of which were christened by Ehrlich et al. (1903). Indeed, this class of dye is used in the periodic acid-Schiff (PAS) reaction to identify glycosaminoglycans, hence, their use as nucleic acid stains must be carefully controlled. 11.1.4 RNA 'part-specific' As yet there is no ideal RNA specific dye although rumours exist that such an agent might soon be forthcoming. By ideal I mean that it should bind exclusively to RNA, that the bound complex should have considerably enhanced fluorescence compared with free dye and finally it should be excitable by an easily obtainable lasing line, i.e. 488 nm, at low light power. Flow cytometric efforts to assay for RNA, as opposed to RNA and DNA simultaneously with acridine orange (see sections 11.1.3 and 11.7.1) are based on observations with classical histochemical light absorption staining including methyl green and pyronin (Taft, 1951; Kurnich, 1955; Perry and Reynolds, 1956). This dye combination stains nuclei green and cytoplasm red corresponding to DNA and RNA respectively as with acridine orange fluorescence. Four dyes, pyronin-Y (Tanke et al., 1981; Shapiro, 1981), thioflavine-T (Arndt-Jovin, 1979), oxanine-1 (Shapiro, 1981) and thiazole orange (Lee, Chen and Chiu, 1986) have
THE CELL CYCLE
207
been used to assay for RNA. The most useful are pyronin-Y and thiazole orange with respective absorption maxima at 540 nm and 510 nm, hence both can be excited by the 488 and 514 nm argon lines. Although pyronin-Y is not absolutely specific for RNA, it is a tricyclic heteroaromatic compound which binds to DNA and glycosaminoglycans, about 75% of its associated fluorescence can be abolished by ribonuclease treatment in fixed cells. Oxanine-1 has a maximum absorption well into the red at 630 nm with very far red fluorescence and has been used by Shapiro (1981). Again, this dye is not specific for RNA but between 60 and 80% of its fluorescence is ribonuclease sensitive. Lee etal. (1986) have used thiazole orange as an RNA reticulocyte stain.
11.2
The cell cycle
In 1951 Howard and Pelc discovered that the DNA synthesis period occupied a discrete interval separated temporally from mitosis. The immediate conclusion was that there must be at least four distinct phases within the division cycle, one of which, mitosis, had already been defined. They termed the postmitotic pre-synthetic phase Gl and the post-synthetic pre-mitotic phase G2. The 'G' designation stands for gap and a representation of this concept of the cell cycle, which stands to this day, is shown in figure 11.6. In 1959, Quastler and Sherman introduced the percent labelled mitosis (PLM) curve from which the durations of the intermitotic phase times could be deduced. In this technique cells are exposed to a pulse of tritiated thymidine, a radiolabelled precursor of thymine which is incorporated into DNA only during the DNA synthesis period. At regular intervals thereafter autoradiographs are prepared and the percentage of mitotic figures in the population which are labelled with silver grains is scored. These percentages are plotted against the time between labelling and sampling which gives a damped sigmoidal curve whose periodicity is that of the cell cycle. Computer model analysis of the PLM curve gives an estimate of the intermitotic phase times with their variances. Almost as soon as the technique became available it was apparent that the cell cycle time was invariably less than that of the doubling time of tumours growing in vivo. This gave rise to the conclusion that only a proportion of cells in the tumour were within the division cycle and Mendelsohn (1962) coined the phrase growth fraction for this compartment. An extra cell cycle phase, G-zero or Go, was proposed to describe immediately post-mitotic cells which spent some time in a Vesting' phase before re-entering the division cycle. In some tissues there is good evidence for the existence of such a compartment, e.g. peripheral lymphocytes which can be stimulated to divide by mitogens, but in many tumour tissues the evidence is tenuous. The PLM technique is labour intensive, very time consuming and it can take up to six weeks to obtain a result for the cycle time and that of the intermitotic phase times. The results obtained, namely the time it takes to complete the various phases, are generally not very interesting in themselves. However, specific biochemical manipulation of cells which induce changes in the phase times can
208
NUCLEIC ACID ANALYSIS
Figure 11.6. The cell cycle (after Howard and Pelc, 1951). give some insight into the biological processes which are modified by the manipulation. Flow cytometric techniques have now completely revolutionized cell cycle kinetics. We can obtain not only the cell cycle and intermitotic phase times but also the proportion in S-phase which is actively synthetic and discriminate these cells from those arrested with an S-phase DNA content in little more than the cell cycle time. In terms of man/woman-hours saved this represents a gain factor of between 20- and 30-fold quite apart from the fact that we obtain information that could not otherwise be acquired, namely the distinction between S phase DNA content cells which are synthesizing and those that are not. Furthermore, there are techniques for some types of cells which discriminate between G o and Gl and subsets within these groups.
11.3
The DNA histogram
The DNA histogram is a very simple data set which characteristically contains two peaks separated by a trough. The first peak, which is usually the larger, corresponds to cells with G 0 /Gl DNA content and the second, which should be at double the fluorescence intensity of the first, corresponds to cells with G2 + M DNA content. Any cell scored in the trough has a DNA content intermediate between Gl and G2 + M and these usually represent cells in S-phase. In a perfect data set, which doesn't exist, all Gl and G2 + M cells would be scored in single channels and any cells between or immediately adjacent to these would be in S-phase. This is shown in figure 11.7; however, in practice, the data are distributed due to a number of factors (see below) and the effect of this is shown in figure 11.8 where the dispersion is assumed to be Gaussian.
THE DNA HISTOGRAM
209
I stated that cells in the trough usually represent cells in S-phase and stressed the 'usually'. In unperturbed populations these cells are in S-phase; however, in populations perturbed by therapeutic intervention, radiation or drugs, it is possible for cells to have an S-phase DNA content which are either temporarily arrested or dead and are no longer synthesizing. Examples of this state will be given later and it is obviously important to make this distinction. The best analogy I have heard to describe this comes from Professor Len Lamerton who said 'you can sit down at the table to have dinner but you don't have to eat anything'. (He later admitted that he had heard it from someone else but couldn't remember who!) Distribution in the data is due to instrumental, staining and biological factors. Variation in illumination intensity due to core positioning instability is one possibility and was considered in sections 3.9.5 and 3.9.6. Staining variability between cells is another factor. This is most likely to occur wherever heterogeneous populations are being studied. These include normal tissues where there are different degrees of differentiation of cells within the sample as well as tumour samples. We do not measure DNA directly, we measure fluorescence. The quantity of fluorescence is directly proportional to the number of dye molecules bound to DNA and the number of binding sites can vary with the conformation of DNA and chrdmatin. Not only the quantity, but also the energy of fluorescence from some stains, e.g. acridine orange (see section 11.7) and Hoechst 33342 (see sections 8.4.3 and 11.8), are sensitive to the number of accessible binding sites and the state of the microenvironment. There may also be variation in the amount of DNA from cell to cell within apparently homogeneous populations. The mouse mammary EMT6/M/CC cell line, originally derived by Rockwell, Kallman and Fajardo (1972), has a between cell variation in its chromosome number from 50 to
Figure 11.7. Idealized DNA histogram with no dispersion where all G l and G2 + M cells are recorded in channels 200 and 400 respectively.
NUCLEIC ACID ANALYSIS
210
4 -
§ X
2 si o
2 -
"o en
20
30 DNA
40 FLUORESCENCE
50
60
70
INTENSITY
Figure 11.8. Example of a real DNA histogram with dispersion and a CV in the data of about 7%. The G l and G2 + M peaks whose true modal positions are channels 30 and 60 respectively are superimposed on the distributed S-phase component. This shifts the apparent G l modal channel towards G2 4- M and that of G2 + M towards Gl, hence the G2 + M : G l ratio will appear to be less than 2.0.
70 (Watson, 1977b). Furthermore, the binding of ligands to DNA (or indeed anything) is governed by dynamic processes. Wherever there is an association binding constant there is always a dissociation constant and the results that we see are governed by the law of mass action. Nicolini et al. (1979) have discussed this at length in relation to acridine orange staining. In order to think realistically about DNA histograms we have to consider the number of dye molecules in relation to the number of accessible binding sites. Although the former can be controlled experimentally, the latter may not be controllable as differences in chromatin structure in different cells and its organization in Gl, S and G2 + M in the same cells may make differences to the quantity of fluorochrome that can be bound per DNA phosphate residue. Some of these factors are considered further in section 11.6. The ratio of the means of the G2 + M : G l peaks should be 2.0 but an ADC offset (see section 9.7.1) and differences in the number of available dye binding sites in G2 + M and Gl may result in a ratio which is not equal to 2.0. Moreover, it is not generally appreciated that dispersion in the data can also effect this ratio. Consider figure 11.8. The 'slope' of the S/G2 + M interface is less steep than that of the Gl/S interface and the Gaussian distributed G2 + M and Gl peaks are 'addedon' to these respective interfaces. This results in a shift of the position of the Gl peak towards G2 + M and a shift of the latter towards Gl (Watson, 1977b).
DNA HISTOGRAM ANALYSIS
211
11.4 DNA histogram analysis The objective of DNA histogram analysis is to obtain a reasonable approximation for the proportions of cells in the Gl, S and G2 + M phases of the cell cycle. A great deal of time and effort has been expended on this using computer models of varying complexity (Baisch, Gohde and Linden, 1975; Baisch and Beck, 1978; Beck, 1978; Christensen et al, 1978; Dean and Jett, 1974; Fox, 1980; Fried, 1976, 1977; Fried and Mandel, 1979; Gray, 1974, 1976, 1980; Gray, Dean and Mendelsohn, 1979; Jett 1978; Johnston, White and Barlogie, 1978; Kim and Perry, 1977; MacDonald, 1975; Watson, 1977a; Watson and Taylor, 1977; Zeitz and Nicolini, 1978) and a comparative review of the various methods has been published (Baisch et al., 1982). As expected some models performed better than others not only with simulated but also with experimentally derived data; however, none was ideal. The models which performed best tended to be those requiring a large main frame computer and these also tended to contain a large number of variables for which a solution had to be found. It is not clear however, whether it was the computing power available on the main frames, hence time, or the intrinsic structure of the models which contributed to the better performances. All models coritain the common assumption that the Gl and G2 + M peaks are Gaussian distributed and they differ in the way in which the S-phase component is calculated.
11 A.I Age distribution theory Many models base the S-phase calculation on age distribution theory in exponentially growing populations (Steel, 1968) which is summarized in figure 11.9. In this diagram we assume, not unreasonably, that each cell divides into two at mitosis, and because of this assumption we define the probability of finding a cell of zero age (immediately after division) as 2.0. Hence, the probability of finding a cell of age unit cycle time, tc, is equal to unity where tc = tG1 + ^s + fe2 + M and where tG1, ts and tG2 + M are the durations of Gl, S and G2 + M respectively. The probability boundary falls exponentially from 2 to 1 throughout the cell cycle as the population is growing exponentially. The proportions of cells in Gl, S and G2 + M are now obtained by finding the area (which is done by integration, but I'm not going into that) within the age distribution occupied by the three phases, and that for S-phase is shaded in figure 11.9. When we translate the age distribution diagram into DNA histogram terms all those cells in the Gl region have the same DNA content and should be scored in a single channel (see figure 11.7). Similarly, all those in G2 + M should also be scored in a single channel at double the abscissa scale reading. The S-phase area of the age distribution spans the interval between the Gl and G2 + M peaks and the shape of its upper surface will be identical to the upper S-phase boundary of the age distribution diagram, subject to scaling factors, if the rate of DNA synthesis is constant. In practice, we have seen that the Gl and G2 + M peaks do not appear in a single channel of the DNA histogram due to the factors considered in section 11.3.
NUCLEIC ACID ANALYSIS
212 2.0->
0.0
Figure 11.9. Age distribution of exponentially growing populations (after Steel, 1968).
In order to apply age distribution theory to the analysis of DNA histograms we must compute the relative durations of the three intermitotic phase times (Gl, S and G2 + M), compute the growth fraction as some proportion between zero and unity and assume that the rate of DNA synthesis is constant. We must also remember that there is a spread in the relative phase durations which have to be assumed to have some probability function, e.g. a normal distribution, which additionally requires the standard deviations of the phase times, atG1 (j tS and 0"tG2 + M/ to be considered. Thus far we have defined seven variables which may have to be computed and if there is any suspicion that the DNA synthesis rate is not constant a minimum of two further variables would have to be added to the computation. Some of the 'kinetic' variables which relate to population growth have now been considered but there are also a number of 'static' variables relating to the DNA histogram. These include the positions of the Gl and G2 + M peaks, their standard deviations and the G2 + M: Gl ratio. A total of 14 variables have now been defined which may have to be considered in the computational procedure and its is clear that the type of data set shown in figure 11.8 is far too simple to be able to support a model with this number of variables. The time taken for this type of computation can become prohibitive without materially altering the results obtained; all that happens is that the uncertainty in the values of the computed parameters increases. Age distribution theory as outlined above should only be used for data sets where there is likely to be a steady state of exponential growth and where the rate of DNA synthesis is constant. These conditions are frequently approximated to in tissue culture when the population is not perturbed by therapeutic intervention. However, in the real world of in vivo tumours, including
DNA HISTOGRAM ANALYSIS
213
human, and therapeutically perturbed populations the age distribution is distorted and can no longer be modelled by a continuous mathematical funtion. Because of these problems some simpler approaches have been adopted to model the S-phase interval of the histogram. 11.4.2 Rectilinear integration This term is a somewhat grandiose description for finding the area, in this context, of a four-sided polygon with straight edges. It would seem that when you have a sophisticated instrument you have to have 'flashy' terms to describe some very simple operations. Consider figure 11.10 which shows two hypothetical DNA histograms. In panel A the S-phase section of the histogram has a horizontal upper border. The height of this above the base-line can be found and multiplied by the distance between the G2 + M and Gl mean channels to give an area approximately proportional to the fraction in S-phase. In practice the height would be calculated as the average of the number of channels between points a and p. This procedure extrapolates the upper border of the S-phase interval of the histogram, dashed lines, to the mean channels of G l and G2 + M and gives the S-phase proportion.
Figure 11.10. Rectilinear integration. Panel A depicts an horizontal top to the S-phase component and panel B depicts an inclined top.
214
NUCLEIC ACID ANALYSIS
In panel B the upper border of the S-phase interval is not horizontal but it is still straight. Thus, if points oc and P are equidistant from the G l and G2 + M mean channels respectively we can still compute the average and multiply this by the distance between the means to give the area of the polygon which is equivalent to the S-phase proportion. This method was introduced by Baisch et al. (1975) and is quite adequate for data sets which approximate to the shapes of the histograms shown in figure 11.10. However, the procedure tends to fall apart when the coefficient of variation of the G l peak is greater than about 5% and where the upper border of the S-phase interval is not flat.
11.4.3 Multiple Gaussian This method of analysis has been used by Fried (1976,1977) and by Fried and Mandel (1979). The S-phase interval is modelled with a series of closely spaced Gaussian distributions with constant coefficient of variation which are appropriately summed. The principles of the analysis can be appreciated by considering the idealized DNA histogram of figure 11.7. If the numbers of cells in all channels of this histogram are 'spread' according to Gaussian distributions we obtain the result shown in figure 11.11. The coefficient of variation is assumed to be constant hence the standard deviation of the distributions increases with channel number. We can see in figure 11.11 that the Gl and G2 + M peaks are fitted by single distributions and the S-phase interval is composed of a number of overlapping distributions which are summed to give the total S-phase distribution. The mean and standard deviation of the G l and G2 + M peaks are estimated from the experimental data
0)
O
S phase compartments 10 -
5 -
10
20
30
40
50
60
Fluorescence intensity (channel no.)
Figure 11.11. Multiple Gaussian analysis (Fried, 1976).
DNA HISTOGRAM ANALYSIS
215
and these are used as 'starting points' to generate the theoretical distribution which is then compared with the experimental data. The various parameters are varied until a satisfactory fit is obtained.
11.4.4 Polynomial A number of different shapes can be generated with polynomial curves and the equation has the form, Y=ao + 01xX1+0 2xX2 + . . . . +
anxXn
where n is the order of the polynomial. Dean and Jett (1974) introduced this method and figure 11.12 is reproduced from their original paper. The lower panel 105
G1
G2 + M
10"
4>
.o E
30
40
50
60
Channel number
o «-
15
E Z
20
30
40
50
60
70
Channel number
Figure 11.12. Polynomial analysis (Dean and Jett, 1974).
216
NUCLEIC ACID ANALYSIS
shows the experimental DNA histogram as the points and the upper panel, which is directly comparable with figure 11.7, shows the 'ideal7 histogram in which there is no dispersion in the data. In the polynomial analysis the Gl and G2 + M peaks are fitted with Gaussian distributions and the upper border of the S-phase interval, between the Gl and G2 + M channels in the upper panel, is fitted by a polynomial. The technique involves estimating the Gl and G2 + M modal channels with their standard deviations plus approximate numbers of cells in the Gl and G2 + M peaks. This, so far, adds up to a total of six parameters all of which can be estimated, to a first approximation, from the experimental data. A second-degree polynomial now requires a further three coefficients making a total of nine parameters which are varied until the model fits the experimental data. The curves in the lower panel were generated by the model and the predicted S-phase distribution, computed from the polynomial after 'spreading' with constant coefficient of variation, is represented by the dashed curve.
11.4.5 Single Gaussian A very simple system of analysis has been developed in our department which only relies on the assumption that the data are normally distributed and is a simplification of the multiple Gaussian technique. The Gl/S and the S/G2 + M interfaces are modelled by a probability function derived from fitting Gaussian curves to the Gl and G2 + M peaks within the region where there is minimal overlap with the S-phase segment of the histogram (Watson, Chambers and Smith, 1987; Ormerod, Payne and Watson, 1987). In the perfect data set depicted in figure 11.7 all Gl cells would be scored in a single channel. Thus, the probability of finding an S-phase cell in the single Gl channel would be zero and the probability of finding an S-phase cell in channel G l + 1 would be unity. Therefore, the probability of finding an S-phase cell at the Gl/S boundary would be 0.5. In real data sets which are distributed the probability of finding an S-phase cell at the Gl/S boundary is also 0.5, and the boundary must be distributed about the Gl mean channel. The probability function to describe this distribution of the Gl/S boundary about the Gl mean channel is modelled as the cumulative frequency curve of the Gaussian which is fitted to the Gl peak. This is illustrated in figure 11.13 which for simplicity shows only the Gl/S interface. The thick curve bounds the whole data set and the dashed curve to the right of the Gl mean represents the Gl component after subtraction of the S distribution. The dot-dashed curve is the cumulative frequency of the Gl distribution which is arbitrarily scaled to the unit peak height of the Gl component. This cumulative frequency curve is calculated from the standard deviation of the Gl peak and represents the probability boundary between the Gl and S components with a value of 0.5 occurring at the Gl mean. At 3 x crG1 above the mean where c G 1 is the standard deviation of the Gl peak the cumulative Gl frequency is unity and the respective probabilities of finding a Gl and S-phase cell are zero and unity. Thus, if we know the frequency of the S distribution at the Gl mean we can
DNA HISTOGRAM ANALYSIS
217
Figure 11.13. Gl/S region of a DNA histogram where the maximum frequency of the G l component is scaled to unity. The thick uninterrupted curve bounds the whole data set. The dotted curve, mainly to the right of the Gl mean is the Gl component (Gaussian distributed) and the dot-dashed curve is the cumulative frequency of Gl, also scaled to unity. The dashed line with negative slope extrapolates the S-phase envelope above G l mean+ 3 x SD to the G l mean channel and cuts the latter at frequency S. The constant kGl is the number of G l standard deviation units measured from the G l mean channel associated with a cumulative frequency of jS.
218
NUCLEIC ACID ANALYSIS
calculate the probability within the whole distribution of rinding an S-phase cell at the Gl mean from the cumulative frequency distribution of the Gl compartment. An approximation for this S frequency can be obtained by extrapolating the upper border of the S-phase distribution above Gl mean + (3 x (jG1) to the value shown as S at the Gl mean using regression analysis. This is shown in figure 11.13 as the dashed straight line with negative slope. We can now find the point on the cumulative frequency curve associated with a value of jS, which is the point at which the probability of finding an S-phase cell is 50%. The number of standard deviation units, kGl, associated with this point can now be calculated which adjusts the position of the Gl/S interface within the histogram so that the chance of finding an S-phase cell at the Gl mean will be 50%. The probability distribution for S-phase, Ps, is such that when the frequency in channel x of the data set is multiplied by its corresponding value of PS(J) we obtain the number of S-phase cells in that channel. The form of this distribution is given by, Ps(z)=
erf(Gl(j)-/cGl)-
erf(G2(x) + kG2)
where erf(Z) is a numerical integration routine for the error function which computes the area under the normal curve from — GO to Z, where Z = (x — £)/SD (Gautschi, 1964). In the equation shown above, ) = (channel(x) —Gl mean)/(7 G1 and G2{x) = (channel(x) — G2 mean)/<7G2 where GQI and crG2 are the standard deviations of the Gl and G2 + M distributions respectively. The constant fcG2 in the S-phase probability function, Ps(x), serves the same function at the S/G2 + M interface as fcGl at the Gl/S interface. A pictorial representation of the probability function is shown in figure 11.14. In the report by Baisch et al. (1982) a number of synthetic data sets with known proportions, in Gl, S and G2 + M were analysed blind by all groups involved in the study. A selection of eight of these data sets, where there was a well-defined Gl peak but with widely differing proportions in the cell cycle phases, were reanalysed using the method described above and are shown in figure 11.15. Figure 11.16 shows the model predicted proportions in each phase from the analyses in figure 11.15 plotted against the known proportions. The closed and open circles represent Gl and S respectively and the squares represent G2 + M. The line has been drawn with unit slope. The value of £# 2 for the 24 comparisons was 5.19 with 15 degrees of freedom, p< 0.0001 that the deviations of the predicted from the true could have arisen by chance. Although 24 points were included in the Z / 2 calculation there are only 15 degrees of freedom as only two values from each histogram can be assigned arbitrarily. The third is fixed by the other two. The average of the predicted Gl mean values was 138.2 compared with a true value of 138, an error of less than 0.2%. The G2 + M: Gl ratio was 1.993, an error of less
DNA HISTOGRAM ANALYSIS
219
1.0 -|
n CO &
o 0.5
G1 mean
G2 mean
Figure 11.14. S-phase probability distribution. When each channel of this distribution is multiplied by the frequency in the corresponding channel of the experimental data set the S-phase distribution is generated.
Figure 11.15. Illustration of histogram analysis (simulated data). The dots bound the whole of each data set and the curves bound Gl, S and G2 + M. Each abscissa division represents 100 channels and the data sets were scaled individually to the maximum height of each histogram. For display purposes these data have been reduced from 10-bit to 8-bit resolution.
NUCLEIC ACID ANALYSIS
220
60 , f oo
O) (Q C 0)
o
40
5
•o 0)
I 20
20 True
40
60
Percentage
Figure 11.16. Model predicted percentages plotted against known percentages for the data analysed in figure 11.15. Solid symbols ( # ) , open symbols (O) and squares ( • ) represent Gl, S and G2 + M respectively.
than 0.36%. The mean coefficients of variation of the Gl and G2 + M peaks were 5.68% and 6.18% respectively compared with a true value of 5.75% for both. The technique has now been used for the analysis of well over 10 000 histograms within our unit (I've stopped counting how many) and in practice the strength of the method has been found to be the ability of the algorithms to cope with therapeutically perturbed data. It was originally tested with five different human cell lines, HT29 (colon adenocarcinoma), MRC5 (fibroblast line; normal donor), AT5BI (fibroblast line from a patient with ataxia teliangectasia) and SV40 transformed variants (MRC5CVI and AT5BIVA) of the latter cell types. Suspensions were prepared at a concentration of 5 x 106 cells ml"* in full growth medium and the cells were stained with triton X-100/ethidium bromide (Taylor, 1980). In this initial evaluation of over 350 DNA histograms from the five different cell lines in both control and drug or radiation perturbed populations the G2 + M.-G1 ratio was 2.009 with 95% confidence limits of 0.015. This overall mean value does not differ significantly from the expected ratio of 2.0, p>0.05. There was somewhat greater variability in the subgroup of drug and radiation perturbed data where the mean was 2.014 with 95% confidence limits of 0.021. The computed proportions in Gl, S and G2 + M varied within the ranges of 10 to 90%, 7 to 90% and 5 to 80% respectively in a multiplicity of combinations. A selection of six histogram analyses are shown in figure 11.17 to illustrate the wide variety of forms that can be analysed by the model. The analyses shown above look reasonable; however, there is no direct evidence that the proportions of cells in the three phases from the experimentally
Figure 11.17. A selection of histograms derived from experimental data. Display directly analogous to figure 11.15.
Ill
NUCLEIC ACID ANALYSIS
derived data are correct. Indeed, direct evidence is almost impossible to obtain as there is no completely independent method of estimating the proportions in Gl and G2 directly, and in perturbed populations the S-phase fraction cannot be estimated reliably. In completely unperturbed populations the 3H-thymidine labelling index gives a good approximation for the proportions in S. But, in perturbed data sets (the majority in our initial evaluation) the labelling index must never be equated with the proportions in S as a cell may have an S-phase DNA content and may not be synthesizing DNA due to the perturbing event. The majority of the experimental data sets exhibited a well-defined Gl peak and the average G2 + M : G l ratio for over 350 analyses was 2.009, very close to the expected value. This is comparable to the result from the simulated data and the range of shapes of the experimental data was very similar to that found in the simulated histograms. We have no reason to suspect that any errors in the analysis of the experimental data were either qualitatively or quantitatively different from those in the simulated histograms and conclude that analysis of the former gives, at least, reasonable results. In order to test the algorithms further a series of experiments was carried out with duplicate flasks and figure 11.18 shows the proportions in Gl, S and G2 + M from the first sample plotted against the comparable values from the second sample. The closed and open circles depict Gl and S, respectively, and the squares represent G2 + M. A total of 75 points is shown in figure 11.18 but the regression line was calculated from a total of 168 points which gave a slope of 0.97 and intercept of 1.04 with 95% confidence limits of 5.2%. The correlation coefficient was 0.962. A 2%2 calculation for the deviation of one measurement from the other was 46 with 111 degrees of freedom, p< 0.0001 that the differences could have arisen by chance. The result in figure 11.18 indicates that the true proportion within a phase will have a 95% chance of being within +5.2% of the computed value and most investigators would accept a 5% biological variability between experiments. The duplicate samples analysed here contain more potential sources of variation than those due to staining, instrumental factors and the analysis procedure. These samples were duplicated from the very start of each experiment, thus additional sources of variation must be considered. These include dilution errors during seeding, growth variation from flask to flask, variations in radiation dose or drug concentration and exposure time (about 70% of these duplicates were perturbed populations), versene artefacts in single-cell suspension preparation, dilution errors in preparing the suspension for staining and possible modulation of the staining by the perturbing treatment under study. When all these factors are taken into consideration it would seem unreasonable to expect reproducibility to be better than + 5% between samples and reruns of the same samples gave results for the proportions within each phase to within +1.5%. We have found this method of analysis to be superior to that based on age distribution theory published previously (Watson, 1977a). The model is considerably more robust and it can cope quite adequately with populations where there is a varying rate of increase in DNA during S-phase, as well as with perturbed data sets.
CELL CYCLE KINETICS
223
6O-1 0) (0
2 40 Q. ©
a
E CO
s 20-
0
20 2nd sample
40
60
Percentage
Figure 11.18. Analysis of duplicate samples. Symbolic representation as for figure 11.16. Data from only 25 analyses (75 points) shown although the regression was calculated from 56 data sets (168 points). The slope and intercept were 0.97 and 1.04 respectively with a correlation coefficient of 0.962.
11.4.6 TCW analysis TCW stands for Trace, Cut and Weigh and can be tried in emergencies when all else fails. It is not seriously recommended and it only works with fairly standard looking data sets. It depends on the human mind's exceptionally good analogue processing, pattern recognition and discriminatory capacity. The histogram is covered by high quality tracing paper and the sections of the histogram estimated to correspond to the Gl, S and G2 + M areas as in figure 11.8 are cut out with a scalpel and weighed on a chemical balance. The weights are then proportional to the proportions in the three cell cycle phases. I have used this method in the past and took the trouble to calibrate the tracing paper where different known areas were weighed to produce a linear calibration. The results for the phase proportions were within + 3% of those obtained by computer model where I was able to compare the two.
11.5
Cell cycle kinetics
The type of histogram data and its analysis discussed in sections 11.3 and 11.4 can only yield the proportions of cells in the various cell cycle phases and the relative durations of the phases. This is not kinetic information even though some publications might lead one to believe that it is. Kinetic information can only be obtained when a perturbing event or second marker is introduced into the steady state where the effects thereof are followed temporally. Analysis of the decay of the introduced event with time yields the kinetic information. There are two basic
224
NUCLEIC ACID ANALYSIS
types of perturbed DNA histogram. The first is due to an alteration in the steadystate age distribution with partial synchrony of the population. The second is more subtle in which a specific marker for S-phase is introduced without altering the steady-state age distribution of the population. 11.5.1 Stathmokinetic techniques An alteration of the steady state of growth may be induced by addition of drugs or radiation which block or delay the population in a specific phase of the cell cycle. Addition of colcemid, which depolymerizes tubulin in microtubules, induces metaphase arrest as cells cannot proceed to anaphase. Figure 11.19 shows DNA histograms of a human breast cancer cell line before (panel A) and after (panel B) treatment with colcemid where the accumulation of cells in G2 + M is obvious. Rasoxane (ICRF 159) is another drug which arrests cells with a G2 + M DNA content and the data shown in figure 11.20 were obtained from a mouse tumour cell line blocked at time zero. The population was sampled at intervals and a progressive shift to the right is noted. A sequential series of data sets such as these can be analysed to give the absolute cell cycle time, the phase durations and their standard deviations (see section 11.5.3). One major objection of the 'stathmokinetic' approach outlined above is that the perturbing event may alter the behaviour of the population in ways other than those that are expected and are being observed. It was during such a series of experiments with stimulated B-cells using colcemid to block cells in G2 that we discovered that this also causes a block in early Gl (Kenter et al., 1986, and see section 11.7.1).
2n
4n
2n
4n
B
Figure 11.19. DNA histograms before (A) and after (B) treatment with colcemid showing accumulation of cells with Gl + M DNA content.
CELL CYCLE KINETICS
225
4n Figure 11.20. Rasoxane (ICRF 159) treated mouse tumour cells showing a progressive increase with time (hours, shown on each panel) in cells arrested with a G2 + M DNA content.
11.5.2 Mitotic selection A second approach, which goes some way to overcoming the objections raised above involves mitotic selection (Teresima and Tolmach, 1963). Cells growing in monolayer cultures are usually fairly firmly attached to the substratum of the containing vessel and are spread over a relatively large area. However, at mitosis the cells become spherical and a relatively small area of the cell wall is in contact with the plastic or glass and the mitotic cells can be selectively detached by gently shaking the flask. The culture medium, containing detached mitotic cells, is poured off, the cells are concentrated by centrifugation and reseeded into a number of fresh flasks. Within a few minutes the cells have completed division and they
226
NUCLEIC ACID ANALYSIS POST SYNCHRONISATION PROGRESSION of EMT6/M/CC CELLS
16
Id U CO
cr
LJ CD
60
30
DNA FLUORESCENCE INTENSITY
Figure 11.21. Mitotic selection synchrony experiment showing a clear progression of cells through two cell cycles after reseeding. The continuous curves bounding the whole of each distribution and the dashed curves bounding the S-phase components were predicted by computer model.
CELL CYCLE KINETICS
111
stick down to the surface as Gl cells immediately post mitosis. At intervals thereafter a flask of cells is stained for DNA content. The results of one such experiment are shown in figure 11.21. At 2 hours after selection there was a clean G l peak. By 4 hours a small proportion of cells have increased their DNA content as they began synthesizing DNA in S-phase. Thereafter, there was a progressive shift to the right and with time a 'wave' traversed the S-phase segment of the histogram. At 12 hours some cells had progressed through the cycle and had divided to reappear with a Gl DNA content. There was then a second 'wave' as cells again moved into synthesis to be followed by a second division. These data were analysed by computer model (Watson and Taylor, 1977) to give a cell cycle time of 13.3 hours. The intermitotic phase times were 4.8, 7.2 and 1.3 hours respectively for Gl, S and G2 + M. The 3H-thymidine labelling index was also determined at each time point and these data were compared with the computed fraction in S-phase shown in figure 11.22. There was generally good agreement between the computed curve and experimentally determined labelling index apart from a discrepancy at the first peak where the labelling index is probably underestimated. Computer modelling of such data sets will be dealt with in the next section.
10-1
a ) 0 5 c
5
10
15 20 Hours post synchronisation
25
Figure 11.22. Tritiated thymidine labelling index (points) compared with proportion in S-phase predicted by computer model analysis (curve) of the data shown in figure 11.21.
228
NUCLEIC ACID ANALYSIS
11.5.3 Modelling population kinetics Two classes of problem arise when modelling flow cytometric population kinetics. The first pertains to the dynamic processes which have to be described in the form of time-dependent mathematical functions. These functions are designed to elucidate how the proportions of cells within the three subphases definable by flow cytometry, namely Gl, S and G2 -f M, vary with time. The second class of problem pertains to how the proportions in the cell cycle phases calculated by the mathematical functions describing the dynamics are expressed as a DNA histogram. Some of the processes involved under the second class have already been covered in section 11.4.5 where the proportions in Gl and G2 + M are modelled with Gaussian distributions. However, a different type of system to that described in section 11.4.5 has to be used to model the S-phase component which will be discussed after considering the dynamics. Many of the mathematical models used in flow cytometry to describe population dynamics take their origin from work carried out in the mid to late 1960s to model percent labelled mitoses curves (Takahashi, 1966,1968; Takahashi, Hogg and Mendelsohn, 1971; Hartmann and Pederson, 1970). Those that can readily be adapted for use in flow cytometry fall into two basic categories. The Takahashi-Hogg-Mendelsohn model divided the cell cycle up into a number of arbitrary compartments each of which represented a time domain. For example, if the cell cycle time was 10 hours and this was divided into 20 equal compartments then each of the latter would be of 0.5 hours duration. If we assume that the durations of Gl, S and G2 + M were 4, 5 and 1 hour respectively then 8, 10 and 2 arbitrary compartments would be assigned to Gl, S and G2 + M respectively. This is depicted in the top panel of figure 11.23 which is an exponential age distribution where the S-phase cells are cross hatched and the G2 + M cells are stippled. At a time t later, where t = ±tG1, the whole population will have moved four compartments (half of Gl), or time domains, to the right. This is shown in the bottom panel of figure 11.23 where the cells which originally were in G2 + M have divided and progressed through the cell cycle to occupy time domains 3 and 4 in Gl. Cells which originally were in the last two time domains of S-phase, i.e. late S cells, have progressed through G2 + M and now occupy the first two compartments of Gl. The remainder of the original S-phase cells now reside in the time domains of mid to late S and G2 + M and half the Gl cells have progressed into S-phase. The data obtained for percent labelled mitoses curves consist of the fractions of mitotic cells which are autoradiographically labelled with silver grains at known times after flash labelling with 3H-thymidine. In the top panel of figure 11.23 the percentage of labelled mitoses would be zero, however, in the bottom panel 100% of mitoses would be labelled as the whole of the G2 + M compartment is now occupied by cells which were in S-phase when the 3H-thymidine was introduced into the system. A typical PLM curve is shown in figure 11.24 where the approximate durations of Gl and S are indicated and the damping is due to
CELL CYCLE KINETICS 2.0
229
G2+ M
1.0-
2.0 ->
1.0
Figure 11.23. Exponential age distribution with 20 equal time compartments each of 0.5 hours duration, top panel. The bottom panel depicts the progression of cells through four time domains to the right, half the duration of tG1.
variability in the phase time durations. In order to analyse these types of data we have to assume that some type of mathematical function(s) can simulate these processes and these must be able to describe not only the phase durations, but also the dispersion in those durations. Various investigators have used log-normal distributions, gamma functions, Poisson and normal distributions to obtain an approximation to the mean phase durations and their variances. In general it doesn't seem to matter very much which distribution is used in PLM analysis, they all give very similar results for the phase times. Joe Gray (1976) at the Lawrence Livermore Laboratories has adapted the Takahashi-Hogg-Mendelsohn model for flow cytometric analysis of sequential DNA histograms assuming Gaussian distributions for the phase times which gives
NUCLEIC ACID ANALYSIS
230
O
o •D
1 50H
0) 0.
10
20
30
Time, hours Figure 11.24. Typical percent labelled mitosis curve which is damped due to variation in the phase times. The points represent the experimental data and the curve was computer model fitted. The durations of Gl and S are indicated, and the duration of G2 + M is from time zero to the time at which the first 'wave' reaches its half-maximum height.
the mean durations with their standard deviation. The transit of cells from one compartment to the next is described by a series of sequential differential equations, one for each compartment interface. This is a very robust model and perturbed populations can be readily analysed by simulating the experimental conditions within the model. For example, if the population had been treated with an agent which kills all cells in S-phase (e.g. hydroxyurea) the starting conditions of the model would be adjusted to include the absence of cells (sounds a bit Irish7 or 'Newfie') in the S-phase domains of the age distribution diagram shown in the top panel of figure 11.23. After mitotic selection all cells would be assumed to occupy the first time domain of Gl but, where cells had been treated with a G2 + M arresting agent (colcemid and rasoxane) the age distribution would commence as shown in the top panel of figure 11.23 but in the mathematics no cells would be 'allowed' to progress beyond the last time domain of G2 + M. Gray's model also contains the added sophistication that the rate of traverse through S-phase need not be constant hence variable DNA synthesis rates can be accommodated. However, this method does have a practical disadvantage, which stems from a restraint in the original concept (Takahashi, 1966, 1968), in that the phase time coefficients of variation (CV) can only be varied in discrete steps. The step size is inversely proportional to the number of arbitrary subcompartments that a particular phase is divided into. Thus, in figure 11.23 the minimum effective standard deviation for G2 + M would be 0.5 hours and as this phase has a duration of 1.0 hour in the diagram the minimum CV would be 50%. In order to obtain smaller CVs the number of subdivisions has to be increased which increases the size of the
CELL CYCLE KINETICS
231
differential equation matrix and consequently increases the computing time. Although Gray used the fast 'predictor—corrector' method of Hamming (1973) to solve the differential equation matrix the computing power needed for 'small' CVs must be considerable particularly for data sets containing a large number of DNA histograms. The second approach to modelling PLM curves which can readily be adapted for flow cytometry is due to Hartmann and Pederson (1970) where a single analytic equation is obtained for each of the three cell cycle phases (Watson and Taylor, 1977). Consider the normal distributions in figure 11.25 where IQI is the mean duration of Gl with a standard deviation of crfG1. Let us assume that cells initially were synchronized at the beginning of Gl which is time zero on the abscissa of the diagram. If we place a piece of card to cover the diagram with the left-hand edge at time zero and progressively move this to the right we will simulate the passage of cells through Gl. All cells will remain in Gl until the lefthand edge of the card hits the left shoulder of the curve which begins at £GI ~~ 3 x (JtGi- As the card is moved further to the right (increasing time) a greater proportion of the area under the curve will be exposed. When the edge of the card
-3CTgi
-2(7gi
~(7gi
Tgi
(Jg
2(Jg
3(Tg
Time — • Figure 11.25. Normal distribution with mean of tGi and standard deviation of
232
NUCLEIC ACID ANALYSIS
hits the point £ = fG1 — 2 x crfG1 approximately 3% of the total area under the curve will have been exposed, top panel. As we move still further to the right half the area will be exposed at t = t G1 , and at t = t G 1 4- crtG1 82% of the area will be exposed, bottom panel. The shaded areas in both panels represent the proportions of the whole population which have completed G l at times tGi — 2 x <7,G1 and tG1 + atG1 respectively. The total area under the normal curve is normalized to unity, thus at t = t G 1 + 3 x atG1 100% of cells will have completed Gl. The 'error function7 erf(Z), which was first encountered in section 11.4.5, computes the area under the normal curve from — GO to Z and in context here Z = (t — tG1)/
lVK 2 +4+(4/)]j
e
where/= I — 1 and erf(x) computes the area under the normal curve from — GO to x. The equation complex listed above describes the kinetics within the population and we now have to translate the proportions in the cell cycle phases into a DNA
CELL CYCLE KINETICS
233
histogram. The proportions in Gl and G2 + M are modelled as normal distributions and the S-phase fraction is generated as follows. If we assume the rate of DNA synthesis is constant, or nearly constant, then the mean rate at which cells traverse the S-phase interval of the DNA histogram is given by (M—l)/t s channels per unit time where M i s the mean channel of the Gl peak. The 'effective mean channel', EMS of the S-phase distribution is given by,
EMStf) = M+ l^Y^Y-
I*GI +tfcx /)]
where / = / — 1 and I varies from K through N cycles. It can be seen that EMS(l) = M for t = tGi at which point half the Gl cells will have entered S-phase. This gives the position of the distribution and the shape is computed with a channel variance of S(i)2 where, S(I)2 = \ —~i
[fftGi
2
+ tfrs2 + (<7fc2x/)]
This accounts for the spreads in the Gl and S intermitotic phase times and only that portion of the S distribution lying within the interval M+l and 2M— 1 channels inclusive represents cells in S irrespective of the values of EMS(i) and S(i). The distribution so obtained is now 'spread' on a channel-by-channel basis to account for the increasing fluorescence standard deviation due to the constant CV and the final distribution is generated with the appropriate summation. The data shown in figure 11.21 were simulated with the model as follows. Initial estimates for the cycle time and the relative phase durations were obtained by inspection of the data and by analysis of an exponentially growing control population. The cell cycle time was obviously between 12.5 and 14.5 hours and the relative phase durations were estimated to be between 0.3 x tc and 0.4 x tc, 0.5 x tc and 0.6 x tc and between 0.05 x tc and 0.15 x tc for Gl, S and G2 + M respectively. The two-hour point was analysed to give a Gl mean fluorescence channel of 30 with standard deviation of 2.5 channels. The coefficients of variation of the phase durations were guessed as being between 10% and 30%. Thus, there were six parameters, namely tc/ tG1, tS/ 0"*GI> ^ts a n d GtG2 which had to be varied within the ranges of the estimates above; tG2 did not have to be varied as this value is fixed by the durations of tc, tG1 and t$. Likewise atc does not have to be varied as this is a function of crtG1, ot$ and crrG2. The parameters were varied iteratively and for every combination the computer predicted distributions were compared with the experimental data. The curves in figure 11.21 were generated with the combination of parameters which give the best fit using the simple sum of deviations as the criterion and the dashed curves within each histogram represent the computed S-phase distribution. 11.5.4 FPI analysis The various equations shown in the previous section may look somewhat 'fearsome' to the uninitiated at first sight; however, they are not really very difficult to understand and with a little perseverence most people can appreciate them.
234
NUCLEIC ACID ANALYSIS
TimeFigure 11.26. Longitudinal representation of the cell cycle.
Unfortunately, the majority of commercial computer packages do not contain programs which can analyse a time sequence of histograms as shown in figure 11.21. There is, however, one very elegant and simple analysis procedure by Zeitz and Nicolini (1978) which can be carried out with only a piece of graph paper and a pocket calculator. Because of its simplicity it is readily available to all users and hence deserves particular attention. Let us consider again what is happening to the biology in the data set shown in figure 11.21. A well synchronized Gl population is progressing through Gl, then doubling its DNA content during S and dividing at the end of the G2 + M phase. This is represented longitudinally in time in figure 11.26. We can arbitarily consider a particular DNA level between Gl and G2 + M and at any time point there will be a flux into a flux out of this 'compartment'. For simplicity let us consider mid S-phase (3ft) in figure 11.21. The input and output fluxes at this DNA level will both be zero until some of the Gl synchronized cells have increased their DNA sufficiently to be scored with 3ft DNA content. The input flux will rise faster than the output flux until half the population has passed through this DNA level. Thereafter, the output flux will exceed the input. Thus, the fraction of the whole population with this DNA level will rise then fall as the synchronized cohort of cells passes through this compartment. A second rise then fall will occur during the second cycle after division has taken place. There will, however, be some damping of the amplitude of the wave due to desynchronization. The frequency, or periodicity, of the wave through this compartment will be that of the cell cycle time. In practice one should not consider a single channel of the DNA histogram (DNA level) but one or two either side of the arbitrarily fixed level to allow for statistical fluctuations in the data. Once the limits have been chosen the calculation merely involves dividing the number of cells within the limits by the total number of cells in the population. Figure 11.27 shows the Fraction of the whole Population In the selected phase, mid-S-phase (hence the term FPI) from
CELL CYCLE KINETICS
235
Figure 11.27. Fraction of the whole population in a small time domain in mid S-phase. The periodicity of the curve is that of the cell cycle. figure 11.21 plotted against time. The cell cycle time was approximately 13.0 hours compared with 13.3 hours from the mathematical model. By selecting different DNA levels, i.e. FPI in Gl or G2 + M, it is possible to obtain estimates of the intermitotic times which were 5.0, 7.0 and 1.0 hours for Gl, S and G2 + M respectively, very close to the computer model results.
11.5.5
Br omodeoxy uridine
Bromodeoxyuridine (BrdU) is a thymine analogue which is incorporated into DNA during synthesis and two methods involving BrdU uptake are available for studying kinetic changes where the steady state of growth remains unperturbed. The fluorescence from the bisbenzimidazole dyes (e.g. Hoechst 33558 and 33342) is quenched by the presence of BrdU in DNA as shown by Latt (1977) and figure 11.28 is redrawn from that publication. Mixtures of the polynucleotides poly(dA.BrdU) and poly(dA.dT) where the molar proportion of the former was varied from 0 to 1 were assayed fluorimetrically after addition of Hoechst 33258 and ethidium bromide. With an increasing fraction of poly(dA.BrdU) there was a progressive decrease in Hoechst 33258 fluorescence reaching a limit at about 15% of that of the poly(dA.dA) control. This decrease in Hoechst fluorescence with increasing poly(dA.BrdU) concentration was accompanied by a very small increase in ethidium bromide fluorescence. Following this observation Latt, George and Gray (1977) were able to show that CHO cells incubated with BrdU for 24 hours and stained with Hoechst 33258 could be distinguished from similarly stained control cells not treated with BrdU. These data are reproduced in figure 11.29 which shows the fluorescence profiles of the BrdU treated and untreated cells together with a 1:4 mixture of the two. Both Bohmer (1979) and Beck (1981) have used BrdU quenching of Hoechst 33258
NUCLEIC ACID ANALYSIS
236
1-0
Mole fraction Poly(dABrdU) 60
CM
(00.50
0.0
0.25 u c
0.25 0.5 0.75 Mole(dABrdU)
40
(0
1.0
2
o 3
20 V
N.
400
450
500 550 Wavelength, nm
600
Figure 11.28. Quenching of Hoechst 33258 fluorescence by increasing molar ratios of poly(dA.BrdU). Ethidium bromide was also included in the sample and there was a slight increase in EB fluorescence with increasing proportion of poly(dA.BrdU). The inset shows the ratio of fluorescence at 462 nm (Hoechst) to that at 5 77 nm (EB) versus poly(dA.BrdU) concentration which represents poly(dA.BrdU) content. Redrawn from Latt (1977).
CO
24 hrs of BrdU incorporation
O 3
Control
X 2
5 o
O 100
200
100
"o3
1:4 mixture of BrdU - substituted and control cells
= 1 0
O
0
200
100
200
Figure 11.29. Quenching of Hoechst 33258 fluorescence in tissue culture cells. Top left, cells exposed to BrdU for 24 hours and, top right, control cells. The bottom panel shows a 1:4 mixture of BrdU treated and untreated cells.
CELL CYCLE KINETICS
237
(0
o
Ho-33342 fluorescence
Ho-33342 fluorescence
Figure 11.30. Flash labelling of tissue culture cells with BrdU for 2 hours where panels A and B show the control and treated cells respectively. Some quenching of Hoechst 33342fluorescencein the S-phase cells can be seen in panel B. The quenching 'moves' these cells to the left and they then tend to overlie each other and some overlapping with Gl cells, which have not incorporated, occurred. fluorescence in cell kinetic studies by following time courses after labelling. However, the method has resolution problems as quenching is directly proportional to the quantity of BrdU incorporated. It can be difficult to obtain sufficient uptake of BrdU in flash labelling experiments to monitor the S-phase fraction independently of Gl and G2 + M as quenched S-phase DNA overlaps the Gl component. This is illustrated in figure 11.30 where 90° light scatter is plotted on the ordinate versus Hoechst 33342 fluorescence on the abscissa as dot-plots for control and BrdU-treated cells (5 |ig ml" 1 BrdU for 2 hours), panels A and B respectively. The fluorescence quenching of the S-phase fraction in the BrdUtreated cells is clearly apparent and many of these would overlap the Gl peak, see panel B. The separation we obtained was not regarded as being sufficient to enable us to use this method for pulse BrdU exposure experiments where the S-phase fraction was to be followed with time. However, this method has been used for continuous labelling experiments. The problems we encountered with BrdU quenching have been overcome by the second method using this analogue which is due to Gratzner et al. (1975) who raised a polyclonal antiserum to the DNA/BrdU complex in rabbits. Some of the original data obtained after BrdU incorporation and immunoperoxidase staining are reproduced in figure 11.31 which shows patchy staining in a nucleus and two chromosomes, one of which exhibits sister chromatid exchange. The first use of this technique in flow cytometry was reported by Gratzner and Leif (1981) where dual parameter data of light scatter signals versus BrdU fluorescence were able to identify the labelled cell fraction after a 60 minute exposure to 10|iM BrdU. Gratzner (1982) produced monoclonal antibodies to both BrdU and IdU as a means of detecting DNA replication and Dolbeare et al (1983) extended this
238
NUCLEIC ACID ANALYSIS
Figure 11.31. Reproductions of some of Gratzner's original immunoperoxidase data (Gratzner et al., 1975) showing incorporation of BrdU into a nucleus and two chromosomes one of which (right) exhibits sister chromatid exchange.
method to measure total cellular DNA simultaneously with BrdU incorporation. Cells were pulse labelled with the analogue, treated with a nuclear isolation buffer and fixed then subjected to an hydrolysis step to denature double-stranded DNA to single stands as the anti-BrdU antibody only recognizes BrdU in single stands. The nuclei were then incubated with the antibody which was subsequently tagged with fluorescein (green) and total DNA was stained with propidium iodide (red). The redrawn data from Dolbeare et al. (1983) are shown in figure 11.32 where the BrdU associated fluorescence (green) is plotted on the ordinate versus DNA fluorescence (red) on the abscissa as a contour map where panels A and B respectively show the control and the BrdU incorporation data after flash labelling. The 'horse-shoe' pattern in panel B is characteristic with Gl and G2 + M cells showing no BrdU associated fluorescence and the S-phase cells exhibiting differing degrees of incorporation which are related to the rates of uptake at different stages of DNA synthesis. Dean et al. (1984) have shown how the rate of DNA synthesis during S-phase can be calculated from data such as those in figure 11.32. Similar data sets are shown in figure 11.33 where an in vivo mouse tumor was analysed both before and after hyperbaric oxygen treatment (Wilson et al., 1985). In both panels there is a component with S-phase DNA content which has not been stained by the anti-DNA/BrdU antibody indicating that some cells with an Sphase DNA content are not synthesizing DNA. However, after hyperbaric oxygen this component is decreased, suggesting that some tumour cells are nutrient limited. A time course experiment using this technique in a mouse tumour is shown in figure 11.34 (Begg et al., 1985). Immediately after the BrdU pulse the data are qualitatively similar to those in figures 11.32 and 11.33. However, with
CELL CYCLE KINETICS
239
o o •o
DNA content
DNA content
Figure 11.32. Bivariate analysis of BrdU incorporation (green fluorescein fluorescence) on the ordinate versus total DNA (red propidium iodide fluorescence) on the abscissa for tissue culture cells. Controls in panel A, BrdU incorporation in panel B. Redrawn from Dolbeare et al (1983).
increasing time between BrdU administration and sampling of the population there is movement of the labelled cohort through S-phase then G2 and division to appear in the G l region of the two-dimensional map with a halving of their green fluorescence intensity. It can also be seen that cells with a Gl DNA content at the time BrdU was administered track through the S-phase domain with no green fluorescence. It is obvious from the data shown in figure 11.34 that we can now track the behaviour of the two different subsets with time, namely cells which were synthesizing DNA when BrdU was administered and those that were not. Calculation of the proportions in each cell cycle phase can now be carried out and these data can be used to estimate the cell cycle time and intermitotic phase times as described in section 11.5.3. The BrdU—antibody technique is potentially of very great importance in cell biology proliferation regulation studies as will be shown in section 12.3. However, it can be a little tricky and a considerable amount of work on the stoichiometry and sensitivity (Dolbeare el al., 1985) and the role of the denaturation step (Moran el al., 1985) has been carried out. Beisker, Dolbeare and Gray (1987) have also improved the immunocytochemical procedures to obtain increased detection sensitivity. This is not a technique which should be undertaken lightly and each cell type should be investigated in pilot studies before embarking on 'full-blow7 experiments. If you are really serious about using this method you should acquire a copy of the November 1985 issue of Cytometry (volume 6) which was entirely devoted to this technique and do some specialized reading. This issue has also been published as a book, edited by Gray and Mayall (1985).
240
NUCLEIC ACID ANALYSIS i
100
IN VIVO 80-
60
-
40
20-
1 -Li
1
1
i
20
r1—i
1
40
1
60
1
1
80
1
1 100
DNA
100-j
HYPERBARIC
80-
60•o 40
-
20-
20
40
60
80
100
DNA Figure 11.33. An in vivo tumour showing BrdU incorporation after flash labelling, top panel, and following hyperbaric oxygen treatment, bottom panel. Both data sets show some cells with S-phase DNA content which have not incorporated BrdU. However, this component is reduced in the tumour treated with hyperbaric oxygen suggesting that these S-phase cells are nutrient limited. Redrawn from Wilson et al, 1985.
CELL CYCLE KINETICS Oh
241
2h
4h
6h
•o CQ
DNA
DNA
DNA
DNA
Figure 11.34. BrdU pulse-chase experiment where the in vivo tumour was followed at 2-hourly intervals up to 6 hours. Redrawn from Begg et ah, 1985.
11.5.6 Biotinolated nucleotides The use of biotinolated nucleotides is similar in principle to the BrdU technique except that the biotinolated precursor is secondarily probed with labelled streptavidin (see section 73.3). This method has been used by Blow and Watson (1987a,b) to study in vitro DNA replication of Xenopus sperm nuclei in the
Figure 11.35. Panels A and B respectively show photomicrographs of DNA and biotin associated fluorescence. Nuclei show different degrees of biotin incorporation in panel B. There is also some variation in DNA staining intensity in panel A. The flow cytometric data in panel C show that biotin fluorescence (ordinate) is both directly and quantitatively related to total DNA (abscissa). This figure is reproduced by permission of the editor of the EMBO journal.
242
NUCLEIC ACID ANALYSIS
cell-free system described by Blow and Laskey (1986). Nascent DNA was biotin labelled by adding biotinolated 11-dUTP to the egg extract growth medium. The system was then sampled at intervals and total DNA was stained with propidium iodide and fluorescenated streptavidin was used to probe for the newly replicated DNA. An example is shown in figure 11.35 where panels A and B respectively show photomicrographs of DNA and biotin associated fluorescence from the same population as was analysed flow cytofluorimetrically in panel C. The fluorescence microscope data show qualitatively that there are different degrees of biotin incorporation per nucleus and possibly some intensity variation of DNA fluorescence. The flow system data (panel C) show that the two are both directly and quantitatively related. This technique was used to show that nuclei act as independent and integrated units of DNA replication (Blow and Watson, 1987a; Blow et al, 1988).
11.6 Tloidy' I debated for some time the wisdom of including a specific section devoted to this topic, which has probably created more problems than any other single area in flow cytometry. Obviously, I decided to 'have-a-go' and doubtless many others will in the future. The first point to make is that 'ploidy', which is derived from cytogenetics terminology, is a bad term to use in flow cytometry. Euploid means that a cell has the correct number of chromosomes. Aneuploid means that a cell has an incorrect number of chromosomes, and applies if it has too many or too few. In flow cytometry we obtain a measure of the total quantity of DNA and although the number of chromosomes is usually related directly to the DNA content of the nucleus this is not always so. Kraemer et al. (1972) have reported DNA constancy despite variability in chromosome number. It is also possible for a tumour cell, for instance, to have more chromosomes than it should have, and hence it would be classed as aneuploid, but less DNA than expected. The reverse is also possible; however, it is generally accepted that fluorescence intensity is proportional to DNA content (Kerker et al, 1982) but this may not always correlate directly with chromosome number. These considerations prompted Hidderman et al. (1984) to coin the phrase DNA index to describe the quantity of DNA assayed flow cytofluorimetrically where DNA index is the ratio of the Gl peak position of test cells to the Gl peak position of a known diploid standard. Hence if the diploid control Gl peak is recorded in channel 200 and the Gl peak of the test cells is scored in channel 300 the DNA index would be 1.5. Not infrequently one is asked by a clinician to do 'some DNA studies' or even more vaguely 'some flow work7 on this or that type of tumour or tissue. Depressingly, it is often more senior people, but I suppose this is not surprising. The first thing that has to be established is the question that is to be answered. Always say yes but with the very firm qualification that the objectives must be clearly defined. Rule 1, don't start till the questions and objectives have been defined and
TLOIDY'
243
preferably committed to paper. Some (perhaps this should read many) clinicians seem to think that if a 'fancy7 machine is available all they need to do is chop a chunk out, dump it on the bench and somehow, perhaps by magic, a result will appear which is meaningful. This type of attitude is not uncommon and stems from established behaviour patterns. Clinicians will order an investigation, be this a chest X-ray, serum electrolytes or whatever, someone else takes the picture or assays the serum and written reports, usually prepared by yet another person, then appear in the patient's notes. If the results are within normal limits the primary data, i.e. the chest X-ray, may not even be looked at by the requesting clinician. I'm referring here to routine investigations with an established place and sometimes usefulness. Tlow studies', particularly 'ploidy', are tending to be viewed in the same category but these are not yet routine investigations and the value of the majority of assays have yet to be evaluated fully in the routine clinical context. Clinicians, particularly the surgical variety, tend to be 'action-men' (that's how they are trained) and expect a result even if they don't know what to do with it when they get it. After the objectives have been established it is the duty of the scientist in charge of the flow system to alert the prospective user to the potential problems. This applies to all assays but trouble most often seems to arise with 'ploidy' and I'll consider the problem areas under headings of stoichiometry, binding site modulation, standards and logistics. Some of these have been considered elsewhere in the book but I hope it helps to have them all lumped together in one place. 11.6.1 Stoichiometry It must be quite clear from the considerations in section 7.3.7 that measuring 'ploidy' is somewhat more complex than simply chopping out a chunk of tissue and dumping it on the bench. Even if you subsequently manage to produce a perfect single nuclear suspension from the disaggregation a number of variables have to be considered, some of which can be controlled and some of which can not. One variable which is controllable is the dye concentration. If dye is in excess then from figure 7.6 we can see that all the DNA binding sites will be filled and CX will be equal to the initial number of available binding sites in the DNA. I could have done some fancy mathematics here with differential equations to prove this formally, but as it is intuitively self-evident I haven't bothered. 11.6.2 Binding site modulation The most important variable, which may not be controllable, is the initial number of free binding sites in the DNA and the 'free' has been stressed in both figure 7.6 and in section 7.3.7 as this variable can be modulated by many factors. Chromatin and DNA associated proteins may mask binding sites. This applies particularly to acridine orange (Fredericq, 1971), and the techniques using this dye have been developed to remove histones to increase the number of binding sites available (Darzynkiewicz et a\., 1975, 1977a; Traganos et al.f 1977). Chromatin
244
NUCLEIC ACID ANALYSIS
associated proteins may also reduce the accessibility of the phenanthridinium dyes (PI and EB) to DNA (Angerer and Moudrianakis, 1972; Brodie, Giron and Latt, 1975). This can occur not only due to masking but also to conformation changes and by the same token any conformation modulating agents, including DNA binding drugs, may alter dye accessibility or dye binding capacity. The state of chromatin condensation and associated DNA denaturability can make profound differences to the number of accessible binding sites and this has been exploited by Darzynkiewicz el al. {1977b,c) for many years to distinguish between G2 and mitotic cells. In tissues which have been fixed there may be permanent cross linking in DNA and its associated proteins due to the fixation process which cannot be 'unfixed7 and this too can mask potential binding sites. Prolonged formalin exposure, particularly in non-buffered saline, and mercury-containing fixatives can give rise to problems of this nature. The time interval between interruption of the blood supply to the surgical specimen and either fixation or processing can also modify the available binding sites. Cells contain endonucleases and proteolytic enzymes which digest DNA and nucleoproteins respectively. Normally, any intracellular proteolytic enzymes are contained in subcellular compartments but with cell death these enzymes are released and generally 'chewup' the cells from the inside. This inevitably degrades DNA, reduces the number of binding sites and degrades the quality of the data obtained. Hedley et al. (1984) have stressed the importance of adequate fixation of paraffin embedded material. Clearly, if fixation is not adequate there will be tissue degradation both before and during the embedding process. In the latter the temperatures reach above the DNA melting point and if tissue is inadequately fixed there will be temperature dependent DNA degradation. Feichter and Goerttler (1986) have identified inappropriate storage conditions of paraffin embedded biopsies as a cause of artefact. Prolonged (years, not specified) central heating temperatures were sufficient to degrade tissue contained in wax blocks. These authors have also identified tissue damage before fixation as a source of artefact. Biopsies which had been stored frozen at temperatures between — 40 °C and — 60 °C which were thawed, fixed and subsequently embedded gave uninterpretable DNA histograms. 11.6.3 Standards Some method of standardization and specific calibration is needed for every instrument. In more conventional assay systems, e.g. a spectrofluorimeter, it is possible to make up solutions containing known concentrations of the fluorochrome to produce a standard calibration curve. This is also normal practice for spectroscopic techniques using light absorption. The test sample is then compared with the standard calibration curve to determine the concentration and 'quantity' within it. This type of procedure is used in flow cytometry for making pH measurements (see sections 8.4.1 and 14.4) but this is simply not possible with flow cytometric DNA measurements. A 'nuclear-sized' package of DNA containing 'nuclear-quantities' of DNA can only be made by a cell. Try dissolving purified calf thymus DNA in water as I tried some time ago. You end up with a
'PLOIDY'
245
saturated colloidal 'sludge' well before you reach nuclear-like concentrations. Moreover, it is completely impossible to run this sludge through the instrument. However, some help is at hand. Biology has provided a variety of cells with different DNA content and two particularly useful examples are trout and chicken red blood cells which, unlike their mammalian counterpart, retain their nuclei. Vindelov, Christensen and Nissen (1982) and Vindelov et al. (1982) have advocated spiking the test sample with both trout and chicken red blood cells treated in exactly the same way as the test cells. Hence, the peak position of the latter can be determined relative to both internal standards and examples are shown in figure 11.36. Jacobsen (1983) used a combination of trout erythrocytes and human lymphocytes as a standardization procedure and Iversen and Laerum (1987) have used trout and salmon erythrocytes as well as human leukocytes as internal standards for ploidy control. However, it should be noted that DNA fluorescence from the compacted chromatin from lymphocytes can be less than that from cells with less compacted chromatin, which is a dye accessibility problem. These systems are fine for fresh tissue where it can be guaranteed that the test sample and the internal standards have been treated identically. But, it is not always satisfactory for archival material where the fixation and embedding history may not be known, which makes it impossible to treat the standardizing cells identically to the test cells. This problem is only partly resolved with physical standards in the form of microbeads which are now available with different fluorochromes in a range of concentrations which can be used to set up the instrument identically from day to day. 3000
2000 o c
O* 0)
1000
50
100
150
200
Channel No. (DNA)
Figure 11.36. A sample of peripheral blood monocytic cells (MO) 'spiked' with both chicken and trout red blood cells (CRBC and TRBC respectively) which act as internal standards. Redrawn from Vindelov et a\., 1982.
246
NUCLEIC ACID ANALYSIS
Our efforts in this area have been to use a known diploid standard of normal colonic mucosa from a single specimen as well as microbeads to set up the instrument. We originally obtained 30 cm of a single colonic specimen and embedded this in 40 different paraffin blocks and we've used three blocks in four years, so it will keep us going for some time to come. We then rely upon finding normal cells in any aneuploid specimen to calculate the DNA index if this is what is wanted. In my experience it is always possible to find cells with diploid DNA content in an aneuploid tumour even if it means cutting sections from a second or third block. If there is no aneuploid spike in a tumour specimen it is easy to check that it does in fact contain tumour by looking at a 4 |im histological specimen cut adjacent to the thick section used for flow cytometry. Furthermore, it is often possible to distinguish between multiple subsets, including between normal and malignant, on forward and 90° light scatter characteristics (Watson etal., 1987a) even if the DNA content is identical. It has been our practice to score aneuploidy if, and only if, we can see two distinct spikes corresponding to normal diploid and aneuploid components respectively. Using these criteria may mean that some of our studies have tended to underestimate the proportion of aneuploidy in tumour groups. A minority of tumours with a 'shoulder' on the right of the diploid spike, which may have been due to aneuploid components, were scored as diploid but at least we can be sure that those scored as aneuploid were in fact aneuploid. In short, we use presumed normal diploid elements within the tumour as the internal control.
11.6A Logistics When your prospective new user has assimilated this little lot and come back for more you know that he/she is serious. It is now time to establish who is going to prepare and then extract the information from the raw data after the samples have been run through the instrument. Remember that the time taken to 'rail-road' the samples through the instrument is totally insignificant compared with the time for preparation, staining, data extraction and interpretation. In a multi-user system the flow cytometry staff, which seldom number more than two, simply do not have the time to prepare everyone's cells as well as running the samples and keeping the instrument in good running order. If prospective users either cannot, or occasionally will not, provide the necessary support to prepare the samples and extract the information from the raw data you have no option but to refuse to collaborate. People who are serious will understand and find a way of providing the necessary support. Those who do not don't matter, so nothing is lost by refusing.
11.7
RNAandDNA
We have already seen examples of the potential power of multiparameter cell cycle analysis in section 11.5, namely the capacity to distinguish between newly replicated and total DNA using BrdU and biotinolated nucleo-
RNA AND DNA
247
tides. In this section we consider the simultaneous measurement of RNA, DNA and size using acridine orange and Hoechst/pyronin-Y. 11.7.1 Acridine orange A number of staining techniques have been developed to quantitate RNA and DNA simultaneously using the metachromatic property of acridine orange but the pioneering work in this area of flow cytometry has been carried out by Darzynkiewicz and colleagues at the Sloan Kettering in New York. Our group has used the two-step technique of Traganos et al. (1977) for a number of years with only minor modifications and it is worth some space to describe the technique in detail. Unfixed cells suspended in whole medium are initially treated with a solution containing the non-ionic detergent triton X-100 and 0.1 N HC1 in isotonic saline. The triton permeabilizes the external cell membrane which remains stable at the low pH and allows the highly polar dye to enter the cell. The low pH also removes basic histones from chromatin thus making available some dye binding sites which would otherwise be inaccessible. After 60 to 90 seconds the second solution is added. This is a phosphate/citrate buffer containing acridine orange and EDTA. The latter chelates divalent cations which destabilizes double-stranded nucleic acids with RNA being more susceptible than DNA. The final pH is in the range from 4.5 to 4.7 which gives the optimum red/green discrimination. Dissociation of double-stranded RNA to single-stranded species which fluoresce red takes about 5 minutes after which the green and red fluorescence signals remain stable for 20 to 30 minutes depending on cell type. This method depends critically on the selective denaturation of double-stranded RNA as any DNA denaturation will be scored as red fluorescence with concomitant loss of green, and a number of warnings have to be sounded about using this technique. Firstly, some DNA denaturation will occur if cells are over exposed to the first solution containing triton X-100 at pH 1. Secondly, DNA is inherently less stable after histone extraction and denaturation will occur with prolonged exposure to EDTA (divalent cations have been chelated) plus AO in the second step. Every cell type should, therefore, be tested for optimum exposure times in both steps. Thirdly, the DNA phosphate-to-dye molar ratio is fairly critical (Nicolini et al, 1979). For mammalian cells the final cell concentration should be about 10 5 ml" * with the AO concentration between 4 and 5 jigml" 1 . In practice 0.4 ml of solution 1 is added to 0.2 ml of medium containing cells which should be at a concentration of about 106 ml ~ \ Then 1.2 ml of solution 2 are added containing AO at a concentration of 6 jag ml" \ giving final concentrations of about 105 cells and 4 |ig ml~ *. Fourthly, the fluorescence emission spectrum is proton concentration dependent and the final pH should be in the range 4.5-4.7 for the best red/green discrimination. Fifth, the analysing filter combination in the cytometer is critical as the 'green' and 'red' fluorescence emissions do not occupy discrete bands in the spectrum. There is a green DNA 'tail' into the red region and a red RNA 'tail' into the green region. The latter is less critical than the former as DNA is present in much larger quantities than RNA and the contribution of the red RNA tail into the green region is
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Figure 11.37. Acridine orange staining of stimulated T-cells for DNA (ordinate) and RNA (abscissa) simultaneously. Panel A shows the control non-stimulated cells. Stimulated cultures are shown in panel B where cells increase their RNA content between Go and Gl. The latter phase is subdivided into two namely G l A and GlB on an arbitrary RNA level above which cells are seen to enter S-phase. Panel C shows data after treating stimulated cells with vincristine.
100
RNA AND DNA
249
insignificant compared with the magnitude of the green intensity from DNA. The long-wavelength red tail from the DNA emission spectrum could, however, constitute a problem particularly for cells with low RNA levels where the DNA content is many orders of magnitude greater than the RNA content. In this case a significant quantity of the signal in the red photomultiplier could be due to DNA fluorescence. These problems can be largely overcome by the correct optical filtration with the use of a 580 nm dichroic mirror, a band-pass filter from 515 to 560 nm for the green photomultiplier (PMT) and a 630 nm long-pass filter for the red PMT. The latter minimizes the green DNA tail contribution to the red RNA signal, and the magnitude of this effect should be checked by treating a test sample with ribonuclease. In our instrument we have found that only between 10 and 15% of the red signal is due to DNA fluorescence in lymphocytes and EMT6 mouse tumour cells. However, this may be different in different cell types depending on the RNA to DNA ratio and the stability of the DNA. Finally, it seems to be more difficult to perfect this technique with instruments which interrogate cells in the jet as opposed to those that interrogate in the flow chamber and a number of explanations have been proposed. These include stripping of cytoplasm by the shearing forces in the nozzle and disturbance of the electrostatic stacking of dye molecules along single-stranded molecules either by mechanical forces or by induced electrical currents within the nozzle. Darzynkiewicz et al. (1976) have used acridine orange to show that G o thymocytes can be distinguished from Gl after PHA stimulation and these data are reproduced in figure 11.37. Panels A and B show the control unstimulated population and cells stimulated with phytohaemaglutanin (PHA) respectively. The Go 'resting' cells (panel A) increased their RNA content as they progressed into Gl before they entered DNA synthesis. Panel C shows stimulated cells treated with vincristine to block the population in G2 + M and it is apparent that there is emptying of the G l component with the higher RNA levels. It is also clear from these data that a 'critical' RNA level had to be reached before Gl cells could enter S-phase. Data such as these have enabled Darzynkiewicz et al. (1976, 1977a) to discriminate between early and late Gl, termed GlA and GlB respectively, where GlB has been defined as the RNA content of Gl cells above which cells can be observed to enter S-phase. Subsequently Darzynkiewicz et al. (1977b) demonstrated that interphase and metaphase chromatin exhibited different sensitivities to thermal denaturation and on this basis they were able to discriminate between G2 and mitotic cells (Darzynkiewicz et al, 1977c). Fixed cells were treated with ribonuclease to remove RNA then heated at various temperatures to partially denature DNA. Thus, on subsequent staining with acridine orange any single-stranded DNA would fluoresce red. Some of these data are shown in figure 11.38 where green fluorescence (double-stranded DNA) is plotted on the ordinate versus red fluorescence (single-stranded DNA) on the abscissa after heating to 50,85 and 95 °C, panels A, B and C respectively. The discrete cluster which became increasingly separated from the main body of the data with increasing temperature was
NUCLEIC ACID ANALYSIS
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Red fluorescence Figure 11.38. Temperature dependent DNA denaturation in ribonuclease treated fixed cells assayed with acridine orange. With increasing temperature there is increasing DNA denaturation manifest by a decrease in green fluorescence and a concomitant increase in red fluorescence. Mitotic cells exhibited greater thermal denaturability as shown by the cluster which becomes increasingly separated from G l and S-phase cells.
composed of mitotic cells which was confirmed with colcemid treatment. This result was a little surprising as it showed that the condensed chromatin in mitotic cells was more susceptible to thermal denaturation than chromatin in interphase. It was also found that BrdU incorporation into DNA suppressed acridine orange DNA staining (Darzynkiewicz et al, 1978). As this analogue is not incorporated into RNA it was possible to identify cells 'in transit7 from Go to GlA (GlT) on their RNA content where their DNA fluorescence was not suppressed. These data are shown in figure 11.39 with DNA plotted on the ordinate versus RNA on the abscissa where panel A shows G l Q (Go) non-stimulated lymphocytes. In panel B the PHA stimulated cells had been exposed to BrdU for approximately one cell cycle, thus all cells within the division cycle had incorporated the analogue. These cells are included in the dashed polygon and the GlA and GlB compartments clearly have reduced green (DNA) fluorescence compared with non-stimulated cells labelled G l Q . The GlT cells, in transit from G o to GlA, are those with nonsuppressed green fluorescence but with RNA levels comparable with those in GlA. These cells are stimulated as their RNA levels have increased above the G o cells but they had not passed through DNA synthesis as their green fluorescence was not reduced. Studies by Traganos et al (1979) with DMSO induced senescence in Friend leukaemia cells revealed non-cycling cells in S and G2 as well as in Gl and these various studies have enabled Darzynkiewicz et al. (1980) to identify 12 different 'compartments' in the cell cycle. Similar studied have been carried out with EMT6 cells synchronized by mitotic selection (Watson and Chambers, 1978a). The RNA levels increased in Gl before
RNA AND DNA
251
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Figure 11.39. BrdU quenching of acridine orange green fluorescence (DNA) in stimulated lymphocytes where green (DNA) fluorescence is scored on the ordinate with red (RNA) fluorescence on the abscissa. Panel A shows data from the control non stimulated cells (GlQ). Stimulated cells which have encorporated BrdU are enclosed in the dashed polygon in panel B. Cells in transit to G l (GlT) have Gl RNA levels but have not entered S-phase and have not incorporated BrdU hence, their green fluorescence is not quenched.
S-phase commenced. This is a similar finding to that of Darzynkiewicz et al. (1976) in stimulated T-cells. However, during early and mid S-phase the levels remained virtually constant but in late S and G2 there was a further rapid increase in RNA then a decrease in mitosis (Watson and Chambers, 1978a). The latter was confirmed by parallel studies with tritiated uridine uptake (Watson and Chambers, 1978b). Actinomycin-D (ACT-D) is a cytotoxic agent which blocks RNA transcription and the pharmacological dose range in man, assuming an even whole body distribution, is within the range 1 —10 ng ml~ 1 when translated to tissue culture terms. When synchronized EMT cells were treated with ACT-D at 6 ng ml" 1 the RNA level decreased exponentially with a half-time of about 32 hours which is consistent with ribosomal-S RNA degradation. At a lower dose of 1 ng ml" 1 the RNA level remained constant following exposure indicating that the production rate was equal to the rate of degradation. We were very surprised to find that subsequent mitosis was only delayed and not inhibited if ACT-D was added to synchronized cells after mid Gl. Mitosis took place in a proportion of cells even though the RNA level was decreasing at the higher dosage. However, mitosis was inhibited if ACT-D (at either dose) was added just before mitotic selection. This observation suggested that these cells were programmed for subsequent mitosis soon after the last mitosis, and it is possible that this occurs in GlA. Multi-parameter analysis of lipopolysaccharide-stimulated B-lymphocytes using acridine orange to give measurements of RNA and DNA, with both 90° and
252
NUCLEIC ACID ANALYSIS DAY T' COL -VF. CONTROL 11-MAY-£
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F/^wr^ 11.40. Acridine orange staining for RNA (630RF AREA) versus DNA (520RF AREA) in 5 day stimulated spleen B-cells. The top panel shows the control data. The middle and bottom panels respectively show the results of colcemid exposure and its withdrawal.
RNA AND DNA
253
forward light scatter has shown that the post-mitotic, pre-DNA synthesis phase (Gl) can now be subdivided into four distinct subphases namely, Go, Gl', GlA and GIB (Kenter et al, 1986). Figure 11.40 shows three data sets where DNA (520RF AREA) is plotted against RNA (630RF AREA) for day 5 LPS-stimulated B-cells. The data in the top, middle and bottom panels respectively were from control and colcemid-arrested cells and from cells 4.5 hours after colcemid release and each panel shows the characteristic GlA, GlB, S-phase and G2 + M pattern. Our initial interpretation of the data in figure 11.40 was that with colcemid (middle panel) GlA emptied into GlB, the latter emptied into S-phase which subsequently emptied into G2 + M where the population was blocked and that there was a residual non-cycling 'Go' population represented by the cells with lowest RNA content. This interpretation seemed to be substantiated by the data in the bottom panel of figure 11.40 obtained 4.5 hours after colcemid was washed off. There was a relative increase in the proportion of GlA and GlB cells which were presumed to have arisen from a resumption of progression through the cell cycle with division at mitosis refeeding the GlA compartment. This interpretation, however, was not entirely satisfactory as there did not seem to be progression through S and G2 + M. The data were then re-examined as the DNA (520RF AREA) versus 90° light scatter (4'80RS WDTH) data space which is shown in figure 11.41. The left and right columns give perspective 3-D views and conventional contour plots respectively where the top, middle and bottom panels correspond to those in figure 11.40. The control data (top panels) show two peaks in Gl distinguished on their high and low 90° light scatter with small proportions in S and G2 + M. The same overall pattern was seen after colcemid (middle panels) with two exceptions. First, there was the expected accumulation of cells with G2 + M DNA content. Secondly, and unexpectedly, there was an increase in the proportion of cells with G l DNA content which exhibit low 90° scatter signals. After release from colcemid (bottom panels) the proportion of cells in S and G2 + M remained about the same but there was a decrease in the Gl DNA content population with low 90° scatter. The three data sets were gated as shown in the right column of figure 11.41 to give the proportions in G l ' (region 1, defined as Gl DNA content with low 90° scatter) GlA plus GlB (region 2), G2 + M (region 3) and S (region 4). The region 2 data were then analysed in the RNA/DNA data space to obtain the proportions in GlA and GlB and a summary of these data are shown in figure WAI. With colcemid there was a relative increase of cells in G l ' due to emptying of GlA and GlB with progression into S-phase with G2 + M accumulation. After colcemid release the proportions in S and G2-f M remained constant but there was a redistribution within Gl from G l ' to GlA and GlB. Thus, the large 'spikes' in the three panels of figure 11.40 were not Go cells, but G l ' cells plus some in GlA. Furthermore, the three ill-defined but distinct RNA distributions in the top panel of figure 11.40 represent cells in Gl', GlA and GlB respectively. This was confirmed by two further pieces of evidence. Firstly, unstimulated cells die and lyse with a half-time of about 18 hours, and after 5 days in culture there were no detectable unstimulated G o cells. Secondly, if the G l ' cells had been Go cells then the
254
NUCLEIC ACID ANALYSIS FILE PA
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Figure UAL DNA (52ORF AREA) versus 90°light scatter (488RS WDTH) for figure 11.40 data. The right column shows conventional contour plots with four gated regions used for data analysis.
stimulated cells within the cell cycle would have had to double in 4.9 hours after release from colcemid in order to attain the proportions seen in the various phases 4.5 hours after colcemid was washed off. The doubling time of the population, from cell counts, was about 36 hours. Thus, this new G l ' compartment, which may be similar or identical with the GlT compartment of Darzynkiewicy et al. (1980), is within the cell cycle and is blocked by colcemid. Kenter and Watson (1987) also used the acridine orange technique in conjunction with Southern blotting (Southern, 1975) to study the S(i to C|i immunoglobulin heavy-chain switching which occurs when stimulated spleen Bcells convert from being IgM expressors to IgG secretors. The proportions of the
RNA AND DNA
255
Cell cycle redistribution of B-cells with COLCEMID
+ 300-
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-100 control colcemid wash
Figure 11.42. Summary of colcemid induced changes in stimulated spleen B-cells showing the unexpected transit block between Gl' and GlA and its rapid reversal following colcemid removal. The expected G2 + M block is also apparent but this was not reversed within the 4.5 hours after colcemid removal. population in Go, Gl', GlA, GlB and S + G2 + M were determined at 24 hour intervals for 4 days after stimulation with LPS and dextran sulphate. It was then possible to estimate the various phase times with their standard deviations from a computer cell cycle model (Watson and Taylor, 1977). The experimental data represented by the points, and computer predicted results represented by the curves, are shown in figure 11 A3. The conversion from IgM expression to IgG secretion is accompanied by rearrangements within the immunoglobulin heavychain locus which are manifest by a loss of the S|i DNA signal from restriction enzyme digest patterns, and the loss of this signal was analysed at intervals after stimulation by Southern blotting. Computer simulations were then carried out
256
NUCLEIC ACID ANALYSIS
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DAYS 11.43. Computer model predicted data, curves, versus experimentally determined proportions of B-cells in G0 + Gl' (OX GlA (#), GlB (D) and S + G2 + M ( • ) at the times in days shown on the abscissa after LPS and dextran sulphate stimulation. with the results from the parallel cell cycle kinetic analysis to predict the proportion of S|i DNA signal remaining after stimulation. These results predicted that the SjJ, to Cjl heavy-chain switch would occur at approximately 85% into the cell cycle which placed it in mid S-phase on the first pass through the cell cycle after stimulation. This is an interesting result as it corresponds to the time in S-phase at which the immunoglobulin locus is replicated and the results are shown in figure 11.44. The predictions were confirmed experimentally by treating stimulated cells with aphidocholine which blocks cells in early S-phase. This also blocked the loss of the S(i signal but the switch was manifest by loss of the signal some 6 hours after release from aphidocholine.
11.7.2 Hoechst/pyronin-Y The staining procedures developed for RNA and DNA using acridine orange are somewhat 'harsh7 and the permeabilization step using acid—triton effectively excludes the addition for monoclonal antibody probing simultaneously with RNA and DNA. Furthermore, acridine orange staining is an equilibrium
RNA AND DNA
257
100 0.5tc
80-
3
4
5
6
7
Time, days
Figure 11.44. Computer predicted DNA rearrangement of Sji signal, curves, versus experimental data, points, obtained from Southern analysis of S|I signal loss. The curves were simulated with switch probabilities of 0.25, 0.5, 0.75 and 1.0 at times corresponding to early Gl(0.25tc), mid G l (0.5tc), Gl/S interface (0.75tc) and mid S-phase (0.85tc). The best correspondence between experimental and simulated data occurred at 0.85 tc with unit switch probability.
technique where the dye equilibrates with DNA, RNA, core and sheath and some groups have found it difficult to obtain consistent results. These considerations prompted Shapiro (1981) to investigate the possibility of using the combination of Hoechst 33342 plus pyronin-Y for RNA and DNA using dual wavelength excitation (UV and blue). CCRF-CEM cells and lymphocytes were used, adjusted to a concentration of 106 ml ~ l in medium and initially stained with Hoechst 33342
25S
NUCLEIC ACID ANALYSIS
Ho:DNA-
AO:DNA-
Figure 11.45. Hoechst 33342/pyronin-Y estimation of RNA and DNA simultaneously, from Shapiro (1981).
at concentration of either 5 |im or 10|iM. After 45 minutes incubation at 37°C pyronin-Y was added to give a final staining concentration of 5 |iM and the cells were analysed after a further 45 minutes incubation. Results from control and concanavalin-A stimulated lymphocytes were comparable with those from acridine orange as were those from CCRF-CEM cells. Results from the latter are given in figure 11.45 where the left panel shows pyronin-Y RNA fluorescence on the ordinate versus Hoechst 33342 DNA fluorescence on the abscissa. Comparable acridine orange staining with cells from the same culture are shown in the right panel. The DNA histograms are very similar but, the RNA resolution in late S-phase and G2 + M is not as good with pyronin-Y as with acridine orange. Shapiro (1981) also demonstrated that only about 60% of the 'RNA' signal from pyronin-Y could be abolished with ribonuclease in ethanol fixed CCRF-CEM cells. Therefore, there was a considerable background, due to non-RNA poly-anion binding, above which the specific RNA staining had to be scored. This non-specific background is likely to vary considerably between different cell types and is possibly one of the reasons for the inferior RNA resolution in late S-phase and G 2 + M compared with acridine orange. Nevertheless, Shapiro's results demonstrated that RNA and DNA could be measured simultaneously with this technique in 'intact' cells. The initial results from Shapiro (1981) prompted a comprehensive physicochemical study of pyronin-Y binding with synthetic polynucleotides by Kapuscinsky and Darzynkiewicz (1987) and a summary of their conclusions is as follows. Pyronin-Y is not RNA specific and only double-stranded nucleic acids form fluorescence complexes with the dye. Fluorescence is quenched by guanine
EMISSION SPECTRUM ANALYSIS
259
residues in both RNA and DNA. At high dye: phosphate ratios, when binding sites are saturated, about 80% of the fluorescence emission is from sites which do not contain guanine. Condensed complexes of pyronin-Y with nucleic acids have considerably reduced fluorescence compared with free dye and at concentrations above 5 x 10 ~5 M the dye preferentially condenses RNA (Darzynkiewicz et al, 1986). Thus, at high dye concentrations with mixtures of nucleic acids the fluorescence will tend to be from DNA which is more resistant to condensation than RNA (Portela and Stockert, 1979). At first sight these conclusions would seem to exclude the use of pyronin-Y as a stain for RNA. However, Darzynkiewicz et al. (1987) have shown that the presence of 0.8 jiM Hoechst 33342 in a 6.6 [iM solution of pyronin-Y increases the specificity of pyronin-Y for RNA and under strictly controlled conditions it can be used very effectively as a probe for RNA in fixed cells. This dye also enters viable cells, but it is taken up into mitochondria (Cowden and Curtis, 1983; Darzynkiewicz et al, 1986) and, therefore, cannot be used as a vital RNA stain (Darzynkiewicz et al, 1987).
11.8
Emission spectrum analysis
It was shown in figure 8.9 that multiple subsets are apparent in mouse bone marrow when Hoechst 33342 stained DNA fluorescence is analysed on two wavelengths simultaneously. Figure 11.46 shows time course results obtained with chicken thymocytes when stained at concentration of 5 |iM. The various panels were recorded at 15, 30, 45 and 125 minutes after the stain was added, top left, top right, bottom left and bottom right respectively (Watson et al., 1985a). Each panel shows the dot-plot of violet (440RF AREA) versus green (560RF AREA) fluorescence in the lower right-hand corner with the associated histograms, and each division on both the X- and Y-axes respresents 100 digitization channels with a maximum of 1024. In each panel there is a single peak on the violet analysis channel (Y-axis) but there are two peaks on the green channel (X-axis) at 15,45 and 125 minutes after staining. At 30 minutes, top right, there is a single peak on each axis. The dot-plots at 15 and 125 minutes show two major subsets very clearly. Figure 11.47 displays data comparable to that in figure 11.46 but with the dye concentration reduced to 1 (iM and only the 15 and 30 minute data sets are shown. Again, two major subsets are apparent. It appeared that the subset labelled 1 at 15, 45 and 125 minutes in figure 11.46 exhibited a 'tighter' distribution compared with that labelled 2. Furthermore, it also appeared that the former remained stationary with time but that the latter showed increasing green fluorescence. This observation is substantiated by the data shown in figure 11.47 (1 (iM Hoechst 33342), where the subset labelled 1 maintains its position at 15 and 30 minutes, but that labelled 2 shows an increase in both violet (Y-axis) and green (X-axis) with time. Moreover, subset 2 shows a greater initial increase in violet fluorescence compared with green, its position tends to be towards the upper left domain of the dot-plot. The proportions of cells in these two major subsets were counted by applying
260
NUCLEIC ACID ANALYSIS 15 min
30 min
560RF AREA
560RF AREA
1+2
45 min
125 min
560RF AREA
560RF AREA
Figure 11.46. Dot plots of violet fluorescence on the ordinate (440RF AREA, where 440, RF and AREA respectively denote analysis wavelength, right angle fluorescence and area under each pulse) versus green on the abscissa (with 560 denoting analysis wavelength) for chicken thymocytes stained with 5 uM Hoechst 33342 at 15, 30, 45 and 125 minutes after staining (respectively top left, top right, lower left and lower right). The associated histograms are shown against the relevant axes.
the elliptically gated regions as shown on the dot-plots. The mean percentages of cells within the three gated regions of figures 11.46 and 11.47 were scored as follows. Subsets 1 and 2 respectively comprised 33.2%+ 0.99% and 41.7%+1.53% of the population, where the limits represent 2 standard errors. Subset 3 contained 12.0%+ 0.55% and subsets 1 + 2 combined constituted 75.0%+ 1.09% of the whole population. About 10% of each data set was not included within any of the regions. It is clear from these data that the subsets designated 1 and 2 are discrete entities. It is also clear that the behaviour of these subsets with Hoechst 33342 staining is different and figure 11.48 shows the green and violet coordinates of the
EMISSION SPECTRUM ANALYSIS
261
15 min
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Figure 11.47. Similar display to that in figure 11.46 but with 1 uM Hoechst 33342 at 15 and 30 minutes after staining, top and bottom respectively. centers of the gated regions for subsets 1 and 2 of figure 11.46 plotted against time. Neither the green nor violet coordinates change significantly with time in subset 1, although there seems to be a tendency for both to fall slightly, and the violet coordinate does not change in subset 2. The significant feature, however, is the rise and then the plateauing of the green coordinate of subset 2. These data demonstrated that two different chicken thymocyte subsets could be distinguished by analysing the emission spectrum time course of the Hoechst 33342-DNA complex at two different wavelengths simultaneously. In one subset {33% of the
262
NUCLEIC ACID ANALYSIS 700
Region 1 600
violet > 500
green
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Figure 11.48. Green and violet fluorescence intensities for subsets 1 and 2, regions 1 and 2 respectively, plotted against time after staining with 5 uM Hoechst 33342 (data from figure 11.46).
total, designated 1) the development of both violet and green fluorescence was very rapid at a stain concentration of 5 |iM with maximal expression occurring in 15 minutes and no change thereafter. In the second subset (42% of the total, designated 2) the violet fluorescence was expressed equally rapidly, and to the same intensity (channel 500), but the green fluorescence increased throughout the 2 hour time course from an initial value of 410 at 15 minutes towards a plateau level of about 625 at 125 minutes. It was also interesting to note that decreasing the dye concentration to 1 |iM did not decrease the violet emission intensity of subset 1 (about channel 500, see figures 11.46 and 11.47), but it did decrease the green emission intensity by about 25%, from channel 500 to approximately 400. Again, however, neither the green nor the violet emission intensity changed in subset 1 at the lower dye concentration during the observation interval. In contrast, subset 2 at the lower dye concentration showed increasing fluorescence on both the green and the violet analysis bands with the latter increasing more rapidly than the former. The quantity of light emitted from a DNA—fluorochrome complex at a given time after staining with a Vital' dye will depend on a number of factors. These may be divided into three basic categories which will be considered under the headings transport, binding and microenvironment. The transport factors include the concentration of the dye, the rate at which it can traverse not only the external cell
EMISSION SPECTRUM ANALYSIS
263
membrane, but also the cytoplasm and possibly nuclear membrane, the rate at which the free fluorochrome is metabolized (if at all) and the rate at which the fluorochrome is 'excreted' by the cell. The binding factors include the ratio of the number of accessible binding sites for the dye to the intra-cellular dye concentration in the vicinity of the DNA and the rate constants for association and dissociation of the fluorochrome with DNA. Once the fluorochrome is bound to DNA the energy of the fluorescence emission, as opposed to the quantity, will depend on the type of binding of fluorochrome to DNA and the microenvironment (see section 3.8.4). Considering these various factors we could make some generalizations about the behaviour of the two major subsets observed in these experiments. It was apparent that the violet fluorescence from subset 1 was not dependent on the dye concentration within the range used (albeit relatively limited), and it was also temporally independent within the observed interval. Therefore, the factors included under both the 'transportation' and 'binding' headings had reached a saturated steady state for violet fluorescence which was neither concentration nor rate limited. This, however, was not true for the green emission from this same subset with the peak being at about channel 400 at 1 pM Hoechst 33342, and at about channel 500 at 5jiM Hoechst 33342 with no change with time at either concentration. Thus, the expression of green fluorescence in subset 1 was dye concentration dependent but time independent. The time independence shows that the expression of green fluorescence from subset 1 had reached a steady state by 15 minutes and the concentration dependence shows that saturation had not been attained at the lower Hoechst 33342 concentration and it may also not have been attained at the higher concentration, but at both concentrations a steady state had been reached. Turning now to population 2 we saw a very different pattern. The violet fluorescence remained constant from 15 to 125 minutes at the higher dye concentration, but there was a considerable increase between 15 and 30 minutes at the lower concentration (see the Y-axis histograms in figure 11.47). The green fluorescence intensity of this subset also showed increasing fluorescence with time not only at the lower (see X-axis histograms figure 11.47), but also at the higher dye concentration (see figure 11.48). Thus, the expression of both the violet and green fluorescence were dye concentration and time dependent in subset 2 over the concentration and time ranges used in these experiments. Moreover, it is clear from figure 11.47 that violet fluorescence in subset 2 was expressed more rapidly than green during the first 30 minutes. This was also apparent at the higher dye concentration (see figure 11.48) where at 15 minutes the green fluorescence intensity was relatively less than that of the violet, but beyond 30 minutes the green exceeds the violet. This is illustrated in figure 11.49 which shows the green: violet ratios for both subsets at the higher dye concentration plotted against time. Subset 2 exhibited an increasing ratio throughout the time course with a tendency towards a plateau level and subset 1 showed a near constant level, or possibly a small decrease towards a plateau value. Thus, the 'shape' of the Hoechst 33342 emission spectrum of cells in subset 2 changes with time with an
264
NUCLEIC ACID ANALYSIS 1.25
i Region 2
. ^o
o
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> c
1.00
d) 0)
Region 1
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0.75 30
60
90
120
Minutes
Figure 11.49. Ratio of green to violet fluorescence for subsets 1 and 2, regions 1 and 2 respectively, plotted against time after staining with 5 uM Hoechst 33342.
increase in green emission, but that of subset 1 did not. It was this difference which made it possible to distinguish the subsets. These various observations strongly suggested that two different binding sites, or two types of binding at the same site might exist; one emitting violet fluorescence preferentially, the other emitting green preferentially indicating different binding energy states. It is also pertinent to observe that the total fluorescence emission from subset 2 was greater than that from subset 1 at the higher dye concentration at 125 minutes. This can be seen from the data presented in figure 11.48 where the sum of the green and violet intensities is 1035 for subset 1 and 1150 for subset 2, an increase of 10%. It is highly unlikely (though not impossible) that subset 2 contains 10% more DNA than subset 1. It is much more likely that the differences observed are due to different dye binding properties in the two subsets with both containing approximately the same number of available sites which give rise to violet fluorescence preferentially and with subset 2 containing more binding sites which give rise to green fluorescence preferentially. From the evidence available in these experiments we proposed that two DNA binding sites, or two binding states, exist for Hoechst 33342. As the violet fluorescence was expressed more rapidly than the green we considered this to be the primary, 'V-site', and the green, 'G-site', to be secondary. In further more extensive studies (Smith et a\., 1985) it was shown that the Hoechst 33342 emission from DNA is highly pH dependent, which can have profound consequences for the green: violet ratio. In summary it is possible to make the following statements.
EMISSION SPECTRUM ANALYSIS
265
(1) The bisbenzimidazoles bind preferentially to repetitive A —T sequences (see review by Latt, 1979) with dye molecules occupying the minor groove of the helix at low dye: DNA-phosphate ratios. (2) The fluorescence emission primary mode binding tends to be violet biassed. (3) Increasing the dye: DNA-phosphate ratio leads to further binding where the dye molecules align more closely with the base planes (Bontemps et al.f 1975; Latt and Stetten, 1976). This secondary binding leads to fluorescence quenching (Bontemps et al, 1975) and being cooperative suggests conformational changes in DNA. (4) A manifestation of the quenching process is a shift of the fluorescence emission to longer wavelengths (lower energy).
12 Nucleic acids and protein
The central dogma of biology, a term coined by Francis Crick, is that DNA makes RNA and RNA makes protein. It is self-evident, therefore, that the capacity simultaneously to measure DNA, RNA and protein at the individual cell level is of fundamental importance. We have seen in the previous chapter that DNA and RNA can be measured simultaneously. However, those measurements were of total DNA and RNA and ideally we would also wish to be able to measure specific gene copy number, messenger RNA (mRNA) and the protein product at the single cell level. The last of these can be quantitated with ease by flow cytometry using monoclonal antibodies and developments are taking place for the detection and measurement of specific genes with in situ hybridization in whole nuclei (Trask et al, 1985,1988). Furthermore, some recent work has enabled ribosomal RNA to be detected in suspended cells using hybridization (Bauman and Bentvelzen, 1988) and Dunne, Thomas and Lee (1989) have sorted small numbers of tells directly onto nitrocellulose filters then probed for interleukin-1 mRNA. However, specific mRNA and copy number cannot yet be quantitated, but I suspect that this will be possible within the next five years or so with improvements in hybridization techniques, the use of nick-translation with biotinolated nucleotides, streptavidin fluorochrome amplification and improvements in instrumentation. The simultaneous staining of DNA with propidium iodide and protein with fluorescein, either directly (FITC) or indirectly with antibodies, has been mentioned in sections 3.S3, 10.3 and 11.1.2 and application of this particular combination will be considered further in sections 12.3, 12.4 and chapter 15. The major problem with propidium iodide is that cells must be permeabilized to allow entry of the highly polar dye. This can only be overcome for viable cell analysis using the Hoechst dyes.
12.1
Viable cells
The combination of DNA staining with Hoechst 33342 and surface immunofluorescence with fluorescein on viable lymphocytes and myeloma cells was introduced by Loken (1980). This combination of fluorochromes requires two excitation wavelengths, UV for DNA/Hoechst and 488 nm for fluorescein. Loken (1980) excited both dyes with a single argon laser containing a specially
267
VIABLE CELLS
constructed set of multi-line mirrors which allowed both the UV and blue lines to be emitted by the laser. Initially, some difficulty was encountered due to the brightness of the DNA/Hoechst fluorescence emission in comparison with that from the fluorescein (see section 3.8.3). However, this was overcome by using biotinolated antibodies with avidin-coupled fluorescein as the second layer to give a degree of immunofluorescence amplification, reducing the output power of the UV compared with the blue laser lines by altering the current and magnetic field applied to the laser tube and by electronic compensation for the spectral overlap (see section 4.2.3). Some of these manoeuvres are highly specialized and it is preferable to use two lasers (if you have them) for three reasons. Firstly, the light outputs can be independently controlled with complete precision. Secondly, both beams can be focussed to the same point or offset in the vertical plane for sequential illumination. Finally, sequential excitation overcomes potential spectral overlap problems. Loken (1980) probed lymph node lymphocytes with an anti-Thy-1.2 antibody then stained with Hoechst 33342 at a concentration of 1.0(ig ml" 1 . Tlymphocytes stain more dimly with this concentration of Hoechst 33342 and he was able to show that these cells were Thy-1.2 positive and obtained a complete discrimination from the B-cells. Exponentially growing S107 myeloma cells, which express large quantities of cell surface IgA, were similarly double stained with Hoechst 33342 and a rabbit anti-IgA antibody and these results are reproduced in figure 12.1. Panel A shows IgA-associated fluorescence on the ordinate versus
cr
o
(0
DNA Fluorescence
Frequency
Figure 12.1. Panel A shows the dot-plot of specific IgA versus specific DNA fluorescence, from fluorescein and Hoechst 33342 respectively, after electronic compensation. Panels B and C respectively show the associated DNA and IgA monodimensional histograms. Redrawn from Loken, 1980.
268
NUCLEIC ACIDS AND PROTEIN
DNA/Hoechst fluorescence on the abscissa with the respective mono-dimensional histograms in panels B and C. Hollander and Loken (1988) extended this approach to the analysis of human bone marrow using sequential excitation with two lasers emitting 488 nm and UV light respectively. The 488 nm line excited either fluorescein or phycoerythrin tagged CD4 or CD34 and the UV was used for Hoechst/DNA. The progenitor cells defined as CD34 positive had the same G 0 /Gl DNA peak as other subsets and these were relatively quiescent with an overall DNA content proliferative index of about 6%. Almost all the cells with S, G2 + M DNA content were within the lymphoid, erythroid and myeloid series after CD34 expression was lost during
NUCLEAR-ASSOCIATED ANTIGENS
269
involved in DNA packing and together with DNA they form chromatin. There are five histones. Four of these, in pairs making an octomeric unit, constitute the cylindrical nucleosome core around which is wrapped two turns of doublestranded DNA. The 'input' and 'output' DNA strands to the nucleosome are tacked into place by the fifth histone. DNA between each nucleosome is termed linker DNA and the whole structure resembles 'beads on a string'. The nuclear enzymes include DNA polymerases, restriction enzymes, ligases, damage recognition and repair enzymes, transcriptases, DNAases and topoisomerases. Polymerases, as their name implies, are responsible for linking together the bases and deoxyribose sugars during DNA synthesis. Restriction enzymes cut DNA at very specific base sequences. They may be involved in physiological geonomic rearrangements of the types which occur at the immunoglobulin locus with the C|i to S|i heavy chain switch as spleen B-cells convert from IgM expressions to IgG secretors. The ligases join DNA strands together at specific sites and their function is the converse of restriction enzymes. DNA damage recognition/repair enzymes are not clearly understood. Thymine dymers, induced by UV irradiation, are repaired in normal cells and there may well be a component where damage has to be recognized before it can be repaired. The repair process involves DNAases which digest out a stretch of bases either side of the damaged site before reconstruction takes place on the complementary strand. It is, however, contentious as to whether specific enzymes exist which recognize the damage before it can be repaired. The transcriptases are responsible for transcribing the genetic code contained within the DNA into messenger RNA which is subsequently translated into protein in the ribosomes. Topoisomerases are DNA strand passing enzymes and are of two types, I and II, which respectively pass single- and double-stranded DNA. They are responsible for the topological integrity of DNA and are involved in winding and unwinding super-helical DNA by strand breakage and rejoining.
12.3.1 Quantitation with antibodies One of the first reports of nuclear-associated antigen quantitation is due to Gershey (1980) who used an antibody directed to SV-40 large T-antigen which binds to chromosomes in infected cells (D'Alisa and Gershey, 1978; D'Alisa, Korf and Gershey, 1979). A fluorescenated probe was used for large T with propidium iodide for DNA content. Since then a number of antibodies have been produced which recognize nuclear antigens and some are now commercially available. They include antibodies to p53 (Harlow et al, 1981), p62c~myc (Evan et al, 1985), p55c~f°s (Evan et al, 1985) and topoisomerase II (Liu, 1983). Some antibodies recognize nuclear antigens in stimulated cells, 6-B1012/N (Reeve, personal communication) and Ki-67 (Gerdes et al, 1983) and others recognize preferentially cell cycle dependent nuclear antigens. These include specific regions in condensed chromatin (MAB 244-7, mW 34 Kd), interchromatin granules (MAB 780-3, mW 105 Kd and 41 Kd) and euchromatin (MAB 58-15, mW 36 Kd) (Epstein and
270
NUCLEIC ACIDS AND PROTEIN
Clevenger, 1985; Clevenger et al, 1985). This list is by no means exhaustive and the number of antibodies which recognize nuclear components is increasing very rapidly. The precise functions of most of the proteins cited in the previous paragraph are not understood but possibilities include both reception and/or transduction of gene regulatory signals from the cytoplasm. Likely candidates for regulatory functions are the various steroid receptors and the protein products of the c-myc, c-fos and c-myb genes; p 5 5 c ~ / o s appears to be a factor necessary for transcription (Distel et al, 1987; Lech, Anderson and Brent, 1988) but the function of the c-myc and related proteins of the myc family (encoded by the N-myc, L-myc and v-myc genes) are not known although the evidence suggests that the c-myc product is involved in cell proliferation regulation. Kelly et al (1983, 1984) have shown that c-myc messenger RNA increases rapidly after mitotic stimulation of lymphoid cells. Similar results with hepatocytes after partial hepatectomy (Makino, Hayashi and Sugimura, 1984) and with growth factor stimulation of quiescent 3T3 cells (Greenberg and Ziff, 1984) have been obtained. It may also play a part in differentiation as mRNA copy number shows a peak at 4—5 weeks in developing placenta (Pfeiffer-Ohlsson et al, 1984) and a peak during spermatogenesis with stem cells and mature sperm showing very low levels (Stewart, Bellve and Leder, 1984). The protein products of the mouse c-myc and human c-myc, N-mcy and L-myc genes share a common amino acid sequence motif, the 'leucine zipper7, in conserved regions (Landschultz, Johnson and McKnight, 1988). This motif is also found in the yeast DNA regulatory protein GCN4 and in the proteins encoded by the v-fos and jun oncogenes which have transcriptional activity (Vogt, Bos and Doolittle, 1987; Landschultz et al, 1988). Evan and Hancock (1985) have shown that p62 c ~ myc is one of a discrete set of non-histone and non-nuclear matrix proteins which elute from the nucleus at salt concentrations below 200 mM. This evidence taken together with the structure of the conserved region suggests a DNA binding function which can be modulated rapidly by ionic changes within the physiological concentration range. Furthermore, both the protein and its mRNA are turned-over with half-times of between 20 and 40 minutes in stimulated cells (Hann, Thompson and Eisenman, 1985; Rabbitts et al, 1985) with no cell cycle phase dependency (Thompson et al, 1985; Rabbitts et al, 1985). The mRNA and protein were synthesized de novo during each phase of the cell cycle and a time course experiment showed that an increase in p62c~myc level in Gl preceeded entry into S-phase. With subsequent development of quiescence the level in Gl decreased before the S-phase fraction decrease (Rabbitts et al, 1985; and see later in figure 12.3). Most of the above information was obtained with blotting techniques which can only give the grand average for the whole population. However, the work of Rabbitts et al (1985) also contained flow cytometric data. The left panel of figure 12.2 shows the results obtained from serum-stimulated exponentially growing 3T3 cells stained for DNA (ordinate) versus p62c~myc associated immunofluorescence (abscissa) using propidium iodide (red) and fluorescein (green) respectively
NUCLEAR-ASSOCIATED ANTIGENS
271
Figure 12.2. The left panel shows DNA (ordinate) versus specific fluorescence on the abscissa for stimulated 3T3 cells. The right panel shows that the p62 c~myc associated fluorescence is abolished by pre-incubating the anti-p62 c ~ myc antibody with the peptide used as the immunogen.
after freeze-thaw premeabilization. The monoclonal antibody used to probe ( M Y C J.5E2Q) w a s S y n thetic peptide induced (Evan et al, 1985) and the right panel shows that preincubation of the antibody with the peptide used as the immunogen before staining abolished the green fluorescence signal. These data demonstrated that the p62 c ~ myc levels do not exhibit cell cycle dependent changes which confirmed the Western blotting data of Thompson et al (1985). Figure 12.3 shows the time course experiment mentioned above. Total DNA content and p62c~myc levels were determined simultaneously at daily intervals in 3T3 cells after stimulating quiescent cells by splitting the monolayer and reseeding at low density in fresh medium. The solid curve and squares show the p62c~myc changes in Gl (left ordinate) versus time (abscissa) and the open triangles and dashed curve depict the proportions in S-phase (right ordinate). The potential value of flow cytometric techniques is also demonstrated by work from Clevenger et al (1985), R. J. Epstein (1988) and R. J. Epstein et al (1988). The former group of authors used a monoclonal antibody directed towards interchromatin granules (MAB 780). These data, obtained with the paraformaldehyde/triton technique and the usual fluorescein (antibody) and propidium iodide (DNA) staining combination, are shown in figure 12.4. The log of the MAB 780 associated fluorescence is plotted on the ordinate versus DNA on the abscissa. The arrowed population is intensely stained and represents mitotic cells, but these would not have been apparent with a 'bulk' analysis procedure such as Western blotting which cannot reveal minority subsets in heterogeneous samples. p62 c-myc
NUCLEIC ACIDS AND PROTEIN
272 2500-1
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Figure 12.3. Time course for changes in p62 c myc levels in G l (squares and left ordinate) and percentages of cells in S-phase (triangles and right ordinate) after stimulating quiescent 3T3 cells with fresh medium (Rabbitts et al, 1985).
MAB 780 240
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DNA content (channel number) Figure 12.4. The log of the MAB 780 associated fluorescence plotted on the ordinate versus DNA on the abscissa. The intensely stained arrowed population represents mitotic cells. Redrawn from Clevenger et al. (1985).
NUCLEAR-ASSOCIATED ANTIGENS
273
Epstein (1988) and Epstein et al. (1989) have studied topoisomerase II levels simultaneously with DNA using fluorescein immunofluorescence and propidium iodide in T-4 7D breast cancer cells during oestrogen stimulation and some of these results are shown in figure 12.5. The origin in each panel is on the left with DNA displayed obliquely from top left to bottom right and topoisomerase II associated fluorescence displayed from bottom left to top right. Frequency, as usual, is scored on the vertical (Y) axis. Control cells stained with the fluorescenated second antibody only are shown in the top left panel. The bottom two panels demonstrate the effects of stimulating cells with oestrogen for 4 and 16 hours, shown in the left and right panel respectively. With increasing time of stimulation there are increasing number of cells exhibiting positive staining with the anti-topoisomerase II antibody. However, the bottom right panel(16 hours stimulation) shows that a small subset of cells in Gl do not exhibit a marked increase in topoisomerase II. The top right panel shows the effects of treating the 16 hour stimulated cells with a high salt buffer which partially dissociates topoisomerase II from the nucleus thus reducing the fluorescence signal. These data demonstrate that this type of flow cytometric technique is capable of determining changes within subsets in heterogeneous populations that could not be made with bulk sample methods. 12.3.2 Turnover measurements Turnover studies of p62c~myc were also conducted by Rabbitts et al (1985) using flow cytometry and these data are shown in figure 12.6. Exponentially growing 3T3 cells at 48 hours after serum stimulation, when both the p62 c ~ myc levels and proportion in S-phase were at a maximum (see figure 12.3), were treated with cyclohexamide which blocks protein synthesis. The MYC 1—6E10 antibody was used to probe for the protein at intervals thereafter and the top, middle and bottom panels respectively show the p62c~myc changes in Gl, S and G2 + M. There was an initial small rise in p62 c ~ myc levels in all cell cycle phases followed by a rapid fall compatible with a half-time of 30 minutes. Western blot data from parallel experiments using actinomycin-D to block mRNA then subsequently the protein, gave directly comparable qualitative results, see figure 12.7. However, these data were only meaningful as the protein levels and turnover were very similar throughout the cell cycle. If there had been marked cell cycle dependent absolute levels and/or turnover the Western blot data would have been meaningless. Furthermore, this would not have been apparent without either similar studies on synchronized cells or flow cytometric analysis. 12.3.3 Cell cycle modulation The data discussed in sections 12.3.1 and 12.3.2 concerning the role of p62 c ~ myc point to some form of control mechanism which is acting at the G o to Gl transition with p62c~myc elevation being required not only to facilitate entry of cells into the cell cycle but also to maintain cells in a potentially active proliferating state. Some evidence suggests that p62c~myc participates in DNA synthesis (Studzinski et al, 1986). However, cells are extraordinarily efficient and logical in
#2 FLU CON
Figure 12.5. DNA (propidium iodide) versus topoisomerase II content (fluorescein immunofluorescence) in T-47D cells after oestrogen stimulation (Epstein, 1988, and Epstein et al., 1989). The origins are on the left with DNA displayed from top left to bottom right and topoisomerase II displayed from bottom left to top right. Fluorescence control cells are shown in the top left panel. Oestrogen stimulation for 4 and 16 hours are shown bottom left and bottom right respectively. The data after treatment with high salt buffer partially to dissociate topoisomerase II are shown top right.
NUCLEAR-ASSOCIATED ANTIGENS
lib
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Figure 12.6. Turnover of p62 c myc. Exponentially growing 3T3 cells were treated with cyclohexamide which blocks protein synthesis. The p62 c ~ myc levels were then followed versus time. There was an initial increase then a rapid decrease in all cell cycle phases (top, middle and bottom panels represent Gl, S and G2 + M respectively) compatible with a half-time of 30-40 minutes (Rabbitts et al., 1985).
276
NUCLEIC ACIDS AND PROTEIN
Act ino. D 30
60
120
240 mins.
Figure 12.7. Pulse-chase Western blot data for cells treated for 1 hour with [3H]lysine in the presence of 5 jig ml" 1 actinomycin-D then assayed at 30, 60, 120 and 240 minutes. There was a rapid decrease in the signal which was completely undetectable at 120 minutes (Rabbitts et a\., 1985). performing their various functions and there is no reason for the c-myc gene to be activated early in Gl to produce mRNA for p62 c ~ myc with both being turned-over at such rapid rates if the protein is only required in S-phase. Because of these considerations Jon Karn of the Laboratory of Molecular Biology, Cambridge, constructed a series of retroviral vectors containing the c-myc gene in various configurations to investigate p62c~myc cell cycle dependency using the BrdU-antibody technique. These retroviral constructs were composed of SV-40 promoter regions (SV0), c-myc long terminal repeat sequences (LTR), a c-myc 'mini-gene' containing the protein coding exon sequences without the introns and the neomycin resistance gene (NEO) for selection purposes. A number of retroviruses were constructed and the structures of three of these, VSN-2, NSM-4 and MSN-7, are shown in figure 12.8. All three viruses contained SV0 (SV-40
NUCLEAR-ASSOCIATED ANTIGENS
277
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promoter), the NEO gene and myc LTRs, but only NSM-4 and MSN-7 contained the myc gene. In NSM-4 the myc gene was under the control of SVO, but in MSN-7 it was under control of its own LTR. After cells were infected with these viruses there was no enhanced production of p62c~myc in the VSN-2 cell line, some enhancement in the NSM-4 cells and considerable enhancement in the MSN-7 cells which was the expected result (Karn et al, 1989). The growth rates of the three cell lines showed progressive increases with p62c~myc amplification, with V S N < N S M < M S N , which I'll abbreviate to V-, N- and M-cells. The cell cycle kinetics were determined by following the changes in BrdU signals versus total DNA at hourly intervals after flash labelling and selected data sets are shown in figure 12.9 for the three cell lines. The left, middle and right columns show the data from the V-, N- and M-cells respectively and the rows, from top to bottom, show the data obtained at 0, 4, 8 and 12 hours after labelling. The origins in these three-dimensional displays are on the left of each panel where BrdU-associated green fluorescence (520RF AREA) is scored obliquely from bottom left to top right and total DNA (630RF AREA) is scored from top left to bottom right. Frequency is scored on the vertical axis. The large 'spike' in each of the top three rows, the time zero data for each of the three cell lines, represents unlabelled Gl cells and is centered at channel 300 on the DNA axis. The S-phase fractions are represented by the characteristic U-shaped patterns and the G2 + M cells, which are also unlabelled, are represented by the small 'spikes' centered at
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NUCLEIC ACIDS AND PROTEIN
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2.9. Bivariate perspective histograms of DNA versus BrdU for V-, N- and M-cells in the columns at 0,4,8 and 12 hours after pulse labelling in the rows. The origins are on the left with DNA displayed from top left to bottom right and BrdU incorporation displayed from bottom left to top right.
channel 600 on the DNA axis. The second row shows the data at 4 hours and in each panel the most obvious change is that some cells which were in late S-phase when the BrdU was added have progressed through G2 + M, split into two and in so doing have halved their BrdU content and now appear with Gl DNA content at channel 300 on the DNA axis (520RF AREA). These are the Gl cells with the positive green signals which appear to 'stream out7 from the large Gl spikes from bottom left to top right. The next row down shows the data obtained at 8 hours and a number of further changes have taken place. Firstly, most of the cells which were initially in S-phase (BrdU positive) have passed through G2 + M, halved their BrdU content and are now scored with Gl DNA content and positive green (BrdU) signals. Secondly, a relatively large fraction of the BrdU labelled V-cells are
NUCLEAR-ASSOCIATED ANTIGENS
279
still in G2 + M compared with the M-cells (row 3, left and right panels respectively). The N-cells, middle panel, show an intermediate pattern. Thirdly, it is now quite obvious that there has been significant progression of the initially unlabelled Gl cells which are BrdU negative. These have moved out of Gl along the DNA axis (630RF AREA) in the direction top left to bottom right and are progressing towards G2 + M. Finally, it is equally clear that the M-cells have progressed further towards G2 + M than have the V-cells, and again the N-cells occupy an intermediate position. By 12 hours the M-cells, right panel bottom row, are exhibiting a pattern qualitatively similar to their time zero counterpart in the right panel of the top row, but where the BrdU labelled cells have half their original green fluorescence signals. In contrast the V-cells at 12 hours, left panel bottom row, still show some cells in G2 + M with positive BrdU signals (these are situated on the rear right wall of the display as the spike) but the majority of these have a G l DNA content. Also, some of the initially unlabelled Gl cells are still in S-phase and G2 + M, where the latter are clearly seen as a spike at channel 600 on the DNA axis. Again the N-cells display an intermediate pattern between the V- and M-cells. The data in figure 12.9, together with the remaining majority of data sets in the experiment, were analysed by placing gates around both the labelled and unlabelled Gl, S and G2 + M regions to obtain the proportions in each of these compartments. Figure 12.10 illustrates this procedure where panel A shows the control time zero data for the V-cells and panel B shows the zones used in the
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DNA fluorescence Figure 12.10. Panel A shows BrdU uptake into V-cells at time zero where the characteristic incorporation horse-shoe is readily evident. Panel B shows the gates used to assess the unlabelled proportions in Gl, S and G2 + M (zones 1, 3 and 2 respectively) and the labelled proportions in Gl, S and G2 + M (zones 4, 6 and 5 respectively).
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NUCLEIC ACIDS AND PROTEIN Zone 1 (G1)
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Time, hours Figure 12.11. The proportions defined in zones 1, 3 and 2 of figure 12.10, unlabelled cells, plotted as the points on the ordinates versus time on the abscissae. The cell cycle phases, Gl, S and G2 + M, are arranged in the columns for V-, N- and M-cells in the rows. The curves were calculated from the 'Hartmann-Pederson' type computer model (Watson and Taylor, 1977; Kenter and Watson, 1987) described in section 11.5.3.
gating analysis procedure where 1, 3 and 2 correspond to unlabelled Gl, S and G2 + M cells respectively and where 4, 6 and 5 correspond to labelled Gl, S and G2 + M cells. The data for the unlabelled population are shown in figure 12.11 where the various proportions are plotted as the points on the ordinates versus time on the abscissae. The cell cycle phases, Gl, S and G2 + M are arranged in the columns for V-, N- and M-cells in the rows. Figure 12.12 shows the comparable data for the labelled cells, i.e. those initially in S-phase. The curves were calculated from the 'Hartmann-Pederson' type computer model (Watson and Taylor, 1977; Kenter and Watson, 1987) described in section 11.5.3. The durations of Gl, S and G2 + M with their 95% confidence limits are shown in figure 12.13 where it can be seen that the durations of S-phase and G2 + M were not significantly different in the three cell types. However, there was a progressive reduction in the duration of G l from V- to N- to M-cells. Further experiments were carried out where the three cell types were BrdU pulse-chased into serum free medium. Again, the durations of S-phase and of G2 + M were not altered but there was a progressive increase in the length of Gl which was greater in V- than in N- than in M-cells. These data not only add support to the hypothesis that p62 c ~myc is involved in cell cycle regulation but also suggest very strongly that this control is exerted in Gl. Furthermore, the control mechanisms for c-myc mRNA and protein are themselves typical of fast response regulatory systems. Blanchard et al. (1985) have
281
NUCLEAR-ASSOCIATED ANTIGENS Zone 4 ( G 1 )
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Figure 12.12. Similar display to figure 12.11 for zones 4, 6 and 5 (Gl, S and G2 + M respectively) of figure 12.10 which represent the labelled cells which initially were in S-phase.
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Figure 12.13. Durations of Gl, S and G2 + M with their 95% confidence limits. The durations of S-phase and G2 + M were not significantly different in the three cell types. However, there was a progressive reduction in the duration of G l from V- to N- to M-cells.
282
NUCLEIC ACIDS AND PROTEIN
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Figure 12.14. Turnover of p62c ~ myc in quiescent 3T3 cells, a similar experiment to that infigure12.6, but these data show that the protein is turned over with a very much longer half-time.
shown that the c-myc gene is transcribed at an equal rate in both quiescent and stimulated Chinese hamster fibroblasts. However, the message was not detectable in the former which means that degradation must have been taking place at the same rate as production. Following stimulation the mRNA level increased which had to be due to a decrease in the degradation rate as there was no demonstrable increase in transcription. This, therefore, represents part of a negative servo control loop which is inhibited by serum stimulation causing a rise in mRNA transcripts and a subsequent rise in protein content. The reverse control process seems to operate at the protein level. In quiescent cells the half-life of the protein is relatively long (250—350 minutes, see figure 12.14) but the absolute content is low; in stimulated cells the half-life is shorter but the level is higher. Thus, the p62 c ~myc content is controlled by two different processes, predominantly at the mRNA degradation level in quiescent cells and predominantly at the protein level after stimulation. The combination of these two control processes is capable of giving rise to very tight regulation of the absolute protein content with the possibility for very rapid modulation.
12.3.4 Dual antigens plus DNA This type of assay can be carried out using two antibodies and a DNA stain as mentioned in section 7.3.2 but the method requires dual wavelength excitation. Our approach (Watson et al.f 1987b) was to probe the c-myc protein with a mouse monoclonal anti-p62 c " m};c antibody then secondarily stain this with a sheep anti-mouse immunoglobulin (IgG) coupled to the UV fluorochrome amino-methyl coumarin acetic acid (AMCA). The c-fos protein was then probed with a synthetic peptide induced rabbit anti-serum which was then stained with a fluorescenated swine anti-rabbit antibody (FITC-SaR) and DNA was stained with propidium iodide. Figure 12.15 shows the emission spectra of the three fluorochromes together with the excitation wavelengths used and the band passes
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Figure 12.15. Emission spectra of AMCA, fluorescein and DNA/propidium iodide with the band passes through which the spectra were analysed indicated by the stippling. The krypton UV lines and the argon 488 nm line are indicated by the arrows.
through which the emissions were quantitated. The 90° scatter versus DNA data space for nuclei extracted from a paraffin wax embedded biopsy of ovarian carcinoma is shown in figure 12.16 which exhibits an aneuploid (Anu) as well as a diploid (Dip) component. These two populations were then gated and the p55c~fos versus p62c~myc associated fluorescence data (520 and 420 nm respectively on the ordinate and abscissa) for both populations are shown in figure 12.17.
12.4 Cytoplasmic antigens 12A.I
Immunoglobulin Zeile (1980) was perhaps the first investigator to analyse intracytoplasmic immunofluorescence simultaneously with DNA in a report which appeared in the same issue of Cytometry as Gershey's paper (1980, and see section 12.3.1) where SV-40 large T antigen was assayed. Zeile (1980) studied bone marrow from 12 patients with multiple myeloma which was disaggregated with collagenase, treated with ice-cold saline containing 0.01% triton X-100 then stained with fluorescein-conjugated anti-human immunoglobulin and propidium iodide.
284
NUCLEIC ACIDS AND PROTEIN
DNA
5
Anu
Figure 12.16. The 90° light scatter versus DNA for an aneuploid ovarian cancer biopsy extracted from paraffin wax. The diploid (Dip) and aneuploid (Anu) components are arrowed.
420 nm (MYC)
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Figure 12.17. The green fluorescence (520 nm, p55 c fos versus low blue fluorescence (420 nm, p62c~myc) data space for the data of figure 12.16 in which the diploid (Dip) and aneuploid (Anu) components are completely separated.
CYTOPLASMIC ANTIGENS
285
Characteristic patterns of normal and pathological immunoglobulin-producing cells were obtained. Hayden et al (1988) extended this approach to quantitate cytoplasmic and surface antigens simultaneously but they did not also measure DNA although this could be carried out with some modifications to their technique. Their method involved initial cell surface antigen staining with a directly fluorescein-conjugated antibody followed by permeabilization and probing cytoplasmic antigens with biotinolated antibodies which were subsequently stained with avidin— phycoerythrin or streptavidin—texas red. A number of permeabilization steps were investigated including 0.1% gluteraldehyde plus 1% saponin (Newell, Hannam-Harris and Smith, 1983), 0.01% triton X-100 (Zeile, 1980), lysolethicin (Schroff et al, 1894) and 50% ethanol in either PBS or RPMI (Walker et al, 1985) and they finally chose the last of these. This method could be used to add DNA staining by probing for the latter on the red channel with propidium iodide, using the green fluorescein channel for the 'brightest' antigen and probing the second antigen with a biotinolated antibody and staining this with streptavidin-AMCA. This combination of fluorochromes was used in the previous section.
12.4.2 Cytoskeleton Mammalian cells contain filamentous protein networks which make up the cytoskeleton (Ramaekers et al, 1983). These can be classified into four types based on their diameters assessed by electron microscopy (Schliwa and van Blerkom, 1981). Microtrabecular filaments are the smallest measuring 2—3 nm in diameter. Microfilaments measure 5—7 nm and microtubules are 22—25 nm in diameter. The last group comprises the intermediate filaments which measure 7-11 nm in diameter. These different groups are further characterized by the various proteins which contribute to their structure, i.e. actin, tropomyosin, tubulin and the intermediate filament (IF) proteins. The latter are subdivided into five different groups which are tissue type specific namely, keratins (epithelia), vimentin (mesenchyme), desmin (muscle), neurofilament proteins (nerve cells) and glial fibrillary ascidic protein (GFAP, astrocytes) (Anderton, 1981; Franke et al, 1978, 1981; Holtzer et al, 1981; Lazarides, 1980, 1981, 1982; and Osborne et al, 1981). Moreover, neoplastic transformation does not alter tissue specific expression of intermediate filament proteins and antibodies to these have been used in the differential diagnosis of 'difficult' biopsies using immunofluorescence and immunoperoxidase techniques (Battifora et al, 1980; Ramaekers et al, 19S2a,b; Sieinski, Dorsett and Ioachim, 1981). These techniques have also been adapted for flow cytometry and used to distinguish between (Ramaekers et al, 1983) and sort cells (Oud et al, 1985) on their IF-protein content and to study tubulin expression in the cell cycle (Wang et al, 1988). The latter is potentially of importance in proliferation regulation. Wang and Rozengurt (1983) have shown that there appears to be an interaction between microtubules and cyclic AMP in modulating initiation of DNA synthesis in 3T3 cells and Ball, Albrecht and Carrey (1982) report that microtubules are involved in
NUCLEIC ACIDS AND PROTEIN
286
T24
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1
Cytokeratin, FITC
Figure 12.18. Dual parameter analysis of the T24 bladder cancer cell line and the lymphoid cell line Molt-4 using DNA and cytokeratin content. Panels A, C and E respectively show the DNA histograms for T24, Molt-4 and a mixture of the two. Panels B, D and F show the bivariate dot-plots of DNA (PI staining) versus FITC immunofluorescence probed cytokeratin. T24 was positively labelled (B, top right) but Molt-4 was negative (D, middle right). Panel F (bottom right) shows the mixture and the T24 gate' was used to assess the DNA histograms associated with each cell type in the mixture.
CYTOPLASMIC ANTIGENS
287
cytomegalovirus initiation of DNA synthesis. Moreover, Crossin and Carney (1981a,b) have shown that tubulin depolymerization early in the cell cycle is sufficient to initiate DNA synthesis (1981a) and that taxol stabilization of tubulin inhibits initiation of DNA synthesis after thrombin and epidermal growth factor stimulation (1981b). One of the first examples of the use of intermediate filament antibodies in flow cytometry to distinguish between different cell types is due to Ramaekers et al. (1984) and their results are reproduced in figure 12.18. The T24 bladder cancer cell line and Molt-4 lymphoid cells were assayed simultaneously for cytokeratin and DNA both separately and in a mixture of the two. The left column from top to bottom shows the DNA histograms (propidium iodide staining) for T24, Molt-4 and the mixture. The right column shows the bivariate cytograms of DNA on the ordinate versus cytokeratin associated immunofluorescence on the abscissa. T24 cells exhibited positive staining for cytokeratin (top panel) but Molt-4 showed no staining (middle panel). The mixture of the two cell types shown in the bottom panel on the right suggested that the two cell types could be completely resolved in the DNA/cytokeratin data space. This was confirmed by placing a gate to include the T24 cells as shown and re-analysing the DNA histogram data of each component of the mixed population. The results were essentially identical to those from the individual populations. It is also worth noting that a chicken RBC internal standard was used in these experiments and that the T24 and Molt-4 DNA histograms are very similar to the hypothetical histograms used as illustrations in figure 11.10.
13 Chromosomes
Conventional chromosome analysis and karyotyping is time consuming, laborious and to some extent subjective as it relies upon interpretation of banding patterns and morphological features. These can vary with staining conditions and preparative methods and results are usually presented for very few metaphase spreads. This inevitably introduces a selection bias as only those preparations which are interpretable can be presented. However, these may not always be representative of the population under study. These considerations apply to any image analysis system including the best of them all, the human eye and mind, but these will always be limited in statistical precision due to the relatively few numbers of objects analysed. A new approach in which many thousands of chromosomes can be analysed using flow cytometry, termed flow cytogenetics, was submitted to the National Academy of Sciences, USA, by Joe Gray and colleagues in December 1974 (Gray et al, 1975b). Chinese hamster cells (M3-1, clone 650A) were used and chromosomes were prepared according to the method of Wray and Stubblefield (1970). The chromosomes were stained with ethidium bromide and the results are reproduced in figure 13.1 A. Later in 1975 Gray et al. (1975a) produced the first flow karyotype derived from a human cell line which is shown in figure 13.IB. By today's standards the human data set shown in this figure is not very impressive; however, this heralded the start of a new area of research and since those initial reports there have been incredible technological and preparative advances. The major technical developments have been made at the Lawrence Livermore and Los Alamos biomedical laboratories but other groups have made very significant contributions. It is now possible with flow cytometry to assay not only for total DNA but also for base composition, centromeric index, banding patterns and chromosome associated proteins.
13.1
Harvesting mitotic cells
Chromosomes are easiest to harvest from tissue culture adapted cells growing as a monolayer. The culture is treated with colcemid for about one cell cycle time to enrich the metaphase fraction and these are harvested by mitotic selection (Teresima and Tolmach, 1963) as described in section 11.5.2. More
HARVESTING MITOTIC CELLS
289
9000 -
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4500 -
1.0
Fluorescence intensity
Figure 13.1. Panel A shows the flow karyotype of M3-1 Chinese hamster cells clone 650A and panel B shows the karyotype derived from a human cell line redrawn from Gray et al. 1975b (A), 1975a (B). difficulty is encountered with suspension cultures as it is not possible to positively select for the mitotic fraction as with monolayers. However, even ficol-paque enriched peripheral blood lymphocytes, stimulated to divide by PHA (T-cells) or LPS (B-cells) and treated with colcemid can give a very workable chromosome: intact nuclear yield. Following cell lysis to release chromosomes (see below) any debris, clumps and intact nuclei can be removed to some extent by sedimentation through a 10—50% glycerol linear concentration gradient (Gooderham and Jeppeson, 1983; Fantes et al., 1989) or a 20-40% sucrose gradient (Wray, 1973).
290
CHROMOSOMES
13.2
Chromosome preparation
The ideal preparation method would produce chromosomes in fluid suspension with no chromosomal fragmentation or clumping and no intact nuclei. In practice, even with the best procedures, there is frequently some fragmentation, occasional clumping and some intact nuclei. Chromosomes are liberated from the metaphase enriched population by combinations of hypotonic solutions, detergent treatment and mechanical shearing. The latter has included syringing through fine-gauge needles (Gray et al, 1975a,b; Yu et al, 1981), the use of mechanical homogenizers (Sillar and Young, 1981), vigorous vortexing (Young et al, 1981) and sonication. These procedures can also damage chromosomes but this can be minimized by addition of polyvalant cations or reducing agents (Blumenthal et al, 1979; Sillar and Young, 1981). The shearing vigour required to disrupt the external cell membrane depends to some extent on cell type. Fibroblasts which have 'tougher' membranes than lymphoblastoid cell lines and lymphocytes require the more vigorous shearing (Langlois et al, 19SO; Stohr et al, 1982; Stewart et al, 1985) but, this has to be evaluated for each cell type (Gray and Langlois, 1986). 13.2.1 Hexylene glycol This was the first chromosome isolation technique to be used in flow cytometry and was based on that of Wray and Stubblefield (1970). The harvested mitotic cells were first suspended in hypotonic KC1 (75 mM) at 4 °Cfor 30 minutes then resuspended and lysed by mechanical shearing in 1.0 M hexylene glycol (2-methyl-2,4-pentanediol) and 1 mM CaCl2 in PIPES buffer, pH 6.7. The latter was composed of 10 mM piperazine-N,N"-bis(2-ethane sulphonic acid) monosodium monohydrate plus 10 mM PMSF (phenylmethylsulphonylfluoride). The presence of the divalent cations (Ca2 + ) stabilizes the chromosomes and analysis of both histone and non-histone proteins shows minimal alterations following this isolation method (Wray and Wray, 1979, 1980) which also yields high molecular weight DNA (Yu et al, 1981). A variation on this theme has been used by Sillar and Young (1981) where cells were resuspended in a buffer containing 0.75 M hexylene glycol, 25 mM trisma base, 0.5 mM CaCl2 and 1.0 mM MgCl2, pH 7.5, for 10 minutes before disruption with an MSE homogenizer. Chromosomes from a number of cell types including fibroblasts, lymphoblastoid cells and various tumour cell lines have been obtained by this method. It also has the advantage that the chromosomes are not contracted and they are suitable for banding pattern analysis following staining and sorting (Gray et al, 1979).
13.2.2 Polyamine This method involves treating the mitotic cells with hypotonic buffer containing 15 mM Tris-HCl, 0.2 mM spermine, 0.5 mM spermidine, 2 mM EDTA, 0.5 mM EGTA, SO mM KC1, 20 mM NaCl and 14 mM p-mercaptoethanol, pH 7.2. After washing and resuspending in the same buffer the detergent digitonin is added to a final concentration of 0.1% and the suspension is then subjected to
CHROMOSOME PREPARATION
291
vigorous vortexing (Sillar and Young, 1981, modified from Blumenthal et al, 1979). This method can be used with most DNA fluorochromes if divalent cations are added during the staining procedure (Lalande et al, 1985) and again high molecular weight DNA is obtained (Blumenthal et al, 1979). However, it suffers from the disadvantage with ethidium bromide staining that the chromosomes are very contracted and are not suitable for subsequent banding (Davies et al, 1981; Buys, Koerts and Aten, 1982).
13.2.3 Hypotonic PI detergent The double-helical structure of DNA is normally in an 'extended7 form as the negatively charged phosphate residues of the sugar—phosphate backbones on the outsides of the helix exert mutually repulsive electrostatic forces as the phosphates are in relatively close apposition. The phenenthridinium dyes, ethidium bromide and propidium iodide, intercalate with the double helix such that their linked tricyclic ring structures (see figure 11.4) 'slot-in' between, and parallel to, the bases positioned in the center of the helix. The positive charges of the dyes then neutralize the negative charges of the phosphates and the helix compacts along its length. Propidium iodide is more efficient than ethidium bromide in this respect as it has two positive charges as opposed to just one. This property has been exploited by Aten, Kipp and Barendsen (1980), Buys et al. (1982), Bijman (1983) and Kooi et al (1984) to stabilize the DNA of chromosomes during hypotonic detergent lysis. Metaphase cells were first treated with hypotonic KCl containing propidium iodide then triton-X 100 was added and the cells were syringed. The chromosomes so produced gave high molecular weight DNA (Yu et al, 1981) and were suitable for subsequent banding. There is also the advantage that the stabilizing agent, propidium iodide, is the DNA fluorochrome which is fine if you want a measure of total DNA per chromosome. If, however, you want to use a different stain then non-fluorescent stabilizing agents, e.g. psoralen derivatives (Yu et al, 1981), have to be used.
13.2.4 Ohnuki buffer This buffer enables chromosomes to be prepared in elongated form whilst preserving their morphology (Ohnuki, 1965, 1968). It has been used by Bartholdi et al (1989) to produce banding analysis by slit-scanning (see section 13.5.2). Metaphase cells are suspended in the hypotonic buffer comprised of an equimolar solution of 55mM KCl, NaNO 3 and NaC 2 H 3 O 2 in a ratio of 10:5:2 (Ohnuki, 1965). Following swelling the cells are treated with the polyamine isolation buffer described in section 13.2.2.
13.2.5 Magnesium sulphate An isolation technique which is suitable for many DNA stains and chromosomes from various cell types, including hybridomas, human amniotic cells and chorionic villus biopsies (Trask et al, 1984) has been developed by van den Engh et al (1984, 1985). The mitotic cells were resuspended in hypotonic MgSO 4 containing dithioerythritol and triton X-100 prior to syringing.
292
CHROMOSOMES
13.3
Staining
All of the DNA specific stains and the phenanthridinium dyes have been used for total DNA staining of chromosomes. The former group has the potential disadvantage that UV excitation is required but this constitutes no problem for mercury arc lamp based systems or those with a laser tunable to UV lines.
13.3.1 Total DNA Comparative studies of the UV excited ligands, DAPI, DIPI and Hoechst stains have been carried out by Otto and Tsou (1985) and CVs between 2.2% and 2.9% were obtained. Overall the best results were obtained with DAPI with the lowest CV and a brightness only 3% less than DAPI. Hoechst 33342 gave the worst results in these experiments with a CV of 2.9% and a brightness 14% less than DAPI. However, all these stains gave the same number of chromosome peaks with chinese hamster chromosomes. Chromomycin A 3 has been used as a single DNA stain in slit-scan studies (see section 13.5) but there is considerable overlapping of the human chromosomes with only eight well-defined peaks being obtained. These are shown in figure 13.2 which is redrawn from Bartholdi et al. (1989). The polyamine/ethidium bromide method developed by Sillar and Young (1981) would seem to have a number of advantages as the dye/DNA complex is 100
X,8-12
Chromomycin fluorescence
1024
Figure 13.2. Human karyotype stained with chromomycin A 3 in which only eight major peaks can be defined.
STAINING
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exited by the most frequently used 488 nm argon line, many of the chromosomes are resolved uniquely, ethidium bromide is relatively inexpensive, the method is very reproducible, it can be performed readily on a regular cell sorter (Young et al, 1981) and chromosomal DNA suitable for cloning and library generation can be obtained (Davies et al, 1981, and see figure 6.6). Figure 13.3 shows two karyotypes from peripheral lymphocytes of the same individual assayed six months apart (redrawn from Young et al, 1981). However, as can be seen from figures 6.6 and 13.3 not all chromosomes can be resolved with this method. There is complete overlap of the 9—12 group, considerable overlap of the 13—15 group and frequently pairs of the smaller chromosomes cannot uniquely be resolved.
13.3.2 A-T:G-C composition A dual staining technique was developed at Lawrence Livermore Laboratories using a dual-beam system (Dean and Pinkel, 1978) to excite chromosomes stained with chromomycin A 3 and Hoechst 33258 (Carrano et al, 1979; Langlois et al, 1982). These dyes bind independently to DNA with chromomycin A 3 showing G—C specificity and Hoechst 33258 exhibiting A—T specificity (see section 11.1). The Hoechst dyes are excited by UV light and chromomycin A 3 is excited by mid blue light (458 nm argon line) but not by UV. The UV excited emission from Hoechst 33258 overlaps the absorption spectrum of chromomycin A 3 and the fluorescence energy from the Hoechst 33258/DNA complex undergoes resonant energy transfer to the chromomycin A 3 (Langlois et al, 1980). Thus, by arranging for the double-stained chromosomes to pass first through the UV beam and then through the 458 nm beam we get two flashes of fluorescent green light. The first is due to UV energy absorbed by the Hoechst 33258 bound to A—T rich sequences which is then energy transferred to chromomycin A 3 and the latter emits green fluorescence in direct proportion to A-T content. When the chromosome subsequently passes through the 458 nm excitation beam the energy is absorbed directly by chromomycin A 3 bound preferentially to G-C rich sequences and the second flash of green fluorescence is directly proportional to G-C content. The processes involved in this technique are shown diagramatically in figure 13.4 and figure 13.5 shows a bivariate karyotype produced by this method and redrawn from Langlois et al. (1982) where Hoechst 33258 dependent fluorescence is plotted on the ordinate versus chromomycin A 3 on the abscissa. The left panel shows the whole distribution and the right panel is a 'magnified' view of the smaller chromosomes. The 9—12 group still remains a single cluster but the remainder have largely been resolved and figure 13.6 shows a statistical summary of the positions of the peaks of the chromosome distributions from a study of 10 normal individuals.
13.3.3 Bromodeoxyuridine We saw earlier (section 11.5.5) that fluorescence from Hoechst dyes is quenched by bromodeoxyuridine incorporation into DNA (Latt, 1977). However, fluorescence from chromomycin A 3 is slightly enhanced (Swartzendruber, 1977)
Fluorescence intensity Figure 13.3. Human flow karyotype prepared by the polyamine/ethidium bromide method from Young et al., 1981. The two panels were obtained from the same individual with an intervening interval of six months. There are three peaks on the far right where usually there is only one with this staining method (compare with figure 6.6). The peaks labelled IA and IB represent heteromorphism of the centric heterochromatin in the chromosome.
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458nm beam detector Collecting lens
UV beam detector Double stained chromosomes
458nm beam Figure 13.4. Sequential excitation of Hoechst 33258; chromomycin A 3 stained chromosomes with first the UV beam and second the mid-blue beam. The Hoechst 33258: DNA complex is excited on passing through the UV beam and the absorbed energy is transferred to chromomycin A 3 which emits fluorescence in proportion to A—T content. The chromomycin A 3 is excited directly on passing through the mid-blue beam and this same dye then emits fluorescence in proportion to G—C content.
oo
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Chromomycin Figure 13.5. Bivariate karyotype produced by dual laser excitation and double staining with Hoechst 33258 (ordinate) and chromomycin A 3 (abscissa). The whole karyotype is shown on the left and 'magnified' view of the smaller chromosomes on the right. Note that almost all the chromosomes are completely resolved apart from the 9—12 group. Redrawn from Langlois et al, 1982.
CHROMOSOMES
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Chromomycin 13.6. Statistical summary of the chromosome peak positions from ten individuals with the Hoechst: chromomycin technique. Small ellipses (chromosomes 2, 7, 8, 9—12,18 and 20) indicate little variation. In contrast chromosomes 14 and 15 exhibit fairly large variability in position from individual to individual.
just as with ethidium bromide. These properties can be used to study the times in S-phase at which different chromosomes are replicated (Cremer and Gray, 1982, 1983) and two approaches can be employed. Firstly, monolayer cells can be synchronized by mitotic selection. Different aliquots of cells would be flash labelled with BrdU for one hour at different times during the cell cycle and treated with colcemid to harvest metaphase cells on the first pass through mitosis after taking up the analogue during S-phase. Chromosomes which were replicated during the interval that BrdU was present would then exhibit a partial loss of Hoechst related fluorescence and a slight gain in chromomycin A 3 fluorescence. It was stated in section 11.5.5 that flash labelling with BrdU produced insufficient quenching of Hoechst 33342 fluorescence to make a reliable distinction between cells which had replicated their DNA during the labelling interval and those that had not (see figure 11.30). However, the position is somewhat different for individual chromosome analysis. In the former case an attempt is being made to assay for Hoechst quenching in whole nuclei within a background where the majority of DNA has not incorporated BrdU. In the latter case the majority of replicated DNA within a given chromosome will have incorporated the analogue if that chromosome was being replicated when the label was present. The second approach would use asynchronously growing cultures and BrdU would be added for intervals of one hour at increasing times before addition of
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colcemid and harvesting the metaphase cells. Thus, if the interval between BrdU labelling and addition of colcemid and harvesting mitotic cells was short we would be observing chromosomes replicated late in S-phase. If the interval between labelling and colcemid was successively increased we would be observing chromosomes replicated earlier and earlier in S-phase.
13.3.4 Partial sequence specificity A number of non-fluorescent minor groove ligands (Baguely, 1982; Zimmer and Wahnert, 1986; Smith, Debenham and Watson, 1989) with A-T specificity, including distamycin and netropsin, can compete for Hoechst dye binding sites (Meyne et al, 1984; Lalande et al, 1985). However, even though they have A—T specificity they also have specific sequence specificity (Lane, Dabrowiak and Vournakis, 1983; Martin and Holmes, 1983; Scamrov and Beabealashvilli, 1983; Van Dyke and Dervan, 1983a,b). Thus, the non-fluorescent minor groove ligands will compete for Hoechst dye binding sites and reduce its fluorescence in preferred A-T regions where the flanking sequences are most conducive to their binding. Such non-fluorescent ligand/Hoechst dye combinations have been used by Sahar and Latt (1978, 1980) and Latt et al. (19&0a,b) to identify polymorphic regions in human metaphase spread chromosomes which contain highly repetitive DNA sequences. This method has been applied in flow cytometry to identify chromosomes 9 and 15 which have long stretches of DNA which bind Hoechst dyes but do not bind netropsin or distamycin (Meyne et al, 1984; Lalande et al, 1985). Thus, these two chromosomes have very little reduction in their Hoechst fluorescence but the remainder exhibit considerable reduction which enables the distinctions to be made.
13.3.5 Chromosome-associated proteins A very brief summary of some of the nuclear proteins was given in section 12.3. The non-histone nuclear structural proteins also contribute to the chromosome skeleton in metaphase with loops of chromatin 'pegged' to the central scaffold, a concept originally proposed by Adolph, Cheng and Laemmli (1977), Paulson and Laemmli (1977) and Laemmli et al. (1978). More recently Earnshaw and colleagues have shown that the kinetochore (centromere) is part of the metaphase chromosome scaffold (Earnshaw et al., 1984). Moreover, Earnshaw and Heck (1985) and Earnshaw et al (1985) have shown that topoisomerase II is a structural component of the scaffold and have demonstrated its central location in mitotic chromosomes using immunofluorescence. As yet, little work has been carried out in flow cytometry to assay for metaphase chromosome proteins as opposed to nuclear-associated proteins. However, extensive studies have been carried out using immunocytochemical techniques to study nucleosome heterogeneity, visualize the presence of histones in transcriptionally active chromatin and isolate DNA sequences associated with specific chromosomal proteins (Bustin, 1987) and considerable potential exists in this area for both flow and image cytometry. Our group have used similar techniques to those of Earnshaw and Heck
298
CHROMOSOMES
Hoechst fluorescence Figure 13.7. A mixture of human chromosomes (Hi, H2, H3 and H4) and Chinese hamster chromosomes (Cl, C2, C3 and C4) double stained for DNA with Hoechst 33258 and human histone H2B with FITC immunofluorescence. The human chromosomes stained with greater intensity on the immunofluorescence
to assay for topoisomerase II in whole nuclei (see figure 12.5 and Epstein, 1988; Epstein et al, 1989) and there seems no reason why this could not also be extended to chromosome analysis. Flow cytometric methods have been developed to assay for histone proteins using immunofluorescence (fluorescein) simultaneously with DNA Hoechst fluorescence and an example from Trask et al. (1984) is shown in figure 13.7. A mixture of Chinese hamster and human chromosomes was used which were probed with an antibody raised against human histone H2B. Fluorescein immunofluorescence is plotted on the ordinate versus DNA on the abscissa and the human chromosomes labelled with greater intensity compared with the hamster chromosomes. Autoantibodies which recognize centromeric structures have been found in the sera of patients with scleroderma (Moroi et al, 1980) and Earnshaw and Rothfield (1985) have identified a family of human centromeric proteins using autoimmune sera from patients with scleroderma. Recently, the gene encoding the major human centromeric autoantigen has been cloned (Earnshaw et al, 1987). Dicentric chromosomes have two centromeres and Fantes et al (1989) have been developing methods to assay for such chromosomes following radiation damage using immunofluorescence flow cytometric methods with sera from patients with proven autoimmune disease.
FLOW KARYOTYPE ANALYSIS
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13.3.6 In situ hybridization All the chromosome staining techniques described above are assaying small, or relatively small, differences between chromosomes to effect a discrimination and very high precision instrumentation, preparation and staining is required. In spite of the sophistication developed over the last 15 years the 9—12 group still defies unique identification. However, all chromosomes have unique DNA sequences which could be identified with in situ hybridization using cDNA probes. Considerable work has been carried out in this area with chromosomes and nuclei attached to slides and Nederlof et al. (1989) have been able to perform triple colour fluorescence in situ hybridization to detect multiple nucleic acid sequences. However, these methods are not yet applicable to chromosomes for flow analysis though Trask et al. (1985) have performed in situ hybridization in whole nuclei in suspension. In situ hybridization techniques for flow analysis are going to be difficult to perfect, but I believe they will be perfected in the not too far distant future and judging by the speed of events in this field it would be a brave (or foolhardy) person who believes otherwise.
13.4
Flow karyotype analysis
Analysis of flow karyotypes involves calculating the relative area under each peak in univariate histograms and the relative volumes of the peaks in bivariate data sets. For example the normal flow karyotype should have 4.348% (^-) of the whole distribution under each unique autosomal peak, the same value under the X chromosome peak in the female but 2.174% under both the X and Y chromosomes in the male. The composite 9—12 peak should comprise 17.392% of the whole distribution. 13A.I
Univariate Analysis of monodimensional histograms of the types shown in figure 6.6 and 13.3 is carried out by fitting multiple Gaussian distributions to the various peaks in the histogram. The equation used in the fitting procedure (Gray and Langlois, 1986) is shown below. g(x)=Yj(0.3989xAi/(ji)
x exp(-0.5 x { ( j - /
i
This may look a little fearsome to the majority of biologists but really, it's fairly simple. However, if you do find it unintelligible it's only because you are not familiar with the nomenclature, and I'll try to explain. If you insist that you have a maths phobia and can't face this you had better skip the next section as well and go on to slit-scanning. If you know all about these things you shouldn't be reading either this or the next section so you too should go on to slit-scanning. So, you're going to give it a try, take a deep breath. There is a total of i separate distributions in the experimental data, each one corresponding to a particular
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chromosome. If all chromosomes were uniquely resolved i would equal 23 in the female and 24 in the male. In practice, due to overlapping, e.g. 9—12, the value of / is less than the theoretical maxima. Aif ot and ft are the area, standard deviation and mean respectively of the /th peak. The expression exp{ — 0.5 x [(x — ft)/ad 2} is the curve which describes the normal distribution and 0.3989 x A-JCi is a constant which normalizes the /th distribution to unity with A{ being the scaling factor for the /th peak. The numerical value 0.3989 is equal to 1/^/(2 x TC). The x is the channel number on the X-axis (fluorescence intensity) of the whole distribution and the symbol Z with its / subscript represents the summation of the contributions of all the / theoretical distributions to that particular channel x. This is denoted by g(x). The expression d(x) represents a continuum which is added to the whole of the theoretical function to approximate any background noise underlying the peaks in the experimental data. The value of / can usually be fixed by inspection of the experimental data and the / values for A, a and \i are varied until the best fit between the theoretical data, g{x), and its corresponding experimental data, f(x), in each channel is found. 13.4.2 Bivariate Analysis of bivariate data in principle is no more complicated than univariate. The mathematical notation is just extended to the two dimensions simultaneously assuming that Gaussian distributions can be fitted in both dimensions and the notation is as follows,
C{x,y)= £ where N is the number of peaks, C(x,y) is the theoretical frequency at the location (x,y) and where the function Gi(x,y) is dependent on the correlation coefficient, p, between x and y, and the means and standard deviations in both the x and the y direction and the volume under each peak. I'm not giving the full expansion of this function here, if you want it you will find it in Cytometry by Dean, Kolla and van Dilla (1989) but it is interesting to note that it was used during the last war. The probability of hitting an aeroplane with a shell is Gaussian distributed in both the x and y directions and a 'correlation coefficient' dependent on the angle of the aeroplane's vector with respect to the position of the gun. The above mathematical function was used to calculate the number of shells required to hit the target at a given height and velocity. It turned out that the theory predicted far fewer shells to obtain a hit than was observed in practice. Then some bright spark realized that this was a three-dimensional problem as the altitude of the plane could not be calculated exactly and the function was extended to three dimensions with the Z-axis (altitude) being added. Theory now predicted that more shells would be required but it was still an underestimate of the reality as just hitting the plane was not always sufficient to bring it down. Some hits were 'non-lethal'.
SLIT-SCANNING
13.5
301
Slit-scanning
The principles involved in slit-scanning were described in chapter 8 and figure 8.2 showed an example of chromosome slit-scanning from Lucas and Gray (1987). 13.5.1 Centromeric indices The centromeric index is the relative position of the centromere along the length of a given chromosome and flow cytometric calculation of this parameter was introduced by Lucas et a\. (1983). Inspection of the slit-scans in figure 8.2 reveals that the centromeric index can be calculated with confidence for only four of the profiles, namely those labelled 2, 4, 5 and 8. In these studies total DNA was measured by propidium iodide fluorescence from human chromosomes after isolation with the hypotonic PI technique and these were then slit-scanned in the object plane with a 1.3 |im 488 nm argon beam. The fluorescence intensity profile
0.90
0.80
_ Y,21,22 -
x
0.70 -
E o
o
0.60 -
0.50 -
2
3
4
DNA fluorescence Figure 13.8. Slit-scan centromeric index (ordinate) versus total DNA (abscissa). The contours of the smaller chromosomes to the left of the dashed line were drawn at different levels compared with those on the right. The squares represent the centromeric indices derived from positively identified chromosomes in human/rodent hybrid cell lines.
302
CHROMOSOMES
of each chromosome was digitized at 20 ns intervals with a model 8100 Biomation waveform recorder as it passed through the exciting light. The data were transferred to computer and the centromeric indices were calculated and plotted on the ordinate versus total DNA content on the abscissa as shown in figure 13.8, which again is redrawn from Lucas and Gray (1987). The peaks from the smaller chromosomes to the left of the dashed line were drawn with different contouring levels than those on the right. The squares within the contours were the data from positively identified human chromosomes in human/rodent hybrid cell lines. The feature of these data is the encouraging separation of the 9-12 group which is not resolved with PI alone or with the Hoechst/chromomycin dual-staining technique. Moreover, the distinct possibility exists that even better resolution will be obtained with the dual-staining method in conjunction with slit-scan centromeric index determination. 13.5.2 Banding Similar types of techniques are being developed at the Los Alamos laboratories to identify human chromosomes by banding patterns (Bartholdi et al., 1989) using a cytometer to record simultaneous waveforms (Johnston et al., 1985). This uses image plane slit-scanning, as opposed to object plane, but it also uses a model 8100 Biomation waveform recorder digitizing at 20 ns intervals. Human chromosomes were prepared from metaphase cells treated in Ohnuki's buffer then released using the polyamine method and stained with chromomycin A3. This stain produces low-contrast R-banding (Sahar and Latt, 1978; Schweitzer, 1976, 1981; van de Sande et al, 1977) similar to that of acridine orange (ISCN, 1985). A typical chromomycin flow karyotype from Bartholdi et al. (1989) was shown in figure 13.2 in which eight major peaks could be resolved on total chromomycin fluorescence. Chromosomes 1-3 were each identified as a single peak and their slitscan profiles were relatively easy to identify and correlated well with the acridine orange R-banding. None of the remaining chromosomes could be resolved uniquely on total chromomycin fluorescence and no clear waveform profiles could be identified which corresponded to R-banding of the smaller chromosomes, 13—22. However, profiles were found in the 4—7 and X,8—12 peaks which corresponded reasonably well with the R-banding patterns of these chromosomes. At present it is not possible to sort chromosomes for positive identification on either centromeric index value or banding pattern. Centromeric index calculation is the simpler of the two to express as a single number and requires between 50 and 100 ms computing time (Lucas and Gray, 1987). However, sorting would require this to be reduced by two orders of magnitude and the current generation of computers, fast as they are, are simply no match for this problem which is further compounded for banding pattern analysis. In the latter there are multiple peaks and troughs in the waveform profile as opposed to just one for centromeric index calculation. It is not yet clear how the data contained in the waveform profile are going to be reduced to the information of a unique single number which would be required in the current generation of sort decision electronics.
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$03
13.6 High-speed sorting No chapter on flow cytometric chromosome analysis can fail to mention the high-speed sorter developed initially at Lawrence Livermore (Peters et al, 1985; Gray et al, 1987) which is a phenomenal example of modern bio-technological instrumentation. Attempts are beind made to clone, map and understand the whole human genome which is composed of about 109 DNA bases encoding 0.5-1.0 X 106 genes. This 'human genome project' (Caskey, 1986) is a simply monumental task which will be facilitated considerably by the availability of DNA purified from individual chromosomes. Chromosome sorting can be carried out with ease using conventional instruments for identification purposes, but the time taken to obtain workable microgram quantities of sorted DNA is prohibitive. As an example let us take the Y chromosome and suppose that 1 jig of DNA is needed. This chromosome contains approximately 10 ~ 13 g of DNA and the total throughput rate of a standard sorter is about 1000 chromosomes s~ l for the highresolution analysis that is needed. However, only about 2% of the total chromosome complement is Y, thus 20 chromosomes will be sorted per second which is 2 pg and we need 1 |ig. It's not too difficult to appreciate that this would take half a million seconds which is about 140 hours and this assumes that everything (instrument, chromosome preparation and all the rest of the paraphernalia) is working perfectly all the time. The LLNL-HiSS (LLNL stands for Lawrence Livermore National Laboratory and HiSS stands for high-speed sorter) was developed to reduce sorting times by about one order of magnitude. It operates with a jet velocity of 50 m s ~ l compared with 1 0 m s " 1 in regular instruments, a sample pressure of 200 psi compared with 15-20 psi and a droplet production frequency of 215 000 per second compared with 30 000—40 000 whilst maintaining the analytical resolution required, an amazing achievement.
13.7 Applications The uses of flow cytogenetics are being developed for diagnosis, gene mapping, cDNA library production and radiation dosimetry. Arguably, the most exciting developments are in the areas where there is an absolute requirement for flow cytometry, namely the generation of chromosome specific libraries.
13.7.1 Diagnosis Many diseases are genetic in origin. Perhaps the best understood examples are the haemoglobinopathies thalassemia (Orkin et al, 1979; Little et al., 1980) and sickle cell anaemia (Orkin et al, 1978) where restriction site polymorphism analyses of the globin loci (Jefferys, 1979) have formed the basis for diagnosis of variants. Further well recognized genetic anomalies with gross chromosomal abnormalities include duplications, deletions and translocations. Kleinfelter's syndrome (XXY), the XYY mosaic associated with psychopathic
304
CHROMOSOMES
Figure 13.9. Isometric hidden line elimination plots of hoechst versus chromomycinfluorescenceversus frequency for a normal female, panel A, and a female with trisomy 21 (Downs syndrome), panel B. Note the increased volume of peak 21 in panel B which is clearly apparent in spite of the somewhat higher background which partly underlies peak 21 in panel A. disorders and Patau's, Edward's and Downs syndromes, respectively associated with trisomies of 13, 18 and 21 are all examples of chromosomal duplications. Turner's syndrome (X0) represents a Y deletion and Burkitt's lymphoma and chronic myeloid leukaemia are associated with t(8:14) and t(9:22) translocations respectively. Conventional chromosome banding analysis is carried out in the diagnosis of suspected cases and this is being extended to small amniotic samples using flow cytometric methods (Gray et al, 1988). An example from Gray and Langlois (1986) is given in figure 13.9 which shows trisomy-21. Techniques such as these can be readily adapted to genetic anomaly screening programs where the specific abnormality is known. However, it is also important to determine the degree of variation within the normal population. An example of a normal variation was shown in figure 13.3 where there are three peaks, namely 1A, IB and 2, on the far right. Usually, chromosomes 1 and 2 occupy the same peak with this particular staining method but this idividual exhibited heteromorphism of the centric heterochromation of chromosome 1 which was confirmed by G- and C-banding (Young et al, 1981).
13.7.2 Genomic libraries Until 1981 most chromosome-specific genomic libraries had been produced from human/rodent hybrid cell lines (Gusella et al, 1980; Olsen, McBride and Otey, 1980; Schmeckpeper et al, 1979). In 1981 Davies et al produced the first library from a flow cytometry sorted chromosome and they derived 50 000 recombinants representative of the human X chromosome and it
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305
was their data which were used as the illustration in figure 6.6. This was followed by similar work from Krumlauf, Jeanpierre and Young (1982) who produced libraries from chromosomes 21 and 22. In the next two years libraries were constructed from chromosomes 1 (Kanda et al, 1983), 13 (Lalande et al, 1984a) and X (Lalande et al, 1984b) then the flood gates opened. By the end of 1986 Scambler et al. (1986) and Donlon et al. (1986) had produced libraries derived from chromosomes 7 and 15 respectively and the National Laboratory Gene Library Project of the USA, a joint venture by Lawrence Livermore and Los Alamos Laboratories had produced libraries from all 24 human chromosomes (Deaven et al, 1986; van Dilla et al, 1986; Fuscoe, Clark and van Dilla, 1986).
13.7.3 Gene mapping Unique sequence DNA in the form of a cDNA probe with incorporated radioactivity or a fluorescent tag can be hybridized to chromosomes to locate not only the chromosome containing that sequence but also the hybridization site on the chromosome. Hence, a probe (gene) map in relation to chromosome bands can be built up. In the study by Krumlauf et al. (1982), in which sorted chromosomes were used to generate probes, it was found that 90% of the single-copy clones derived from chromosome 22 hybridized to chromosome 22 and 10% to chromosome 21. In view of the proximity of chromosomes 21 and 22 on the histogram (see figures 13.3 and 6.6) and the early stage in the development of the staining technique used to sort these chromosomes (Sillar and Young, 1981) this must have been a gratifying result. One of the first reports of flow cytometry being used to assist in gene mapping is due to Lebo et al (1979) where the p-, y- and 5globin genes were assigned to the short arm of chromosome 11 by sorting coupled with restriction analysis. Lebo et al. (1984) have mapped McArdle's syndrome, a rare genetic defect resulting in myopathy due to enzymic deficiency of muscle glycogen breakdown, to chromosome 11 and the insulin gene to the short arm of this chromosome (Lebo et al, 1982). A very direct and interesting approach to gene mapping is afforded by cell lines containing chromosomal break points and translocation in the vicinity of the gene being mapped (Bernheim et al, 1982; Lebo et al, 1984; Collard et al, 1985; Harris et al, 1986). This operates as follows. The c-myb oncogene had been localized to chromosome 6 between bands q22 and q24 (6q22-q24) by in situ hybridization (Harper et al, 1983). Collard et al (1985) then used a primary teratocarcinoma cell line in which there were translocations involving chromosomes 6 and 11. There were two break points on the number 6 chromosomes, at 6q21 on the first of these and at 6q23 on the second and one break point on one of the number 11 chromosomes, at I l q l 3 . The shorter chromosome 6 fragment (6q23—qterm) was translocated to the chromosome 11 break point. The longer chromosome 6 fragment (6q21—qterm) was translocated to the 6q23 break point of the second number 6 chromosome which now had 6q21 to 6q23 duplicated. Finally, the (ql3-qterm) fragment of chromosome 11 was translocated to the 6q21 break point site of the first number 6 chromosome. A diagramatic summary of these
306
CHROMOSOMES Chromosome 6
Chromosome 11
q13"
q21
q23-
Figure 13.10. Chromosome banding analysis of translocations in chromosomes 6 and 11 of a teratocarcinoma cell line. The top panel shows the normal chromosomes with the break points in the teratocarcinoma cell lines indicated by the arrows. Both chromosomes 6 were cleaved at q21 and q23 respectively and one chromosome 11 was cleaved at ql3. The middle panel shows the rearrangements with the 6q21—qterm fragment being translocated to the q23 break point on the second chromosome 6. The 6q23—qterm fragment from the latter translocated to the ql3 break point of chromosome 11 and the
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307
13-16+11/6
9-12
o 4) 0)
21
DNA Fluorescence Figure 13.11. Flow karyotype from the teratocarcinoma where both of the chromosome 6 translocations show a net gain in DNA. The tit translocation appears with chromosome 3, the 6/11 translocation with chromosomes 4 and 5 and the 11/6 translocation, which has lost DNA, has moved out of the 9-12 peak and appears in the 13—It group.
Figure 13.10 (cont) Ilql3-qterm fragment from 11 translocated to the q21 break point of the first number 6 chromosome. These translocations, 6/11, tit, 11/1 are depicted in the bottom panel together with the normal chromosome 11. The identical repeat segments of the tit translocation are indicated by the arrows. This figure was abstracted from the work of Collard et al.r 1985.
308
CHROMOSOMES
translocations is shown in figure 13.10. Hence, if c-myb was located in the (6q23—qtrem) fragment one copy of the gene would appear on chromosome 11, the 11/6 translocation, and the second copy would appear on the second chromosome 6, the 6/6 translocation. If, however, c-myb was located between 6q21 and 6q23 the gene would be deleted from the first number 6 chromosome and both copies would appear on the second number 6 and it would not be present on 11. The flow karyotype of this cell line which is shown in figure 13.11 revealed a reduced area under the 9-12 group as the 11/6 translocation, had considerably less DNA (see figure 13.11) and this now appeared in the region of the 13-16 chromosome group. Similarly, both chromosomes 6 had more DNA than normal. The 6/6 translocation appeared in the same peak as chromosome 3 and the 6/11 appeared with chromosomes 4 and 5. A total of 60 000 chromosomes from each of these peaks were sorted directly onto nitrocellulose filters and were hybridized with the c-myb probe and only chromosomes from the 3 + 6/6 peak gave a positive signal. Thus the gene had to be located in the q21—q23 repeated region of chromosome 6/6. The previous study had mapped this gene to (6q22—q24) and combination of these two results assigns c-myb to 6q22—q23.
13.7.4 Radiation bio-dosimetry Radiation induces a large number of chromosomal anomalies which are dose dependent. However, not all cells will exhibit detectable changes, which applies particularly at low doses and, furthermore, the changes in affected cells will not be uniform. Flow karyotype analysis is an attractive approach to detecting low-dose environmental radiation exposure as large numbers of chromosomes can be analysed rapidly but even with flow we run into the problems of rare-event analysis. One approach is to assess radiation-induced alterations in the karyotype which include broadening of the peaks and an increase in the underlying background continuum (Otto and Oldiges, 1980; Nusse and Kramer, 1984; Welleweerd et al, 1984). However, these types of end-point can be difficult to assess quantitatively. A second approach is the detection of specific chromosome anomalies, e.g. dicentrics, the frequency of which is dose dependent. Two methods are currently being evaluated for dicentric frequency assessment, namely the use of centromeric indices (Lucas and Gray, 1987), and immunocytochemical assessment of centromeric protein content which should be doubled in dicentric chromosomes (Fantes et al, 1989).
14 Dynamic cellular events
Time-dependent biological events monitored by flow cytometry have been studied almost since the technology was invented and examples of DNA histogram changes in populations of cells released from a synchronizing event giving cell cycle kinetic data were described in section 11.5.3. In these types of study the time-dependent biological reference frame is long and sampling the population at intervals of hours gives the required resolution and information. In this chapter the use of flow technology to study dynamic events within the temporal reference frame of a few seconds to minutes will be considered. The majority of such studies have been conducted in the general area of enzyme reaction kinetics, termed flow cytoenzymology (FCE) (Dolbeare and Smith, 1979; Watson, 1980a,b; Dolbeare, 1981; Watson, 1984), where the aim is to determine both the quantities and activities of enzymes in populations of single intact cells. However, similar techniques can also be used to determine rates of influx or efflux of molecules across the cell membrane, binding of ligands to intracellular constituents, and changes in intracellular calcium, pH and membrane potential in response to various stimuli. Total quantities of enzymes can be determined using antibodies (Coons et al., 1941) or fluorescently labelled tight-binding inhibitors (Gapski et al, 1975) and activities can be determined using various fluorogenic and non-fluorogenic substrates which yield fluorescent and light-absorbing products respectively. With increasing time after mixing cells with substrate greater quantities of either fluorescent or light-absorbing product are released within or on the cells of the population, and these can be monitored quantitatively with time. Flow techniques have important advantages over conventional biochemical and histochemical assays of enzyme activities, particularly as cells can be assayed under near physiological conditions. Artefactual results may be generated by the disruption of cellular and subcellular permeability barriers in the preparation of the cell-free extracts for conventional biochemical methods (Youdim and Woods, 1975). Quantitative data can be obtained with conventional methods using bulk samples, but heterogeneity within samples is completely masked by average values. Useful qualitative information regarding heterogeneous cell populations can be obtained by traditional histochemistry; however, the capacity for quantitative accuracy is extremely limited. Furthermore, histochemical procedures
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DYNAMIC CELLULAR EVENTS
are slow and certainly not ideal for collection of detailed dynamic biochemical data. With flow technology the enzyme activity of each individual cell in a sample is recorded by the cytometer. This results in the very important capacity to obtain distributional information for identification and quantitation of cell subpopulations differing in enzyme activities in a heterogeneous cell sample, including minority populations. The techniques are rapid, highly sensitive and good statistical precision is obtained. Another important advantage to flow cytometry over conventional methods is the capacity for multi-parametric analysis. Potential exists for measurement of multiple enzyme activities, multiple substrates (Watson, 1980a; Malin-Berdel and Valet, 1980), and enzyme activities simultaneously with other biologically and pharmacologically relevant cellular parameters such as DNA content, glutathione and oncoproteins.
14.1
Incorporation of time
Clearly, in order to measure the dynamics of reactions it is necessary to include time in the data base, and we will start with this, the most important single parameter for such studies and there are four methods available. 14.1.1 Discontinuous sequential sampling This is appropriate whenever the dynamic event under study is varying within a time frame of a few tens of minutes to hours. The population is sampled discretely at defined intervals after the initiating event and the measurements are made at those defined time intervals. Examples include mixing cells with substrate for enzyme kinetics of 'slow7 reactions and DNA histogram analyses after a synchronizing event to give cell cycle data. 14.1.2 Continuous interrupted sampling With this technique cells are mixed with substrate and the sample is introduced into the instrument as fast as possible. 'As fast as possible' in this context usually means a 'dead' time of about 20—30 seconds but if everything goes very well this can be reduced to a minimum of 15 seconds. The sample runs through the instrument continuously and the data acquisition computer is instructed to record for a defined interval, say 5 seconds, then to wait for a further defined interval, say 10 seconds, before recommencing data acquisition. The median of the distribution obtained within each 5 second recording interval can be printed out during the period when data are not being collected. The median values are then plotted against time to generate a reaction progress curve. This technique was introduced in flow cytometry over a decade ago to study the hydrolysis of fluorescein diacetate (FDA) by EMT6 cells (Watson et al., 1977) and some of these data are reproduced in figure 14.1.
INCORPORATION OF TIME
311
60-1
LU
u z
096
UJ
o UJ
O
•—-•
048
ID
°'24 TIME, MINUTES Figure 14.1. Hydrolysis of FDA (mM concentrations shown against each curve) by EMT6 mouse mammary tumour cells. (Watson et al., 1977).
14.1.3 Continuous time recording The continuous interrupted sampling technique introduced by Watson et al. (1977, 197S) had one major deficiency. The fluorescence from substrate hydrolysis was increasing during the recording interval; hence the distributions obtained during the recording interval were skewed to the right and the median values were overestimated. This was not a problem for 'slower7 reactions but it could be a severe limitation for 'fast' reactions. This was overcome very elegantly by Martin and Swartzendruber (1980) by incorporating time directly into the data base. Their initial method used a voltage ramp generator where the potential increased linearly with time and a recording of the voltage was made from the ramp generator each time a cell was analysed in the flow chamber. This method had one disadvantage, namely that time could only be recorded over an interval of about 15 minutes. However, immediately following the introduction of continuous time recording by Martin and Swarzendruber (1980) we incorporated the time stamp from the data acquisition computer directly into the data base. Hence, events were timed automatically with 50 ms resolution by the computer clock and this time, in the form of the number of clock 'ticks' (one tick per 50 ms), was recorded for each event analysed. Thus, unlimited time could now be recorded and an example of mouse bone marrow where cells were incubated with FDA is shown in figure 14.2 and four subsets labelled A, B, C and D can be defined.
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DYNAMIC CELLULAR EVENTS
Time—-• Figure 14.2. Contour plots of fluorescence from fluorescein diacetate hydrolysis versus computer clock time for mouse bone marrow where four subsets, labelled A, B, C and D are apparent.
14.1.4 'Stop—flow' cytometry in flow Each of the various methods described above suffers from a considerable disadvantage, which is the finite time taken between mixing cells with substrate or ligand and recording the first event. This 'dead time' is due to mixing, location of the containing vessel in the instrument, surge pumping the reaction mixture through the sample feed tube into the flow chamber, and restoration of stable flow. In our instrument the absolute minimum dead time is 15 seconds if everything proceeds smoothly, but more often this was about 20 seconds. There was a clear need to reduce this temporal delay, so as to facilitate the analysis of biochemical events taking place over the time period of a few seconds. Such a development would be valuable not only in flow cytoenzymology (e.g. for substrate diffusion kinetics, very rapid reaction and membrane enzyme analysis), but also for a variety of other biological applications involving very short time scales (e.g. drug uptake and ion flux analysis). Kachal, Glossner and Schneider (1982) described a flow chamber in which timeresolved measurements could be made within 1 second but this was not variable. Recently, we have developed a system which markedly reduces the temporal reference frame so that this can be varied within the interval 1 to 20 seconds (Watson et ah, 1988a, 1991a). The technique employs computer-controlled precision drive syringe pumps, one for substrate the other for cells, together with variable length tubing between a mixing chamber and analysis point, selected by an array of zero dead-space pinch valves. The different tube lengths at a given
INCORPORATION OF TIME
313
FCN
Figure 14.3. Schematic of 'stop-flow' device which allows kinetic measurements to be made during the first few seconds of a dynamic reaction. Pi and P2 = pumps 1 and 2; J = 4-way junction; PVA = pinch value assembly; FCN = flow chamber needle. pump flow rate give different times between mixing and analysis. A schematic of the system is shown in figure 14.3. Calibration was effected using two sets of microbeads with different fluorescence intensities (Polysciences Inc. Warrington, PA, USA). Pumps 1 and 2 were filled with beads of the higher and lower intensity respectively. The concentrations were adjusted to give a flow rate of 250 beads per second with both pumps running at 100 |il min" 1 . The concentration of beads in pump 2 (lower intensity) was about 1.4 times greater than in pump 1. Both pumps were activated before data collection in order to fill the input pipes to the mixing chamber, and they were then stopped. The chamber was then flushed through and pump 1 was restarted before data collection. Pump 2, containing the lower intensity beads, was started during the run after about 1500 of the 10 000 requested events had been recorded. This procedure was repeated for each tube length at various flow rates. Figure 14.4 shows fluorescence versus time data as frequency contour plots at the 3, 6 and 12 event levels with the fluorescence and flow rate histograms adjacent to their respective axes. The saw-tooth pattern of the flow rate histogram is caused by interruption of data collection due to time sharing on the PDP 11/40 computer which dumps the data to disk, displaying data on the screen between each buffer dump and checking the pump flow rates before recommencing data collection. These data were recorded with flow rates of 100 ul min" 1 from each pump and
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DYNAMIC CELLULAR EVENTS
TIME Figure 14.4. Fluorescence versus time data as frequency contour plots at the 3, 6 and 12 event levels with the fluorescence and flow rate histograms adjacent to their respective axes.
INCORPORATION OF TIME
-30
-20
-10
0
315
20 5 10 Tube Length, cm
Figure 14.5. Plots of time from mixing chamber to analysis point versus tube length for pump flow rates of 100, 150, 200 and 250 ul min" 1 .
panels A, B, C and D respectively were obtained for tube lengths of 5, 10, 20 and 40 cm. Full scale on the abscissa is 40 seconds, and each division on the ordinate represents 100 digitization steps. The long vertical lines drawn through each panel represent the time which is flagged in the data base when pump 2 was activated. The immediate flow rate increase is apparent and the sudden surge is also manifest by a widening of the distribution of the higher intensity beads. The short vertical lines show the time at which the beads from pump 2 first appeared in the data record. The interval between these lines represents the time for the lower intensity beads from pump 2 to travel from the mixing chamber to the analysis point. Plots of time from mixing chamber to analysis point versus tube length are shown in figure 14.5 for pump flow rates of 100, 150, 200 and 250 JLXI min~ \ The regression lines for these pump flow rates extrapolated almost to a common point and all the intersections are included in the region defined by the open circle shown in figure 14.5. Therefore, the four equations defined by the regression analyses were solved simultaneously to give a common intersection point with X and Y coordinates of —24.73 cm and 0.6 s respectively. This value of 24.73 cm represents the volume of the 'non-variable' (dead-space) section of the system which comprises an individual pair of arms of the four-way junctions, the flow chamber injection needle, the mixing chamber and its outflow. The volume of unit length of the tubing contained in the variable section was measured using
316
DYNAMIC CELLULAR EVENTS
0.25
\L°9e
SORT
LJJ O _l
0.15
CO
0.05-
4.6
5.0
5.5
Flow rate
10 SQRT Flow rate
15
Figure 14.6. The slopes of the four regression lines plotted against both the square root and the log of the respective flow rates. Regression analyses gave correlation coefficients of 0.9999 and 0.991 respectively. Hamilton syringe injection of eight different lengths. The average of the eight readings showed that 1.0 cm was equivalent to 1.046 pi. The volume of the dead-space, excluding the mixing chamber (18.1 pi), was measured (again by Hamilton syringe injection) to be 8.1 pi. Thus the total dead-space volume was 26.2 pi, which corresponds well with the theoretical value of 25.8 pi (24.7 cm X 1.046 pi cm" 1 ) represented by the intersection point in figure 14.5. The vertical displacement of the intersection point, 0.6 s, constituted a puzzle until we discovered that the assembler language routines controlling the pump flow rates, which had been developed for a different application, not only test, but also correct for, any 'backlash' before commencing delivery. This involves a feedback hysteresis loop to the computer and the time taken for backlash correction is inversely proportional to the requested flow rate. At 100 pi min" 1 the backlash
ENZYME KINETICS
317
assessment and correction time is between 500 and 600 ms, which accounts for the observed vertical displacement. This minor problem was only encountered when the second pump was started during data collection when backlash had to be tested for and corrected. Figure 14.6 shows the slopes of the four regression lines plotted against both the square root and the log of the respective flow rates. Regression analyses gave correlation coefficients of 0.9999 and 0.991 respectively. From this we assumed that the square root transformation was more appropriate, which gave a slope of — 0.0283 and intercept of 0.528. From these various data it was possible to express time in relation to flow rate and length of tubing between mixing and analysis points. This is given by the following equation, T= ((0.528 - (0.0283 x SQRT(F'))) x (L + 24.73)) + 0.6 where T is time, F is the average flow rate of the two pumps and L is tube length. The expression 0.528 —(0.0283 x SQRT(F)), derived from figure 14.6, is equivalent to the slope, m, in the equation Y= mX+ C, and L + 24.73 is equivalent to X, derived from figure 14.5. The constant C, 0.6 s, can be dropped when both pumps are started before data collection.
14.2
Enzyme kinetics
The first non-kinetic description of enzyme measurements by flow cytometry (Hulett et ah, 1969) exploited the phenomenon of fluorochromasia (Rotman and Papermaster, 1966) in which the lipophilic, membrane-permeable fluorogenic substrate fluorescein diacetate (FDA) was converted to the comparatively polar fluorescent product fluorescein by intracellular esterases. Since then there have been considerable advances which will continue with the further developments of probes.
14.2.1 Substrates A schematic for the conversion of substrate to product by enzyme action in whole cells is shown in figure 14.7. Substrate must first cross the external membrane, then interact with the enzyme generating the reaction product which can then be measured if it remains inside or associated with the cell. Unlike classical biochemical assays only product which is cell-associated is 'seen' by the instrument. The ideal substrate for flow enzymology is one which is lipophilic, non-toxic and either colourless or non-fluorescent. During the reaction this is converted to a highly polar product which is either light absorbing (coloured) or fluorescent. Substrate lipophilicity generally is required for rapid transport across the external cell membrane and high polarity of the product is desirable in order to 'trap' the product within the cell. However, no substrate meets all these criteria and a number of 'tricks' have been employed to simulate the behaviour of the 'ideal' substrate. Many 'classical' histochemical enzyme-staining procedures deposit insoluble
318
DYNAMIC CELLULAR EVENTS INTRACELLULAR
ENZYMES
Figure 14.7. Schematic for the conversion of substrate (Se) to product (P) by enzyme action in whole cells. Substrate must first cross the external membrane, then interact with the enzyme generating the product which can then be measured if it remains inside or associated with the cell. light-absorbing products which enables cells with the enzyme activity being studied to be identified. Some of these techniques have been adapted to flow technology. Peroxidase activity in white blood cells (Kaplow and Eisenberg, 1975) has been assayed based on supravital benzidine dihydrochloride staining where zinc chloride was used as a stabilizer for the blue reaction product (Kaplow, 1975). oc-Naphthol acetate has been used as a substrate for esterases (Kaplow, Dauber and Lerner, 1976) where the reaction product was coupled to fast blue salt BB to give a final product which was grey—black. The methods developed by Kaplow and collaborators are excellent for cellular identification in the systems for which the techniques were developed, but relatively 'static' patterns were obtained. Furthermore, these light-absorbing methods are relatively insensitive and not suitable for 'real-time' studies. This is particularly true where enzyme progress curves are required in order to obtain the kinetic parameters of enzyme action, and fluorogenic substrates are more suited for these types of studies. There is now a considerable variety of such substrates based on a number of different fluorophores. These include fluorescein, rhodamine, naphthol, naphthylamine, quinolines, methylumbelliferone and monochlorobimane for studying esterases, lipases, sulphatases, phosphatases, glucuronidases,
ENZYME KINETICS
319
transferases, peroxidases, peptidases, transpeptidases, galactosidases, arylmidases, glucosidases and glutathione-S-transferases to mention just a few. In general, the fluorescein and rhodamine based substrates and monochlorobimane are either weakly or non-fluorescent which is ideal. In contrast, the 4-methylumbelliferone conjugates are generally fluorescent but both their excitation and emission wavelengths are much shorter than those of the released product 4-methylumbelliferone and with correct optical design any 'overlap' can be minimized or eliminated. Techniques using the naphthol derivatives involve 'trapping' the released product within the cell by coupling with 5-nitrosalicylaldehyde which forms an insoluble fluorescent complex with an emission spectrum that is shifted into the red (Dolbeare and Smith, 1977). A comprehensive list of substrates and the reactions to release the associated fluorophores is not in order here and the reader is referred to the Molecular Probes Catalogue (Molecular Probes Inc. Eugene, Oregon, USA) and an excellent volume Applications of Fluorescence in the Biomedical Sciences (Lansing-Taylor et ah, 1986).
14.2.2 Light absorption quantitation Most light-absorbing reaction products are blue, blue—grey or black and a helium—neon (HeNe) laser emitting red light is ideal for such assays for two
CELL STREAM, SINGLE FILE PHOTOSENSORS
Figure 14.8. Absorbed light quantitation with two sets of light-sensitive detectors.
320
DYNAMIC CELLULAR EVENTS
reasons. Firstly, red light is well absorbed by the products and secondly, HeNe lasers are very stable. The absorbed light can be quantitated with two sets of lightsensitive detectors and a typical system is depicted in figure 14.8. Cells in flow intersect the focus and as each cell is illuminated there is a decrease in intensity on the detector A. This decrease in intensity is proportional to the cross-sectional area of the cell and is largely independent of the optical density. In contrast, the amount of light scattered into the S detector is inversely proportional to optical density. The instrument is set up initially with an unstained sample so that the amplitudes of the pulses from the S and A detectors are adjusted to be approximately equal. When a sample containing cells stained with light-absorbing material is subsequently analysed there is a decrease in the amplitude of the S detector (but not of the A) whenever a stained cell passes through the light beam. Thus, by comparison of the S-pulse with the A-pulse for each cell it is possible to define clusters which absorb light and hence to identify the stained cells in the population. 14.2.3 Fluorescence quantitation Fluorescence measurement is simpler, quicker and more sensitive than light absorption for a number of reasons. Firstly only one detector is needed for quantitation and secondly, the reaction is followed as it is taking place. Finally, there is no 'upper' detection limit in contrast to absorption methods where the lower' detection limit due to loss of signal represents greater activity. This problem can be partly overcome by having the capacity to vary the gain in the preamplifier circuits by defined quantities (Cox et a\., 1987). For absorption work the gain would be increased in the S detector and with fluorescence the gain would be reduced. However, this does have limitations. If very high fluorescnce activities are recorded during a run a neutral density filter can be placed in the light path to the detector. This attenuates the signal by a further defined quantity depending on the optical density of the filter. But no comparable manoeuvre can be applied in light absorption methods. 14.2.4 Cytoplasmic enzymes Kaplow and Eisenberg (1975) identified lymphocytes, monocytes, neutrophils and eosinophils in peripheral blood using peroxidase activity. These data are reproduced in figure 14.9, in which scattered light (ordinate) is scored against axial light loss (abscissa). Each cell in the sample is represented by a single dot on the storage oscilloscope with x and y coordinates that are respectively proportional to axial light loss and scattered light intensity. This technique has also been applied to patients with various haematological disorders and characteristic patterns of eosinophilia, lymphocytic leukaemia and chronic granulocytic were obtained (Kaplow, 1979). Monocytes contain large quantities of esterases and this enzyme activity is demonstrated in figure 14.10 which shows two samples from peripheral blood in which the monocyte clusters exhibited low (panel a) and high (panel b) esterase activity (Kaplow et al, 1976). Kaplow (1979) has also investigated the influence of incubation time on monocyte esterase activity and
ENZYME KINETICS
321
Figure 14.9. Identification of lymphocytes, monocytes, neutrophils and eosinophils in peripheral blood using peroxidase activity in which scattered light (ordinate) is scored against axial light loss (abscissa) from Kaplow and Eisenberg (1975).
Figure 14.10. Monocyte esterase activity in two samples from peripheral blood in which the monocyte clusters exhibited low (panel a) and high (panel b) esterase activity (Kaplow et al., 1976).
322
DYNAMIC CELLULAR EVENTS
has observed a progressive increase in axial light loss, but accurate quantitation of the reaction velocity was not possible. Dolbeare and Smith (1977) studied peptidases with a fluorescence technique which required product trapping. This type of technique was subsequently used by Pallavichini et al. (1977) not only to distinguish between intestinal crypt and villus cells, but also to sort these subpopulations based on leucine—amino peptidase activity. The differentiated villus cells contain considerably higher activity of this enzyme than the non-differentiated cells of the crypt. The continuous interrupted sampling technique (Watson et al., 1977) with FDA as substrate was used to show that cells in late plateau phase EMT6 cultures, in which more than 95% of the population was arrested in a Gl/G 0 state, exhibited considerably higher esterase activity than exponentially growing cells (Watson et al., 1978). The progress curves are shown in figure 14.11, with the data from the plateau phase and exponentially growing population in panels A and B respectively. The micromolar concentrations of substrate are shown against each progress curve. Figure 14.12 shows the substrate-dependent velocity plots associated with these data, which should theoretically follow the Michaelis-Menten rectangular hyperbola (Michaelis and Menten, 1913). There was a highly abnormal 'double-sigmoid' pattern for the plateau-phase cells but the exponentially growing cells exhibit less abnormal kinetic behaviour. Krisch (1971) has reported abnormal kinetic behaviour in certain esterase preparations and it has been suggested that the reaction mechanism may need two or more interacting catalytic sites. Substrate activation, where the reaction proceeds most rapidly when more than one substrate molecule is bound to a single enzyme molecule, may also be involved (Adler and Kistiakowsky, 1961). Furthermore, it is highly probable that more than one esterase is involved with the hydrolysis of FDA, which is a non-specific substrate. Guibault and Kramer (1966) have shown that FDA hydrolysis is catalysed by a number of enzymes including oc- and ychymotrypsin and lipase. However, further factors must also be considered for the abnormal kinetic behaviour shown in figure 14.12. Firstly, cellular and sub-cellular permeability barriers are likely to exist in the intact cell which could limit the availability of substrate at the enzyme site. Secondly, there could be active transport mechanisms for the substrate with intracellular accumulation. Each of these factors would result in a difference between the substrate concentration external to the cell and at the site of enzyme reaction and all of these various factors could contribute to the upward concavity (lag kinetics') seen for plateau phase cells in figure 14.12. Substituted naphthol was used as a substrate which did not require a trapping agent for the fluorescence product by Dolbeare and Phares (1979). This enabled them to produce progress curves for (3-glucuronidase and acid phosphatase. The reaction was allowed to proceed outside the flow cytometer and was stopped at intervals before flow analysis in a discontinuous assay. However, because of the long incubation time required to develop fluorescence, product diffusion became a limiting factor in these experiments. Dolbeare and Smith (1979) used a
ENZYME KINETICS
323
30-
144
TIME, Minutes Figure 14.11. Esterase activity in log and plateau phase EMT6 cultures using FDA as substrate, panels A and B respectively. The micromolar concentrations of substrate are shown against each progress curve.
DYNAMIC CELLULAR EVENTS
324
1-On
LOG
Substrate Concentration
Figure 14.12. Substrate-dependent velocity plots associated with the data in figure 14.11 which should theoretically follow the Michaelis-Menten rectangular hyperbola. combination of forward light scatter and (3-glucuronidase activity to distinguish lymphocytes, monocytes and macrophages in washings from the peritoneal cavity of the rat. These data are reproduced in figure 14.13 which shows the twodimensional histogram of frequency on the vertical axis versus light scatter and fluorescence on the two horizontal axes. Vanderlaan, Cutter and Dolbeare (1979) have shown that y-glutamyl transpeptidase activity is considerably higher in hepatocytes following carcinogen exposure than in control populations. However, Vanderlaan et al. (1979) have also shown that in mixed populations it can be difficult to identify positively the transformed cells in the absence of product trapping as the reaction product can diffuse from cells with high enzyme activity and subsequently enter those with little or no activity. However, this problem can be largely overcome by short incubation times and multiparameter analysis. Alkaline phosphatase and an arylamidase can be used as markers for normal and transformed Wi-38 cells (Dolbeare et al., 1980). These results demonstrated that the enzymes in the transformed cells differed by not only a qualitative but also a quantitative change in alkaline phosphatase, as well as a quantitative loss of arylamidase.
ENZYME KINETICS
325
Figure 14.13. Forward scatter versus (3-glucuronidase activity versus frequency which distinguished between lymphocytes, monocytes and macrophages in washings from the peritoneal cavity of the rat (Dolbeare and Smith, 1979).
Glutathione (GSH) metabolism is a critical determinant in control of cellular response to anticancer drugs and radiation. Depletion of protective GSH results in sensitization. Kosower et al. (1979) were the first to use fluorescent bimanes to study intracellular thiols and Rice et al. (1986a) using flow cytometry have shown that monochlorobimane (mClB) can act as a reporter molecule in GSH metabolism. As an extension to this we developed a sensitive multi-parametric flow cytoenzymological assay using continuous time measurements to determine reaction kinetics for conjugation of mClB with GSH in populations of intact viable cells catalysed by the enzyme family, the glutathione-S-transferases (Workman and Watson, 1987). Monochlorobimane is a non-fluorescent probe which after conjugation with GSH results in a relatively insoluble fluorescent complex excited by UV light with emission in the blue (460—510 nm). The reaction is illustrated in figure 14.14 and the reaction rate is a function of added mClB, intracellular GSH content and the activity of the transferase(s). The progress curves generated should reach an asymptope when all intracellular GSH is converted. Figure 14.15 shows the results from a FicoU—Paque lymphocyte-enriched preparation obtained
326
DYNAMIC CELLULAR EVENTS
CH 3 +
V-Glu-Cys(SH)-Gly
CH2CI
GSH
rnCIB ( non-fluorescent, penetrates cell)
GSH - S - transferase
mClB - GSH conjugate ( fluorescent, trapped in cell)
Figure 14.14. Reaction of monochlorobimane with the tripeptide glutathione mediated by transferases to produce the insoluble fluorescent conjugate.
from heparinized whole blood of a normal subject which was mixed with 120 pM mClB plus propidium iodide at a concentration of 50 |ig ml ~ l (Workman, Cox and Watson, 1988). Forward and 90° scatter signals were collected together with blue and red fluorescence. The latter is also excited by UV from the DNA of dead cells which do not exclude propidium iodide. Panel A shows forward versus 90° scatter in which three regions can be defined. Regions 1 and 2 correspond to lymphocytes and monocytes respectively. Region 3 represents debris and propidium iodide positive dead cells. Panels B and C show the accumulation of blue fluorescence with time as frequency contour plots where it can be seen that monocytes (panel C) exhibited greater activity than lymphocytes (panel B) consistent with larger quantities of GSH and/or GSH-S-transferase. A more conventional display, derived from the data in panels B and C, shows medians of the distributions at
ENZYME KINETICS
327
SCAT TEI
A
|
o
A //n
REGION 2 REGION 1
B
REGION 3
f
U-
9O° SCATTER
REGION 2 MONOCYTES
REGION 1 LYMPHOCYTES
figure 14.15. Ficoll—Paque lymphocyte-enriched preparation obtained from heparinized whole blood of a normal subject which was mixed with 120 JiM mClB plus propidium iodide at a concentration of 50 |lg m l " l (Workman et al., 1988). Forward and 90° scatter signals were collected together with blue and red fluorescence. The latter is also excited by UV from the DNA of dead cells which do not exclude propidium iodide. Panel A shows forward versus 90° scatter in which three regions can be defined. Regions 1 and 2 correspond to lymphocytes and monocytes respectively. Region 3 represents debris and propidium iodide positive dead cells. Panels B and C show the accumulation of blue fluorescence with time as frequency contour plots where it can be seen that monocytes (panel C) exhibited greater activity than lymphocytes (panel B) consistent with larger quantities of GSH and/or GSH-S-transferase. A more conventional display, derived from the data in panels B and C, shows medians of the distributions at discrete time intervals plotted against time in panel D. The dead cells and debris in region 3 exhibited no activity.
328
DYNAMIC CELLULAR EVENTS
discrete time intervals plotted against time in panel D. The dead cells and debris in region 3 exhibited no activity. The data in figure 14.15 represent a fivedimensional set as two scatter and two fluorescence measurements were recorded with the fifth parameter, time. Further flow cytoenzymological studies using single substrates have included the measurement of elevated y-glutamyl transpeptidase levels in aflatoxin-induced rat hepatoma cells with implications in toxicology (Manson et al, 1981), the detection of acid-P-galactosidase activity in human fibroblasts (Jongkind, Verkerk and Sernetz, 1986) and the determination of cell cycle phase-specific changes in cellular phosphatase and glycosidase activities in stimulated lymphocytes and cultured cell lines (Britten and Dyson, 1987).
14.2.5 Membrane enzymes An automated fluorimetric method for assaying alkaline phosphatase using 3-0-methylfluorescein phosphate was developed by Hill, Sumner and Waters (1968). An adaption of this technique has been applied to intact cells using flow cytometry by Watson, Workman and Chambers (1979). Again, the continuous interrupted method was used. The results for EMT6 cells are shown in figure 14.16. These are obviously very different from those for intracellular esterases shown in figure 14.11 and they presented a considerable interpretative problem which was not resolved until a sample was viewed under the fluorescence microscope. It was then seen that the fluorescence was concentrated in 'halos' at the external cell membrane with no fluorescence from the interior of the cells. Subsequent incubation of cells with product, 3-0-methylfluorescein, failed to demonstrate entry into intact cells. The viability of EMT6 cells decreases considerably after 3 hours incubation with protein-free phosphate-buffered saline (PBS). In a sample of cells so treated it was found that the fluorescence from 2>-omethylfluorescein was no longer located at the cell surface but was being emitted from granular structures surrounding the nucleus. This fluorescence was considerably more intense than that emitted from the cell surface, so much so that the latter could no longer be seen. These various data suggested that substrate hydrolysis in intact viable cells takes place at or within the cell by phosphatases located in the plasma membrane and that the product was lost from the immediate vicinity of the cells by diffusion and consequently was not 'seen' by the instrument. Thus a steady state would be reached in which the rate of production of fluorescent product would equal the rate of loss, giving rise to asymptotic fluorescence responses from the population at each substrate concentration. On the assumption that this hypothesis was correct, Watson et al (1979) were able to show that the progress curve at a given concentration, S, should be described by the equation, x(1.0-exp(-fcxf))
(14.1)
where P(t) is the fluorescence response at time t, P^ is the theoretical maximum asymptotic response at infinite substrate concentration, Km is the Michaelis
ENZYME KINETICS
329
Time, minutes
Figure 14.16. Progress curves for hydrolysis of 3-O-methylfluorescein phosphate. The micromolar concentrations of substrate are shown adjacent to each curve.
constant and k is the rate constant.for product loss assuming a first order kinetic process. When a steady state exists (i.e. beyond 2.5—3 minutes in figure 14.16) the term exp( — kxt) in equation 14.1 will tend to zero and the asymptotic fluorescence response will be given by the expression P^ x S/(S + Km) and will vary with substrate concentration. P^ can be eliminated from this expression by taking ratios, thus, P (t ) Pltfoo)
S
(*
_
(14.2)
where P^oo) and P2(to0) are the asymptotic fluorescence values associated with substrate concentrations SY and S2 and where R12 is the ratio of P2(^oo) to P^oo)Equation 14.2 can be rearranged to give,
330
DYNAMIC CELLULAR EVENTS
where for N substrate concentrations / varies from 1 to (w — 1) and j varies from (/ +1) to N, to give a triangular matrix for the ratios containing jN(N— 1) values. Thus, by plotting Rtj against [(1/St) — (R tj/SJ)] a line with slope Km is obtained which intersects the ordinate at unity. In three separate analyses values of 110.0 + 31 |lM, 122.3 + 31 uM and 120.5 + 24 |lM were obtained where the limits were calculated at two standard errors and in all cases the ordinate intercept did not differ from unity, p > 0.1. It can be seen from equation 14.2 that if P^ is the asymptotic fluorescence response at infinite substrate concentration, Soo, then, P
S
_oo__^o_
(I
_-
where Pn is the asymptotic response at Sn. The term Soo^Soo+Km) is unity; therefore, Pn x (Sn + Km) = P^ x Sn. By plotting Pn x (SB + Km) against Sn a line of slope PQO is obtained which intersects the origin. Thus P^ can be obtained after a value for Km is found. It was also shown previously (Watson et al, 1979) that the maximum reaction velocity, Vmax, is equal to the product of P^ X k. As equation 14.1 is an inverted exponential an approximate value of k can be found from the time taken for the curves to reach half their maximum height and a more accurate estimate can be obtained by curve fitting. The latter gave a rate constant of 1.98 min~ \ thus Vmax can be defined in the arbitrary units of channels per minute. The three analyses gave maximum reaction velocities of 107.0 110.0 and 109.2 channels per minute. The progress curves in figures 14.11 and 14.16 are very different and two major differences between the fluorogenic substrates should be considered. Firstly, 3-omethylfluorescein, the reaction product of 3-o-methylfluorescein phosphate, is considerably less polar than fluorescein, the reaction product of FDA. Thus, if 3-omethylfluorescein enters the cell we would expect the rate constant for leakage from the cell to be greater than that for fluorescein. Previous studies indicated that fluorescein leaks out of EMT6 cells with a half-time of 7-8 minutes (Watson et al, 1979; Watson, 1980a), thus the leakage rate constant is about 20 times greater than that for fluorescein. Secondly, fluorescein diacetate is lipophilic and will penetrate the cell without prior hydrolysis by any membrane esterases. The direct observations made with the fluorescence microscope suggest that the product of 3-0-methylfluorescein phosphate hydrolysis either does not enter the cell or it diffuses out of the cell very rapidly although some remains associated with the external membrane. Both possibilities are compatible with the magnitude of the loss rate constant whatever the mechanism. These results are interesting biologically as they suggest that dephosphorylation at the cell membrane does not necessarily lead to appreciable uptake or accumulation in the cytoplasm.
14.2.6 Dual substrate analysis The substrate-dependent initial velocity plots shown in figure 14.12 suggested the possibility that two or more enzymes were hydrolyzing fluorescein diacetate in EMT6 cells. As this is a non-specific esterase substrate it was not
ENZYME KINETICS
331
unreasonable to expect that a second non-specific esterase substrate with a different molecular structure might show different reaction rate characteristics. Furthermore, it was also not unreasonable to postulate that two different cell types would contain either different esterases or if the same enzymes were present they were unlikely to be present at the same concentration or exhibit the same activity. Thus, by assaying with two different non-specific esterase substrates (fluorescein diacetate and 4-methylumbelliferyl acetate) simultaneously using dual laser excitation (argon 488 nm and krypton UV) in a mixture of two different cell types it should be possible to distinguish between the populations. The results of one such assay are shown in figure 14.17, where the green (fluorescein diacetate hydrolysis) fluorescence for each cell is scored on the ordinate against the violet (4methylumbelliferyl acetate hydrolysis) fluorescence on the abscissa. Two distinct populations are apparent. The cluster to the upper left represents the EMT6 mouse mammary tumour and that to the lower right represents the human colonic adenocarcinoma HT29. These two cell lines were chosen for the initial analysis for two main reasons. Firstly, the cell types were sufficiently different to stand a reasonable chance of obtaining a discrimination and, secondly, the plating efficiencies and culture characteristics were well documented and understood. Apart from the primary objective of distinguishing between different cell types these assays were being developed with a view to maintaining cell viability. This
0) O
c 0)
o > 0)
o 3
0)
Violet fluorescence Figure 14.17. Dual non-specific esterase substrate assay where green fluorescence (fluorescein diacetate hydrolysis) for each cell is scored on the ordinate against violet fluorescence (4-methylumbelliferyl acetate hydrolysis) on the abscissa.
332
DYNAMIC CELLULAR EVENTS
has largely been achieved with both cell types maintaining a plating efficiency of about 90% even after a 6 hour exposure to maximum concentrations of the substrate mixture. It has also been reported that a discrimination can be made between fibroblasts, a lung tumour and a second colon carcinoma, all of human origin, using this combined esterase assay (Chambers and Watson, 1980; Watson, 1980b). These results were sufficiently encouraging to attempt to discriminate between the different subsets to be found in the much more complex biological system of bone marrow. Using a combination of six simultaneous measurements on each cell (UV and blue light both scattered at 90° and at narrow forward angles, coupled with the two non-specific esterase substrates, fluorescein diacetate and 4-methylumbelliferyl acetate) it has been possible to identify between 10 and 16 different subsets in mouse bone marrow (Watson and Chambers, 1980; Watson, 1980b). The same combination of fluorochromes has been used by Malin-Berdel and Valet (1980) to characterize mouse spleen and bone marrow cell subpopulations based on differing esterase and phosphatase activities. Some examples of this type of multiparameter analysis, in which only one substrate was used, were shown in chapter 5 (figures 5.5 and 5.8) as an illustration of multi-parameter data handling and display. A combination of esterase and y-glutamyl transpeptidase activity using fluorescein diacetate and y-glutamyl-7-amino-4-methyl-coumarin simultaneously as substrates has been used to discriminate between normal and malignant liver cell lines. This technique also requires a twin-laser instrument to excite the reaction product from y-glutamyl transpeptidase activity (4-methylumbelliferone, krypton UV excitation) and esterase activity (fluorescein, 488 nm argon excitation). Esterase and y-glutamyl transpeptidase activities were both greater in the aflatoxin-transformed malignant cells which enabled an excellent discrimination to be made between the two cell types.
14.2.7 Inhibition kinetics Chloroethylnitrosoureas (Cnus) are an important class of antitumour agent. Their exact mode of action is not known but chloroethylation of DNA and subsequent crosslinking has been implicated (Gibson, Mattes and Hartley, 1985). However, protein carbamoylation may also be involved as organic isocyanates as well as alkylating species are formed when Cnus decompose in aqueous environments. Carbamoylating agents have been shown clearly to inactivate a number of enzymes, and inactivation of glutathione reductase has been used to determine the protein carbamoylation potential of Cnus (Babson and Reed, 1978). Because of the susceptibility of serine hydrolases to isocyanate inactivation (Brown and Wold, 1973) Paul Workman of our laboratories proposed that flow cytometric measurement of esterase activity might form a basis for the determination of intracellular carbamoylation by Cnu-derived isocyanates (Dive et al., 1987b,c). This proved to be the case and an example of esterase inhibition induced by BCNU-derived isocyanate is shown in figure 14.18. By using a number of different drug doses as in figure 14.19 it is possible to obtain an estimate of the
333
ENZYME KINETICS
B 50
I
40
UJ
O
UJ
30
I
20
11.
10
U
o
0
100
200
300
TIME ( SEC )
Figure 14.18. Inhibition of esterase activity by BCNU-derived isocyanate (Dive et al, 1987b). The top two diagrams (panel A) show size versus fluorescence on the X- and Z-horizontal axes with time (which increases upwards on these displays) on the Y-axis. Contour plots of size versus fluorescence for ten equal 'time-slices' are shown within these three-dimensional data spaces. Top left is the control and top right shows the inhibition due to BCNU. Panel B shows the medians of the fluorescence distributions of each 'time-slice' plotted against time.
drug concentration which causes a 50% reduction in FDA hydrolysis activity, defined as the I50 value. Using the I50 it is possible to compare directly the inhibitory effects of a number of Cnus and related cytotoxic agents and the potential utility of this is discussed in section 15.3.2.
14.2.8 Short time scale kinetics Kinetic measurements in the temporal reference frame of a few seconds after biochemical perturbation are potentially of great importance for studying cell activation and a new technique for this type of measurement was described in
334
DYNAMIC CELLULAR EVENTS
100
10'6
10'5
10"4 BCNU CONCENTRATION (M)
10'3
10'2
Figure 14.19. Enzyme activity for multiple concentrations of BCNU. The dose which produces 50% inhibition of enzyme activity, I50, can be estimated from data such as these. section 14.1.4. The method was tested with EMT6 mouse mammary tumour cells in exponential growth adjusted to a concentration of 2 x 105 cells ml" 1 and introduced into pump 1 (see figure 14.3). FDA was made up at a concentration of 2 |oM and loaded into pump 2. Both pumps were started and the high tension voltage of the green detector was adjusted to record the fluorescein emission histogram with a mean in about channel 600 at pump flow rates of 100|j] min~ l for a tube length of 40 cm. Recordings were then made at each of the four tube lengths at the same flow rate. From the data shown in figure 14.20 it can be seen that the fluorescence distribution is progressively shifted to higher values with increasing tube length. It should also be noted that the distribution remains constant with time as the period taken for cells to flow from the mixing chamber to analysis point is constant. This overcomes one of the potential problems associated with continuous time recording of 'fast' reactions where, because of the reaction velocity, only relatively few cells can be recorded with a given fluorescence intensity. A number of further recordings were made with various tube lengths and pump flow rates. The medians of the green fluorescence distributions so obtained are plotted against time in figure 14.21 which shows that the accumulation of fluorescence was biphasic over the first 16 seconds of the reaction. A regression analysis (solid line) was carried out for the data beyond 5
MEMBRANE POTENTIAL
335
5 cm
10 cm
o c 0)
20 cm
3
& 0)
40 cm
Fluorescence intensity Figure 14.20. FDA hydrolysis fluorescence distributions for four tube lengths at the same flow rate from EMT6 cells. seconds and this gave a correlation coefficient of 0.99 which is compatible with a linear increase in fluorescein with time between 5 and 16 seconds. However, the dotted curve drawn by eye, is more compatible with the biological reality and the lag probably represents the time taken for substrate to diffuse across the external cell membrane and cytoplasm to the site(s) of enzyme action.
14.3
Membrane potential
Fluorescent membrane potential probes are charged symmetrical, 'mirrorimage ring-structure molecules with hydrocarbon side chains. The molecule retains lipophilicity as the charge is not localized and the relative lipophilicity can be engineered by changing the length of the side chains. The cationic cyanin dyes 7
DYNAMIC CELLULAR EVENTS
336
6OO1 ft
I
* 400 o o o
1 200 LL
10
15
Time, seconds Figure 14.21. Biphasic FDA hydrolysis over the first 16 seconds of the reaction shown by the dashed curve. The data from 5 to 16 seconds can also befittedwith a straight line (non-interrupted) but this is less likely to represent the biological reality. were the first such molecules to be recognized as membrane-potential probes (Sims et al, 197A). They partition in lipids to an extent that varies partly with side chain length and partly with potential across the cell membrane. A second class of dyes, the oxanols, are functionally similar to the cyanins differing only in that they are anionic (Rink et al, 1980). Cyanins are excluded as cells undergo depolarization whereas oxanols are excluded on re- and hyper-polarization. The cyanins, however, suffer from the disadvantage that they are taken up extensively by mitochondria which can reduce the 'signal-to-noise' ratio when assessing external membrane potential. This problem, however, is overcome by using the oxanols. These probes have been used in studies of granulocyte and lymphocyte function and in mitogenic stimulation of T-cells (Tsien, Pozzan and Rink, 1984).
14.4
Calcium
Ligand activation of cell surface receptors linked to the phosphatidyl inositol pathway generates the second-messenger molecules inositol triphosphate and diacylglycerol (Berridge and Irvine, 1984). Inositol triphosphate mobilizes calcium leading to an increase in free calcium ions (Ca2 + ) in the cytoplasm. As stated in section 8.4.2, Indo-1 is the preferred calcium probe as it exhibits a shift in emission spectrum on binding calcium. These spectra are shown in figure 14.22 where it is apparent that as the Ca2 + concentration rises there is a progressive shift of the emission to shorter wavelengths. In the absence of Ca 2+ the emission peak is at
CALCIUM
337
0.1-1 mM
X 0)
4
4) O 0) O (0
o =2 2
500
400 Wavelength, nm
Figure 14.22. Changes in the emission spectrum of Indo-1 with increasing Ca2 + concentration which are given in nanomoles against each curve except for the maximum which is micromolar. These data were redrawn from Grynkiewicz et al. (1985) who pointed out that the 'notch' at 465 nm was an instrument artefact.
480-485 nm and at saturating concentrations this has shifted to 400-405 nm. Thus, the ratio of the emissions at 400 nm and 480 nm gives a relative measure of calcium chelated by the probe. Rabinovitch et al. (1986) and more recently Keij et al. (1989) have produced a method for expressing the fluorescence ratio as a concentration of Ca 2+ by the following equation, nMCa2+=Kdx
f
b2
The meanings of these various symbols are as follows. Kd is the Indo-1/Ca2 + dissociation constant which is numerically equal to 250 nM (Grynkiewicz et al., 1985). R is the 400:480 nM fluorescence ratio and Rmax and Rmin are the 400:480 nM fluorescence ratios for Indo-1 loaded cells in the presence of saturating concentrations of Ca2 + and in the absence of Ca 2+ respectively. A value for Rmax can be obtained in intact cells by treating with the ionophore ionomycin (Rabinovitch et al, 1986) which allows equilibration of internal Ca2 + with the very much higher external concentration to take place. Rm\n is obtained by treating the cells with ionomycin + EGTA. The latter chelates Ca 2 + external to
DYNAMIC CELLULAR EVENTS
10
2 3 Time, minutes
2 3 Time, minutes
Figure 14.23. T-cell activation showing [Ca2 + ] versus time where panels A and B give dot-plots for each cell and population means respectively.
the cells and hence 'drains' Ca2 + from the cells. S b2 and Sf2 are the fluorescence values at 480 nm for Ca2 + -bound Indo-1 and Ca2 + -free Indo-1 respectively and these too are obtained from cells treated respectively with ionomycin and ionomycin + EGTA. A slight variation on this theme was used by Keij et al. (1989) where saponin + EGTA was used instead of ionomycin + EGTA. Keij et al. (1989) have used the formula given above to present results in the form of Ca 2+ concentrations in studies involving both T- and B-cell activation with PHA and pneumococcal polysaccharide respectively. The T-cell results showing [Ca2 + ] versus time are reproduced in figure 14.23 where panels A and B give dot-plots for each cell and mean population values respectively. Time was not incorporated into the list-mode data base directly for these studies but it was 'inferred' from the computer recorded duration of the run by dividing sequentially the list-mode data into 255 equal channels. Thus, a time-related factor was produced which was used to plot [Ca2 + ] versus time. This is not the ideal method for incorporating time into the data base as extreme care must be taken to keep the flow rate constant. However, it is the only compromise possible for commercial instruments which do not include the facility to incorporate time in the data base from the computer clock. However, Griffioen et al. (1989) have used this method to study Ca 2+ kinetic changes in lymphocytes. Indo-1 has also been used to study Ca 2+ kinetic changes in lymphocytes under various stimuli by Chused et al. (1986,1987) who were able to distinguish between T- and B-lymphocytes from mouse spleen cultures where the mixed population was subjected to B-cell mitogenic stimuli. Within 20 seconds the B-cell component had responded as indicated by their increase in Ca2 + . It has also been used to study Ca 2+ changes in polymorphonuclear leukocytes (Lopez, Olive and Mannoni,
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1989) and in platelets subjected to thrombin stimulation (Davies et al, 1988). In the latter study there was an initial increase in Ca 2+ which was maximal by about 15 seconds followed by a slow decline. The use of flow cytometry enabled two subsets to be defined where one responded fully but the other responded partially or not at all. Rabinovitch et al. (1986) studied not only Ca 2+ changes during lymphocyte activation but also cell surface determinants simultaneously with Ca 2+ using antibodies labelled with phycoerythrin in a multi-parameter assay. Heterogeneous Ca 2 + responses were observed which to some extent were related to immunophenotype. Only examples of Ca2 + responses using Indo-1 have been given in this section as this is the current probe of choice; however, the uses of fura-II and quin-II together with Indo-1 have been reviewed by Ransom, DiGiusto and Cambier (1987).
14.5
Mitochondrial function
Rhodamine-123 is a class of cationic dye which partitions into electronegative environments and has been described as a mitochondrial specific dye (Johnson et al, 1981; Weiss and Chen, 1984). This description was based on fluorescence microscopy observations which revealed intense mitochondrial staining and is not strictly correct as rhodamine-123 will partition into any electronegative compartment. However, the interior of mitochondria is very electronegative if the proton pump is functioning normally and staining intensity gives some indication of the integrity of normal mitochondrial function. Rhodamine-123 has been studied in some in vitro tumour cell lines where it is reported to be preferentially retained and selectively cytotoxic (Lampidis et al, 1982). A decrease in its uptake has been used as an indicator of loss of mitochondrial function possibly associated with decreased respiratory activity in L1210 cells treated with anticancer drugs (Bernal, Shapiro and Chen, 1982). Martinez, Vigil and Vila (1986) have also used this probe as an indicator of respiratory activity and its uptake is increased in some small cell lung cancer cell lines after interferon-y treatment (Jabbar, Twentyman and Watson, 1989).
14.6
Drug transport
Transport of any agent across the external cell membrane from without occurs by at least three mechanisms; see review by Goldenberg and Begleiter (1984): (1) passive diffusion, where rate of increase of the intracellular concentration is directly proportional to the concentration gradient; (2) facilitated diffusion, where influx involves specific interactions between transport molecules and drug which, unlike passive diffusion, is temperature sensitive and exhibits saturation kinetics but the intracellular concentration cannot exceed that externally; (3) active transport, where the agent can be concentrated within the cell
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against a gradient using an energy-dependent mechanism. Clearly, these factors also apply to transport from inside the cell to outside, and this has important implications in multi-drug resistance. Flow cytometric quantitation depends on fluorescence and any direct measurements of drug uptake must rely on the drug itself being fluorescent, quenching of a reporter fluorochrome by the drug or the availability of a fluorescent analogue. Two classes of agents fall into these categories. First, the commonly used anthracyclines, daunorubicin and adriamycin, are both fluorescent and can induce quenching of propidium iodide/DNA emission. Second, fluorescent analogues of the anti-folates, aminopterine and methotrexate, have been synthesized (Gapski et al, 1975; Henderson, Russell and Whiteley, 1980; Rosowsky et al, 1982; Kumar et al,
1983a,b).
The quenching of propidium iodide DNA fluorescence as a means of assessing nuclear adriamycin content was demonstrated by Krishan and Ganapathi (1979) and these investigators also demonstrated the feasability of measuring intracellular anthracycline fluorescence directly (Krishan and Ganapathi, 1980). Durand and Olive (1981) used similar direct fluorescence techniques to quantitate cellular adriamycin and additionally they showed time courses for uptake and compared nuclei with whole cells. Some of these data are reproduced in figure 14.24. Moreover, Durand (1981) demonstrated a considerable adriamycin concentration gradient across multi-cell spheroids. Lower adriamycin fluorescence was found in cells in the center which had greater cell survival probability than those at the periphery where fluorescence was greater. Multi-parameter analysis of adriamycin and daunomycin uptake in mouse bone marrow and acute myeloid leukaemia cells has been carried out by Sonneveld and van den Engh (1981) using forward and 90° light scatter properties to identify different subsets (Visser et al, 1980). Fluorescence was related directly to cytotoxicity and myeloid progenitor cells were an order of magnitude more sensitive to daunomycin compared with adriamycin, a result which correlated with fluorescence. In contrast, the fluorescence from acute myeloid leukaemia cells was greater for adriamycin than for daunomycin. Further studies of daunomycin fluorescence uptake by rat bone marrow were carried out by Nooter, van de Engh and Sonneveld (1983) where dead cells, lymphocytes, blast cells, granulocytes and red cells were separately identified on light scatter. At higher concentrations the lymphocyte fraction exhibited greater fluorescence than granulocytes arid at given concentrations the dead cells exhibited considerably greater fluorescence than viable cells. These various effects were attributed to quantitative differences in active transport of these agents into different cell types. Absolute calibration of drug content per cell was also effected in these studies using [3H]-daunomycin and, in conjunction with cell sorting, a detection limit below 10~ 18 M cell" 1 was obtained. Anthracyclines are actively transported both into and out of cells, but by different pump mechanisms. One of the efflux pumps is the 170 kda membrane associated glycoprotein (pg170) encoded by the Multi-Drug-Resistance, MDR-1,
DRUG TRANSPORT
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1000o | 500-
50
100 150 Fluorescence
200
250
0)
o
O
3-
o
30
60 90 Time (minutes)
120
Figure 14.24. Panel A shows adriamycin fluorescence distributions for 2 hour exposures at the concentrations, in Jig ml" 1 , indicated adjacent to each histogram. Time courses for the increase in adriamycin fluorescence for whole cells (O) and nuclei ( # ) exposed to 1.0 |lg ml" 1 are shown in panel B. Redrawn from Durand and Olive (1981).
gene (see section 15.3). Extensive evidence now exists which shows that multidrug-resistant cells have increased numbers of membrane associated gp 170 molecules and as a result MDR cells exhibit lower fluorescence on exposure to anthracyclines compared with sensitive cells as these agents are actively transported out of MDR cells with greater efficiency. Ross et al (1989) have used this property to cell sort and isolate a very low frequency but highly MDR population from within a sensitive P388 cell population on duanorubican fluorescence. The correct functioning of the efflux pump mechanisms can be modulated by Ca 2+ channel blockers (chloropromazine, trifluoperazine and
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verapamil; Tsuro et al, 1982). A number of studies on the modulation of anthracycline uptake by Ca2 + channel blockers have been carried out using flow cytometry in resistant and sensitive cells in both animal and human systems (Krishan et al, 1986, 1987; Ross, Joneckis and Schiffer, 1986; Nooter et al, 1989; Morgan et al, 1989; Watson, Morgan and Dive, 1989). The 'bottom line' in all these studies is that the lower accumulation of anthracyclines in multi-drugresistant cells can be partially reversed by exposure to Ca 2+ channel blockers which interfere with the efflux pump mechanism. This is easily monitored by flow cytometry to give a predictive assay for MDR which will be described in section 15.3. Similar types of studies have been carried out with cells sensitive and resistant to the antimetabolite methotrexate using fluorescent analogues of the latter. However, methotrexate resistance is different from that in MDR and two of the three mechanisms identified are attributable to Fisher (1961, 1962). The enzyme dihydrofolate reductase, DHFR, converts folic acid to folinic acid which is required in one of the pathways to DNA synthesis. Methotrexate binds to DHFR with an affinity about 40-fold greater than that of folic acid and blocks its action. Fisher (1961) demonstrated that methotrexate resistance could be caused by elevation of dihydrofolate reductase levels. Cells grown continuously in medium containing methotrexate exhibit amplification of the DHFR gene (Hanggi and Littlefield, 1976; Alt, Kellems and Schimke, 1976) where the multiple copies are contained in 'double minute' chromosomes and are manifest in such cells at metaphase. Stable mutants are obtained when these double minutes become integrated into the normal chromosomes and the amplified gene can then be transmitted predictably from one generation to the next which confers considerable methotrexate resistance on the population. Fisher (1962) also demonstrated that the rate of influx of methotrexate (MTX) was about 15-fold lower in resistant compared with sensitive cells. At equilibrium the intracellular MTX concentration was between 10- and 30-fold lower in the resistant cells. However, this is not due to metabolic changes as dihydrofolate reductase levels were equal in both the resistant and sensitive cells. Changes in methotrexate membrane transport contributing to resistance (Schimke, 1984) have also been demonstrated by Sirontak et al. (1981) and Dembo, Sirotnak and Moccia (1984) have presented evidence that the cellular influx and efflux pathways for methotrexate are different. The third mechanism of methotrexate resistance is due to an alteration of the affinity of methotrexate binding to DHFR (Flintoff, Davidson and Siminovitch, 1976; Haber et al, 1981). To date relatively limited work has been carried out on methotrexate-resistant cells using flow cytometry. This has been in part due to the difficulty of producing fluorescent analogues with low background as pointed out by Gaudray, Trotter and Wahl (1986). However, these authors overcame this problem with a fluorescenated derivative of the ligand and presented data which suggested that staining heterogeneity with the analogue was partly due to transport variability within the population. Assaraf and Schimke (1987) loaded cells with fluorescent methotrexate then examined the ability of hydrophilic and lipophilic antifolates to displace the probe. Methotrexate-resistant cells incubated with methotrexate
CONCLUDING REMARKS
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200-
4
6
8
Time (hours) Figure 14.25. Uptake kinetics for fluorescent methotrexate in a parental cell line (AA8, # ) and a dihydrofolate reductase diffident cell line (DG-44, O) from Assaraf et al (1989).
(hydrophilic) exhibited no reduction in fluorescence compared with sensitive cells however, incubation with lipophilic analogues produced reductions in fluorescence in both sensitive and resistant cells. This is very compelling evidence for a membrane active-transport mechanism for methotrexate and hydrophilic analogues which is deficient in resistant cells. The lipophilic analogues enter cells by passive diffusion without the need for an active-transport mechanism, hence these displaced the fluorescenated probe bound to DHFR in both the sensitive and resistant cell lines. Similar types of studies have been carried out by Rosowsky et al (1986) and Wright et al (1987). Figure 14.25 shows the uptake of fluorescent methotrexate versus time in a parental Chinese hamster cell line, AA8, and in a DHFR-deficient cell line, DG-44. The former exhibits very considerably greater fluorescence which is attained at a more rapid rate. The effect of a temperature reduction, which slows the uptake rates of active-transport processes but not of passive diffusion, is shown in figure 14.26. There was a profound decrease in fluorescent methotrexate uptake in parental CHO when the temperature was decreased from 37°C to 4°C, an effect which was easily observed in the initial stages of uptake with a temperature decrease to 27°C. Both of these last two data sets were redrawn from Assaraf, Seamer and Schimke (1989).
14.7
Concluding remarks
Measurement of dynamic cellular events in intact cells under physiological or near physiological conditions, irrespective of the assay system, is arguably one of the most powerful techniques in cell biology. Physiological and
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25
Time (minutes) Figure 14.26. Temperature-dependent uptake of fluorescent methotrexate in parental CHO cells. The insert shows that cooling from 37°C to 4°C effectively abolishes uptake. The main graph shows that a reduction in uptake can be measured with a temperature decrease to only 27°C, from Assaraf etal. (1989).
pathological processes are not static but are continuously varying. Observing and measuring an event in isolation gives us little or no insight into what gave rise to the event or what the future consequences might be. The measurement of time structures our perception of the biological process as it places sequential interdependent events in the correct temporal relation to each other. It is becoming increasingly obvious that many of the initial events involved in cell proliferation and differentiation control take place within a time frame of seconds, but the effects of those initiating events (e.g. growth factor stimulation, membrane calcium flux and pH changes and carcinogen interaction) may only become apparent some days, weeks or even years later. Clearly, an understanding of the dynamics of inappropriate or abnormal initiating events will be of crucial importance in attempts to modulate pathological states. Incorporation of time into flow cytometry data bases, particularly for short time scale processes, undoubtedly will make contributions to that understanding.
15 Applications in oncology
This chapter originally started life as applications in clinical medicine and as such it would have been relatively easy to write five years ago. However, with the amazing proliferation of flow cytometry applications in medicine during the past few years this has become such a daunting prospect that I 'ducked-out' and decided to contract it to applications in clinical oncology. The latter discipline in the UK means all aspects of cancer patient management including diagnosis, pathology, surgery, radiation therapy and drug treatment. Writing in my capacity as a clinical oncologist I think I can cope with this, but I would like to stress the 'think', as this is still a formidable undertaking. At this point I would advise people who have no interest in cancer and whose area has not been covered to move smartly on to the epilogue where you may find just a brief mention of your field which has been omitted from the volume. However, I suppose that won't help much so you might as well stop here. After further deliberation I decided not to embark on a comprehensive account of all that has been done in cancer with flow cytometry although many of the references are included. I thought it might be more constructive to try to concentrate on what needs to be done and how flow cytometry might be able to help. In order to effect this approach it is necessary to ask a number of questions although I'm not trying to pretend there are any 'real' answers at present. As a physician confronted by a patient with cancer I would like to know a number of things. Firstly, the exact diagnosis, which is usually straight forward, but not always. For instance, it is sometimes difficult to be precise about tumours in lymph nodes in the neck. Even the very best histopathologists can have difficulty discriminating between lymphomas and undifferentiated carcinomas at this site particularly if the latter is arising in the nasopharynx. The metastasis can look exactly like a lymphoma and the primary may be very small, even microscopic, and have been missed on ENT examination. This doesn't happen very often, but it does occur. Similar problems can arise with primary melanoma in the maxillary antrum. Again, this is rare but does happen. These are diagnostic problems; can flow cytometry help here? I'll illustrate some further problems and very serious dilemmas by a story of two patients (which could be entitled a Tale of Two Titties' and is an equally sad story) who presented with apparently identical disease. The human mind has an
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extraordinary capacity to recall anecdotal rare coincidental events, unlike the computer which is hopeless in this respect, but as certain aspects of the saga were so harrowing it's not surprising they made such an indelible impression and are still so readily recalled. It started in 1984 shortly after the SAC meeting in Asilomar. Two young women in the 30—35 age group presented on the same day having both had wide biopsy excisions of small lumps ( < 1.5 cm) in the upper outer quadrants of their right breasts. Both had had two children and both had been taking oral contraceptives intermittently during the previous 10—15 years. In neither case had there been skin involvement or deep tethering and neither had palpable lymph nodes in the axilla. In both cases there had been complete excision, as far as it was possible to tell, and the histological diagnoses were identical, moderately differentiated infiltrating duct carcinomas. Both patients were treated identically with radiation to the breast and gland areas and during treatment they became mutually supportive good friends which tends to occur with considerable intensity when people are under severe stress. One was dead within 10 months with generalized metastatic disease and the other is alive and well over 5 years later though she still suffers psychological trauma due to her friend's death and the realization that this could still happen to her. Obviously, these two cases were very different in spite of the superficial similarities, but were the tumours different or were the patients surrounding the tumours different? It was almost certainly a combination of the two; however, both factors are difficult to investigate although it has long since been a part of empirical oncological knowledge that faster growing tumours tend to be associated with a reduced chance of a successful outcome. Was the tumour growing faster in the patient who died? These are questions which relate to prognostic factors; can flow cytometry help us here? These two cases also illustrate a number of further classes of problems, one of which is therapy selection. With the benefit of the retrospectroscope we may ask if it was necessary to treat with post-operative radiotherapy the patient who survived. After all, the excision of the small lesion appeared to have been complete and there were no palpable lymph nodes which all added up to a favourable prognosis. The patient who died also fell into this category and the decision to treat her was correct but, clearly, radiotherapy was the wrong choice. This raises further points. Did she have microscopic disease in axillary lymph nodes which was not clinically apparent? If so, were the cells resistant to radiation and consequently survived to metastasize or had the disease undergone generalized metastasis before diagnosis? If this were the case then local radiotherapy was totally inappropriate and, in the present state of our knowledge, chemotherapy should have been employed. However, would this have made any difference and can flow cytometry help us with these types of problems? We can attempt to gain answers to some of these questions using clinical trials where one treatment modality or combination is compared with another. The problems with this approach are multi-fold. Firstly, many anti-cancer clinical trials are based purely on empiricism and there is insufficient basic knowledge available to make more than a random guess as to what treatment modalities or
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combinations are worth comparing. One is reminded here that if you give enough chimpanzees a type writer each and leave them for long enough they will type out, purely by chance, the whole of the works of William Shakespeare and probably the Bible as well. The clinical trial om'cionados may well, at this point, cry 'what about lymphomas, leukaemias, chorion carcinoma and teratoma'. And, indeed these are some of the few tumours which are curable by chemotherapy, but it is worth noting that the initial major advances in these tumours did not come about from clinical trials but by inspired guesses. Moreover, some of the other guesses were not well reported as they didn't work. The lack of real knowledge is the major contributor to the overwhelming vast excess of essentially negative results obtained from such multi-center clinical trial enterprises over the past quarter of a century. Moreover, most trials now seem to accept within the statistical design specification that there is likely to be a very small difference in results between comparative arms of such studies. This means that large numbers of patients, up to 25 000 in some examples, need to be 'recruited' (a highly used euphemism) to obtain statistically significant results. This is great for keeping cancer research statisticians employed and maintaining high turnover in the paper industry but bad for trees and most of the time it doesn't do the patients much good either. Those that fare particularly badly are the poor devils recruited to phase I toxicity studies where the aim is merely to determine the maximum dose of a new agent that can be achieved with no attempt or hope of obtaining any benefit for the patients in the trial. Obtaining fully informed consent from these patients, who are usually pre-terminal, is not usually sought with rigour as nobody would agree to enter such an experiment (current euphemism is 'study') if they were told the whole truth in straight forward, blunt and simple language which might run something like this. 'Mr Smith, you have known for sometime now that you have a cancer and that this is not likely to be curable. We have tried all the currently available treatment and the disease is still progressing. There is a new drug which has never been tried in human beings although we know the dose which kills 50% of rats, mice and some other animals. We don't know if it is likely to have any beneficial effects but we are certain it has side effects which could be very severe. What we want to do with you is give you increasingly large doses until we find out how bad the side effects are and how much humans can tolerate.' Would you say yes to this proposition if it had been spelt out as clearly as this? Moreover, I would submit that the realization that such large numbers are required for some trials is tantamount to admission of failure at the very outset. Even if a positive result from a clinical trial is obtained, and by positive I mean that it is shown that one form of treatment confers a survival advantage, the physician still has a problem. The results of the trial will say, for example, that at a given level of statistical significance (say 0.95) 20% of the patients will live 25% longer if treated according to protocol A compared with B. This isn't a great deal of help as we do not know which 20% of the total will benefit or even if the extra 25% of time is worth having from the patients' point of view, notwithstanding the fact that most of this 'gained' time will have been spent undergoing intensive and frequently very
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APPLICATIONS IN ONCOLOGY
toxic therapy. Perhaps the most telling statistic is that only 19% of Ontario cancer specialists would have consented to enter a chemotherapy trial for metastatic lung cancer (Mackillop et al, 1988). The major problem in the therapeutic management of cancer is that we do not know when we should intervene at the individual patient level. The population statistics obtained from clinical trial results cannot directly be applied to the patient who is consulting you and is in front of you at this very minute. As a further example let us suppose that a series of independent prognostic factors are available which tell us that 80% of patients with a given tumour do not require further intervention following surgical removal. We have a probability of 0.8 of being correct if we manage the whole of the group by observation alone and the vast majority of cancer therapists would be quite pleased with themselves if they had 80% five-year survival figures for the majority of the tumours they manage even if they didn't prescribe any treatment. But, what about the remaining 20% who are doomed to die with this philosophy? Equally, we may have prognostic factors which tell us that 60% of patients will survive if they are treated with adjuvant radiotherapy plus a particular chemotherapy regime. Again, in order to obtain fiveyear survival figures of 60% all patients within the group would have to be treated which means that 40% would be subjected to toxic intervention with no benefit. I don't want to give the impression that I am a disbeliever in clinical trials, in fact I believe in them absolutely as this is the only true and objective means of testing the efficacy of treatment. The problem lies in our depressingly considerable lack of real understanding of the processes involved in the diseases and the modulation of both abnormal and normal cell behaviour, let alone that of organ systems, by the treatments we employ. However, there is no need to get too depressed as very considerable technological strides have been made in the past 15 years which are enabling us to gain a better understanding of the biology. And here, I would like to draw your attention to the quotation from Whitehead at the beginning of the book,'... it is not the imagination of man that improves but his capacity to measure which increases ...'. Flow cytometric methods combined with those of biochemistry and of molecular and cellular biology are beginning to lighten the darkness by enabling us to measure, and some assay systems are emerging which may allow us to grasp the 'Holy Grail' of cancer therapy, individualized treatment specifically designed for and aimed at a given tumour within an individual patient. 15.1
Diagnosis
Flow cytometry has a very limited role in primary diagnostic decision making. A biopsy will be taken and subjected to standard histological procedures and interpretation and in the majority of cases the diagnosis can be made. Even where there is potential difficulty, e.g. neck lymph nodes where the tumour could be anaplastic carcinoma or lymphoma, flow cytometry still has little or no use. Antibodies to cytoskeletal elements can assist in making discriminations such as these using classical immunoperoxidase or immunofluorescence staining
DIAGNOSIS
349
(Ramaekers et al, 1982b, 1983) and these assays have been adapted for flow cytometry (Ramaekers et al, 1984, and see figure 12.18). The latter was completely convincing and produced very pretty data, but we may ask if flow cytometry was really necessary? The answer must be that it isn't as the simpler classical methods can cope with this perfectly adequately. If you happen to have a flow cytometer and time to spare then certainly do this type of assay but you wouldn't buy a cytometer just to do this particular job. 15.1.1 Leukocyte classification Flow cytometry has been used extensively in leukocyte and bone marrow immunophenotyping (Nicola et al, 1981; Hoang et al., 1983; Loken and Lanier, 1984; Watt et al, 1984; Loken, 1986; and see in leukocyte typing, 1984) and can be useful in subclassification within the lymphomas and leukaemias which is carried out after the primary diagnosis has been established. A large number of antibodies to various leukocyte cell surface differentiation determinants are now available and the list is increasing all the time. Immunological typing of lymphomas has been carried out for many years (Lukes and Collins, 1974). However, following the advent of monoclonal antibody technology (Kohler and Milstein, 1975) and the recognition of discrete differentiation stages in both T-cells (Reingertz et al, 1980) and B-cells (Nadler et al, 1982,1983) which can be identified with antibodies there has been an explosion in this field. Antibodies to these various differentiation antigens have been used extensively in the classification of lymphomas and leukaemias (Griffin et al, 1981; Anderson et al, 1984; Foon and Todd, 1986) and the role of flow cytometry, which can encompass multi-dimensional analyses (Civin and Loken, 1987; Terstappen and Loken, 1988), has recently been reviewed by Parker (1988). I'm not going any further with this as it is a whole book's-worth in its own right.
15.1.2 Cytological prescreening The technology can be of potential assistance in primary diagnostic procedures in screening where large number of cells, or large numbers of samples have to be analysed. Any automated system which is reliable could have a very valuable place in cytological prescreening. The problems with manual methods are considerable. They are labour intensive, skilful, tedious, repetitive and require a high degree of sustained concentration. Some of these factors are mutually exclusive for many individuals. One of the major problems, almost by definition, is that the vast majority of screening specimens are entirely normal. Assuming there are no problems with specimen collection and preparation (that's a big 'if') perhaps only one sample in every hundred is likely to be questionable let alone obviously malignant. Whenever the expectation of observing an event is low it is very difficult for the human mind to maintain concentration so that when eventually that event does present it is not missed. The objective in any automated instrumental system is to screen out the normal samples to leave the questionable and abnormal specimens for humans to make the decisions. If at the outset 99% of
APPLICATIONS IN ONCOLOGY
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Figure 15.1. Nuclearfluorescenceplotted against nuclear-to-cytoplasmic ratio calculated from the slit-scan profiles. The horizontal line represents the abnormal cell decision boundary.
specimens are normal and a machine can decide that 90% are normal then only 10% have to be looked at by humans. This has two advantages. Firstly, the expectation of seeing an abnormal specimen is increased 10-fold which helps to maintain concentration and increases performance and, secondly, it decreases the number of skilled 'cerebral units' required to perform a repetitive and boring task. Slit-scan flow cytometry which was described in section 8.1 has been used by Wheeless et al to analyse both gynaecological (1984) and bladder specimens (1986a) in an extensive experimental prescreening programme. The specimens were stained with acridine orange and total nuclear fluorescence was plotted on an individual cell basis against nuclear-to-cytoplasmic ratio calculated from the slitscan profiles of each cell. A typical example is shown in figure 15.1 where the horizontal line represents the abnormal cell decision boundary. No screening system (including humans) will be 100% effective all the time. The most important fundamental requirement of automated prescreening systems is that the number of false negative results, defined as a positive which the instrument fails to recognize, should be acceptably low. A second but less critical requirement is that the false positive rate, defined as being scored positive by the instrument when in fact it was negative, should not be unacceptably high. Exactly what constitutes acceptable low or not unacceptably high is debatable; however, if the false positive rate is very high there is little point in using an automated system as it will not be screening out a worthwhile proportion of the total. Wheeless et al. (1986b) have developed a statistical analysis system to evaluate their multi-parameter data and in 251 gynaecological specimens have achieved a
PROGNOSIS
351
1.2% false negative error rate at the expense of a 24% false positive error rate. This false negative error rate of 1.2% compares very favourably with human performance. The 24% false positive error rate means the 75% of normal specimens were correctly classified, which would cut down the manual screening needed to 25%. It would seem, therefore, that this is well worth pursuing. In the feasability programme for bladder prescreening a total of 153 irrigation specimens have been analysed (Wheeless et al, 1986a). Of the 38 normal specimens only four were classified as abnormal, a false positive error of 10.5%. Sixty nine specimens were derived from patients with transitional cell carcinoma grades 1—2 and 66 were correctly classified as abnormal, a false negative rate of 4.3%. A total of 17 specimens were derived from grade 2—3 lesions and all were classified correctly. Only eight cases of dysplasia were analysed and the instrument scored seven of these as abnormal. These results are also extremely encouraging particularly as the chance of obtaining a false negative twice from the same patient must be extremely small and, undoubtedly, we should look forward to having such instrumentation available within the next decade or so to assist in routine screening programs.
15.2 Prognosis The most extensively studied parameter in attempts to produce prognostic information using both image analysis and flow cytometric systems has been total nuclear DNA content. This gives encouraging results in a number of tumours and the advent of antibodies to oncogene-encoded proteins has added another dimension to this field and both of these are discussed.
15.2.1 DNA index DNA index (ploidy) has been studied extensively (Tribukait, 1984; Friedlander, Hedley and Taylor, 1984) and the spectrum of studies seem to fall into three categories. Those in common or relatively common tumours where a large number of different studies have been performed, those in common tumours where few studies have been performed and those in rare tumours. The first category includes tumours of the breast, ovary, colo-rectum and non-Hodgkin's lymphoma. This almost certainly reflects the feeling that we could be doing better with these tumours if we had better prognostic factors, an important point I will return to later. The second group includes lung cancer (one archival study up to the end of 1988) where the general impression is that there is little point in obtaining better prognostic factors as they won't make any difference. The last group comprises rare tumours which are of considerable academic interest. However, it was only with the advent of nuclear extraction from archival biopsies (Hedley et al, 1983) that such studies became practicable as the assay could be carried out in reasonable numbers of samples where the outcome is known. I'm not going to embark on an exhaustive review of this topic, and the following references are included to complement those in the remainder of this section: Alanen et al, 1989; Auer et al, 1984; Barlogie et al, 1978; Ewers et al, 1984;
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Fossa et al, 1984; Hedley, Friedlander and Taylor, 1985; Horsfall et al, 1986; Jakobsen et al, 1984; Lakhanpal et al, 1987; McGuire and Dressier, 1985; Merkel, Dressier and McGuire, 1987; Van den Ingh, Griffioen and Cornelisse, 1985; Volm et al, 1985; Wolley et al, 1982. The best overall agreement has occurred in ovarian cancer where a number of studies have reported that DNA index is an important prognostic determinant (Blumerfeld et al, 1987; Rodenberg et al, 1987; Friedlander et al, 1988; Kallioniemi et al, 1988b). Moreover, Kallioniemi et al {1988a) have shown that DNA index relates to histological features and have indicated that the proportion of cells with S-phase DNA content (referred to subsequently as S-phase fraction) may also be an important determinant (Kallioniemi et al, 1988b). Rodenberg et al. (1988) have carried out morphometric analyses with DNA index and found agreement and good prognostic significance. Trebeck et al (1987) have studied Brenner ovarian tumours and found elevated DNA indices in higher grade tumoups and some evidence suggests that the rare borderline malignancy tumours with elevated DNA indices are the more aggressive (Friedlander et al, 1984). Our group has carried out DNA index determinations in archival biopsies from 225 patients with ovarian cancer of epithelial origin, 6 patients with borderline low potential malignancy and 12 normal ovaries. All normal ovaries had diploid DNA content as did 5 out of 6 cases of 'borderline7 malignancy. The majority of cases of carcinoma, 170 out of 225, were aneuploid. There was a statistically significant difference in the distribution of aneuploidy, p < 0.001, between invasive carcinoma and normal ovaries, and between invasive carcinoma and those classified as borderline low potential malignancy, p < 0.025. There was no difference between normal ovaries and those of borderline malignancy, p>0.1. The five-year survival of patients with diploid tumours was 70% which compared with 22% for patients with aneuploid tumours, p < 0.001, and these data are shown in figure 15.2. The group of patients with well differentiated diploid tumours (n = 39) had the best prognosis with a five-year survival of 82%. In contrast, patients with poorly differentiated aneuploid tumours (n=119) had a very poor prognosis with a five-year survival of only 10%. The 50% survival probability of the group of patients with moderately and poorly differentiated diploid tumours {n = 16) was comparable to the value of 47% in the group with well differentiated aneuploid lesions (n = 51), see figure 15.3. These results are fairly typical for ovarian carcinoma. The position in breast cancer seems to be less clear. Cornelisse et al (1987), in a large series of over 560 patients, found that DNA index was a weak but significant prognostic factor. In contrast, in another large series of 354 patients there was no correlation between prognosis and DNA index (Dowle et al, 1987). Furthermore, Hedley et al (1987) with 490 patients and Kallioniemi et al (1987) with 93 patients reported that S-phase fraction was a more significant prognostic variable than DNA index. In advanced disease both hormone responsiveness (Stuart-Harris et al, 1984) and chemosensitivity (Masters et al, 1987) correlated with DNA index. In general, the breast cancer data suggest that proliferation is more important prognostically than the DNA index.
PROGNOSIS
353
0.2
0.0
1
2
3 Time (years)
4
Figure 15.2. Survival curves for ovarian cancer patients with normal DNA index (Dip) and elevated DNA index (Anu).
The overall results in colo-rectal carcinoma are somewhat similar to those in breast cancer. Armitage et al. (1985), Kokal et al. (1986) and Scott et al. (1987) have reported DNA index as an independent prognostic variable. Bauer et al. (1987) report that proliferation is the more important factor compared with DNA index in early stage disease, Quirke et al. (1987) suggest that both DNA index and S-phase fraction have prognostic implications in rectal cancer, Chang, Enker and Melamed (1987) in a small study of 30 patients report that the DNA index predicts for recurrence in rectal tumours and Blijham et al. (1985) found that both DNA index and S-phase fraction were prognostically significant in Duke's stage C disease. However, Finan et al. (1986) have shown that the prognostic significance of DNA index is lost in patients with widespread hepatic metastasis, a result which is not altogether surprising. DNA index (Banner et al., 1987) and both DNA index and Sphase fraction (Walloch, Solans and Herman, 1987) are reported to correlate with development of adenomas. These results were not unexpected as the proliferative activity of adenometa is increased compared with normal mucosa.
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354
n=39
2. "5 3
O 0.4
0.2
0.0
1
2
3 Time (years)
4
5
Figure 15.3. Survival curves for ovarian cancer patients according to histological grade and DNA index. Dip and Anu respectively denote normal and elevated DNA index. W and P signify well and poorly + moderately differentiated tumours respectively.
Non-Hodgkin's lymphoma, albeit relatively uncommon, has received fairly considerable attention. Bauer et al. (1986b) and Young et al. (1987) both report that S-phase fraction predicts for a bad prognosis and Macartney et al. (1986) found a greater risk of developing more clinically aggressive disease in the higher S-phase fraction tumours. In non-endemic Burkett's lymphoma the high DNA index tumours carried the worst prognosis (Lehtinen et al., 1987). Lung cancer, one of the commonest and most depressing tumours to treat has received relatively little attention, possibly for the reasons given in the introduction to this section. In the one archival study up to the end of 1988 which comprises 100 non-small cell tumours it was found that DNA index was a powerful prognostic factor (Zimmerman et al., 1987). DNA index studies have been carried out in a number of other tumours (recently reviewed by Hedley, 1989) including those arising in the ENT region
PROGNOSIS
355
(Kaplan et al, 1986; Tytor, Franzen and Olofsson, 1987; Sanders et al, 1988; Grace et al, 1988), malignant melanoma (Meecham and Char, 1986; Coons et al, 1987) and adrenal tumours (Bowlby, DeBault and Abraham, 1986; Amberson et al, 1987; Hosaka et al, 1988) where the results were generally consistent. DNA index and/or S-phase fraction correlated with prognosis and histology where the more poorly differentiated neoplasms showed elevated DNA indices. In carcinomas of the urinary system there have been some unexpected results though insufficient studies have been carried out to date. In bladder cancer, Murphy, Chandler and Trafford (1986) and Blomjous et al (1988) found correlation between DNA index, tumour grade and prognosis; however, Jacobsen et al (1987) have reported that a normal DNA index carried a poorer prognosis in advanced tumours. In renal adenocarcinoma Rainwater et al {1987b) in a series of over 200 cases found that DNA index was prognostically significant in well differentiated tumours, but Ekfors et al (1987) found that DNA index did not relate to survival in 96 cases. Some interesting results have arisen in studies of the blastomas. Tomita et al (1988) have found that elevated DNA index is a good prognostic factor in medulloblastoma. In neuroblastoma, Gansler et al (1986) have reported that elevated DNA index and low S-phase fraction are prognostically favourable. Results in nephroblastoma have shown that tetraploid tumours (DNA index = 2.0) carry a worse prognosis than diploid and aneuploid tumours (Rainwater et al, 1987a) and Schmidt et al (1986) correlated S-phase fraction and DNA index with aggressive behaviour. As a general summing up we can state that DNA index and/or S-phase fraction are important prognostic factors in most cancers. However, it should not go unmentioned that this was strongly suggested by the pioneering work of N. B. Atkin at the Gray Laboratory, Northwood, who measured DNA content in populations of individual nuclei with manual light absorption microscope techniques two decades ago (Atkin, 1972) which was well before flow cytometric techniques became generally available. Atkin and Kay (1979) were also the first to introduce the concept of multi-variate analysis for such studies as they had recognized that DNA index alone (modal DNA as they called it) was insufficient to make an absolute distinction between normal and malignant and between good and bad prognostic groups of patients. Recently, van der Linden et al (1989) have reported that multi-variate prognostic index analysis in breast cancer including nodal status, tumour size, mitotic activity plus DNA index gave better prognostic information than DNA index alone. The two major advances in this field in the past 10 years have been in automation with its more general availability and nuclear extraction from archival biopsies enabling retrospective studies to be carried out in even very rare tumours. However, although more assays can now be carried out more quickly than in Atkin's time we are still confronted with a number of technical and interpretive problems. Firstly, with the increased number of cells that can be analysed it is possible to obtain estimates of the fraction of cells with S-phase DNA content. I
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APPLICATIONS IN ONCOLOGY
would again, however, draw your attention to the distinction between percentage of cells with S-phase DNA content and percentage of cells in S-phase (see section 11.5.5). Perhaps more striking correlates would be obtained in prospective studies in which patients were to be given BrdU before biopsy as this is the only way to make this distinction. However, this would entail considerably more work than wax block extraction and would take very much longer. Secondly, the S-phase fraction, particularly if this is 'low', can be difficult to estimate reliably even with the 'best' computer software. This is due to a number of problems including overlapping of mixed diploid and aneuploid populations which is compounded further in archival material where thick sections have been cut as some nuclei will have been sliced. Furthermore, some of the commercial computer software packages are really not sufficiently sophisticated to cope with these types of data sets. I suspect that published reports in this field which have only addressed DNA index and not S-phase fraction were limited by software capability. Nevertheless, if the S-phase fraction can be estimated reliably and if it gives meaningful correlations which can be used clinically it may not be necessary to make the distinction between fraction of cells with S-phase DNA content and percentage of S-phase cells.
15.2.2 Oncogenes It has been my opinion for some time that DNA index and/or S-phase fraction will not be sufficiently reliable to make good enough distinctions between good and bad prognostic groups to influence patient management. Because of this, which I freely admit is a prejudice and not based on scientific considerations, our group embarked on studies to see if measurement of oncogene-encoded proteins could give additional information. In order to 'set the scene' I'll begin with a brief review of this field. The human genome contains a number of genes which may be involved in the aetiology of cancer (Bishop, 1985; Varmus, 1984; Slamon, 1987). These segments of DNA, the proto-oncogenes, came to light from the pioneering work of Peyton Rous (1911) who discovered that chicken sarcomas could be transmitted by cellfree extracts. In 1951, Gross showed that a retroviral agent was responsible for a murine leukaemia and since then a number of transmittable tumours in higher vertebrates have been shown to be due to retroviruses including Rous sarcoma. The retrovirus genome is composed of RNA and is small with only three genes. These are called gag, pol and env and they code for core protein, a reverse transcriptase (Baltimore, 1970; Temin and Mizutani, 1970) and the viral envelope respectively. When a cell is infected, the viral RNA is handled in exactly the same way as the cell's normal RNA and it is translated to protein. The reverse transcriptase product of the pol gene can now splice a new segment of DNA into the host cell genome which is complementary to the viral RNA. Many rounds of transcription are induced and viral RNA identical to that initially infecting the cell is produced. Core protein and envelope are manufactured simultaneously and amplification of the virus takes place which is released on rupture of the cell.
PROGNOSIS
357
Not all retroviruses are oncogenic, but most that are contain an extra gene. These 'one-genes have three-letter acronyms, for example sre, erb and myc stand for Rous sarcoma, chicken erythroblastosis and chicken rat/elocytosis respectively. The retroviruses tended to be regarded as curiosities with little or no relevance to human cancer until the key discovery was made by Stehlin et al. in 1976 where it was shown than normal cells contain segments of DNA which are structurally very similar to the retroviral v-src gene. After this progress was rapid and many of the retroviral oncogenes were found to have cellular counterparts which were very similar though not identical (Bishop and Varmus, 1982). Furthermore, not all oncogenes have retroviral homologues. This had lead Coffin et al. (1981) to propose that the identifiers of the retroviral oncogenes should be prefixed with V-' to distinguish them from cellular oncogenes to be prefixed with 'c-'. We now know that one class of oncogenes encode proteins which are intimately involved in growth regulation at the levels of extracellular signal transmission (c-sis, platelet-derived growth factor, Doolittle et al., 1983; Waterfield et al, 1983); signal reception and transduction across tne external membrane (c-erbB, epidermal growth factor receptor, Downward et al, 1984, and c-fms, receptor for colony stimulating factor 1, Roussel et al, 1984; Scherr et al, 1985); intracellular signal transmitters (N-ras, Wakelman et al, 1986, product related to G-proteins, Hurley et al, 1984) and nuclear signal receivers and/or transducers (v-erb-A, thyroid hormone receptor, Sap et al, 1986; Weinberger et al, 1986, which has extensive homology with oestrogen receptor, Green et al, 1986). Further likely candidates for nuclear transducers are the proteins encoded by myc, fos and myb, which have DNA binding capacity and p55c~fos has been shown to be involved with transcription (Distel et al, 1987; Lech et al, 1988). A second class of 'oncogenes' has now been identified as tumour-suppressor genes where loss of normal function is associated with tumour formation. This possibility, which in engineering terms would be described as the failure of a negative feedback servo control loop mechanism, was considered by Comings (1973) and has now been identified in a number of hereditary human tumours (Knudson, 1983, 1985). The first suspicion that hereditary factors might be involved in cancer was voiced by Norris (1820) based on observations of what was probably malignant melanoma in successive generations of the same family. Familial polyposis coli (McKusic, 1962; Ashley, 1969) carries a well defined risk of carcinoma development which, at a given age, is about three orders of magnitude greater than that in the remainder of the population. Another good example is retinoblastoma (Knudson, 1971, 1978) where a visible deletion involving band 14 on the long arm of chromosome 13 (13ql4) is found in a small proportion of cases (Knudson et al, 1976; Yunis and Ramsay, 1978). It is now established that the genetic abnormalities in retinoblastoma are not random (Benedict et al, 1983a) and that predisposition is a recessive inheritance via one affected and one normal chromosome 13 with the gene located at 13ql4 (Benedict et al, 1983b; Cavenee et al, 1983). Development of the neoplastic phenotype is a consequence of somatic mutation at 13ql4 in the normal chromosome and hence complete loss of the
358
APPLICATIONS IN ONCOLOGY
retinoblastoma suppressor gene function. Increasing evidence suggests that p53, discovered a decade ago (Lane and Crawford, 1979; Linzer and Levine, 1979) also has tumour-supressor function (Wolf and Rotter, 1985; Masuda et al, 1987; Munroe et al, 1988; Finlay, Hinds and Levine, 1989; Hinds, Finlay and Levine, 1989; Banker et al, 1989) where mutation of the gene or conformation changes in the normal protein contribute to transformation. The fundamental pathological diad of cancer is disordered proliferation and the capacity of malignant cells to metastasize. The genes discussed so far are obviously concerned with proliferation control and probably also with control of differentiation. Further discoveries have potentially linked the metastasis phenomenon with disordered functioning of oncogenes encoding cytoskeleton elements. The v-fgr gene encodes a hybrid protein containing a portion of the actin molecule (Naharro, Robins and Reddy, 1984) and onc-D codes for a non-muscle tropomyocin (MartinZanca, Hughes and Barbacid, 1986). This would seem to be highly significant as it might signify a third category of 'oncogenes7, those concerned with sub-cellular architecture and hence possibly with metastatic potential, to complement those involved with proliferation. Most studies involving the oncogenes carried out to date in both tissue culture and in human cancer have relied upon hybridization techniques. These methods, particularly for mRNA, require fresh tissue which is not always obtainable in sufficient quantities from cancer patients. Also, it may take a considerable time to accumulate sufficient material and information to make meaningful clinical correlates with fresh tissue. This applies particularly to the rare tumours. Moreover, neither the gene nor its message is the effector molecule; this is the province of the protein and monoclonal antibodies directed to specific oncoproteins have been developed. Examples include p53 (Harlow et al, 1981), p21 c ~ras (Furth et al, 1982) and p62c~myc (Evan et al, 1985). Herein lie possibilities for clinical applications using protein probes for not only body fluids but also biopsy material. Studies with the former indicate the potential for oncoproteins to become a new generation of tumour markers. Crawford, Pirn and Bulbrook (1982) have detected antibodies against the cellular protein p53 in sera from patients with breast cancer. Antipeptide antibodies have detected and compared oncogene-related proteins in urine in normal subjects, pregnancy and in cancer patients (Niman et al, 1985). Similar studies have been conducted using an antibody to the c-myc protein. A 40 000 da breakdown product of p62c~myc was detected in cancer patients and in pregnancy (Chan et al, 1987). Such antibodies have been used not only for immunoprecipitation and Western blotting, but also for immunocytochemical localization in biopsies of both frozen and formalin-fixed normal and tumour tissue. They have been used to define differential ras gene expression in malignant and benign colonic disease (Thor et al, 1984). Slamon et al (1989) studied HER-2/neu expression in breast and ovarian cancers and found good correlation between immunocytochemical staining, Western blotting and both DNA and mRNA hybridization signals. However, these investigators stress that it is important to identify which antibodies can be
PROGNOSIS
359
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Time (days) Figure 15.4. HER-2/neu expression and survival probability in ovarian cancer where the top panel is for gene copy number and the bottom panel is for the protein product assayed immunocytochemically. used in formalin-fixed biopsies, and frozen sections had to be used for their immunocytochemistry as completely negative staining was observed after formalin fixation. Patient survival correlated inversely with HER-2/neu gene amplification and its protein expression in ovarian cancer and these data are reproduced in figure 15.4. Immunocytochemical studies with an anti-p62 c ~ mK monoclonal antibody, Myc 1-6E10, have shown that normal testis expressed only small amounts of the protein. Seminomas exhibited increased nuclear and cytoplasmic staining. Undifferentiated teratomas showed barely detectable staining whereas well differentiated epithelial structures and yolk-sac elements exhibited intense staining (Sikora et al, 1985). Normal colonic mucosa exhibited maximal expression in the maturation zones of the crypts of Lieberkuhn where there was mixed nuclear and cytoplasmic staining (Stewart et al, 1986). However, p62c~myc is known to be nuclear associated (Evan and Hancock, 1985) and in further more extensive studies it was shown that this protein is redistributed from a nuclear to a cytoplasmic location with increasing maturation of the normal colonic mucosa (Sunderesan et al, 1987). This has also been seen in mucosa freshly
APPLICATIONS IN ONCOLOGY
360
fixed within seconds of biopsy (Forgacs et al, 1986) and active exclusion of the protein from the nucleus may be part of the normal control mechanism for regulating proliferation and differentiation. In familial polyposis coli, which inexorably progresses to the malignant invasive phenotype, nuclear staining persisted to the surface of the crypts and in carcinomas the staining was predominantly nuclear (Sunderesan et al, 1987). Immunocytochemical techniques have the advantage that the architecture is preserved but they suffer from the disadvantage of poor quantitation; however, the careful work of Slamon et al. (1989), see figure 15.4, was able to effect a discrimination into low', 'medium' and 'high' HER-2/neu protein expression which had meaningful clinical correlates. Fluorescence quantitation of p62 c~myc and DNA simultaneously was developed in our laboratories to study a number of tumours using flow cytometry in an attempt to overcome some of these problems (Watson et al, 1985b). The technique was adapted from that of Hedley et al (1983) and uses pepsin to release nuclei by cytoplasmic digestion after dewaxing and rehydration (see section 7.1.3). As the c-myc protein is nuclear associated (Evan and Hancock, 1985) it can be stained with the Myc 1-6E10 antibody after nuclear 1000H
800
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o
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600-
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o
a
o
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NOR
SEM
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Figure 15.5. Levels of p62 ~ in normal testis (NOR) and testicular cancer. Both semonomas (SEM) and teratomas exhibited elevated levels. In the latter the p62c~myc increased with increasing differentiation from MTU (malignant teratoma undifferentiated) to MTI (malignant teratoma intermediate) to MT + YS (malignant teratoma with yolk sack elements).
PROGNOSIS
361
extraction. However, very great care must be exercised with this method for the reasons given in section 7.3.4 and if you've forgotten what they are please read that bit again. Low p62c~myc levels were found in normal testicular tissue and significantly elevated levels were found in both teratoma (p < 0.001) and seminoma (p < 0.001). However, the oncoprotein level increased significantly with increasing differentiation in teratoma (p<0.01). These data are shown in figure 15.5. Patients who developed recurrence and died within three years of diagnosis had lower levels than those who were disease free since their initial treatment, p < 0.001 (Watson et ah, 1986) and these results are shown in figure 15.6. Somewhat similar results were obtained in colon neoplasia (Watson et ah, 1987c). Normal mucosa and polyps from non-malignant specimens exhibited lower p62c~myc levels than carcinomas (/?<0.02) but there was a wide spread in the latter as can be seen in figure 15.7.
1000n
800
600-
o CM CD
a
400-
200-
A/W
R/D
Figure 15.6. Comparison of p62c~myc levels in testicular cancer patients who developed recurrence and died (R/D) within three years of diagnosis with those who were disease free (A/W) at three years. Seminomas and teratomas are represented by the open and closed symbols respectively.
362
APPLICATIONS IN ONCOLOGY uuu-
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N HISTOLOGY Figure 15.7. Increasing expression of p62c~myc mucosa to polyps then to carcinomas.
levels from normal colonic
Villous adenometa (pre-malignant) exhibited elevated levels as did morphologically normal mucosa from specimens containing a carcinoma. There was also a tendancy for p62c~myc levels to fall as the tumours became more poorly differentiated, a finding which was corroborated in parallel studies with Northern blotting for mRNA (Sikora et al, 1987). Comparison of normal with dysplastic mucosa and carcinomas developing in patients with ulcerative colitis have shown that the nuclear p62c~myc content increased with the transition from 'mild' to 'severe7 dysplasia (Forgacs et al, 1986), results which are shown in figure 15.8. Moreover, the protein content was raised in morphologically normal colonic mucosa derived from malignant compared with non-malignant specimens (Watson et al, 1991b). We have also studied some gynaecological malignancies using these methods and aneuploidy with a well defined Gl peak was not observed in a total of 127 biopsies of uterine cervix neoplasia (Hendy-Ibbs et al, 1987). Normal biopsies exhibited higher p62c~myc levels than carcinomas, p< 0.000 01, and there was a progressive decrease in oncoprotein level with progression from cervical intraepithelial neoplasia, CIN I to CIN III, p<0.05 as shown in figure 15.9. Furthermore, the maximum fluorescence signal in the normal tissues occurred at a lower antibody concentration compared with tumour tissue, p<0.000 01. There
PROGNOSIS
363
70006000o o § 5000-
o
(0
2 400030002000H 1000-
NORMAL CHRONIC COLON U.C
MILD SEVERE DYSPLASIA
CARCINOMA
Figure 15.8. Comparisons of normal colonic mucosa, quiescent mucosa in ulcerative colitis, dysplastic mucosa in the latter mild and severe and invasive carcinomas developing in patients with ulcerative colitis.
was no correlation with histological grade, stage, age or prognosis in patients with invasion. Serious papillary ovarian carcinoma expressed significantly higher p62 c " m y c levels compared with normal ovary, p < 0.000 03 (Watson et al., 1987a). Biopsies classified as 'borderline low potential malignancy' exhibited levels between normal ovary and carcinoma. The difference between normal and borderline was significant at p < 0.003, but no difference between borderline and frankly invasive biopsies was observed, p = .149. There was no difference between the histological grades of carcinomas. All normal ovaries had diploid DNA content as did 5 out of 6 cases of 'borderline' malignancy. The majority of cases of carcinoma, 28 out of 36, were aneuploid. There was a statistically significant difference in the distribution of aneuploidy, p < 0.005, between invasive carcinoma and those classified as borderline low potential malignancy. These results are summarized in figure 15.10 which shows p62c~myc levels for normal, borderline and invasive carcinoma. It would seem that elevation of p62c~myc preceded the development of aneuploidy in the evolution of the malignant phenotype in ovarian cancer; however, there is no evidence to suggest that these are causally related. The findings in colonic neoplasia, seminoma and ovarian cancer were partially anticipated but those in both carcinoma of the cervix and in the histological breakdown of teratoma were completely contrary to initial expectation. However, an increase in either the gene or mRNA copy number (or both), which should give
APPLICATIONS IN ONCOLOGY
364
2520-
10 50 10 (0
c
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5
0 10 5
-P.
Figure 15.9. Decrease in p62c ~ myc levels with 'progression' from normal cervical mucosa (panel A) to invasive carcinoma (panel E). Panels B, C and D were obtained from patients with intraepithelial neoplasia, CIN I, CIN II and CIN III, respectively. rise to an increased protein production rate, need not necessarily be reflected in a marked increase in the total protein content for two main reasons. Firstly, inappropriately increased message may result in rate limitation at the protein synthesis level. Secondly, an increase in protein degradation may offset an increased production rate. The latter is most likely to occur with a protein which has a short half-life and, clearly, this is a distinct possibility for p62c~myc with a half-life of 20—30 minutes in rapidly cycling and stimulated cells (Greenberg and Ziff, 1984; Rabbitts et al., 1985). Hence, the lower absolute levels in carcinoma of the cervix compared with normal and undifferentiated compared with the better differentiated teratomas, may reflect an increased protein turnover and an increased cell production rate in the former. Further possibilities include posttranslational protein modification in the more malignant teratomas and in cervical
PROGNOSIS
365
7000H
6000-
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Figure 15.10. Levels of p62c ~ myc in normal ovaries (N), borderline tumours (B) and invasive carcinoma (C). The closed circles represent lesions with elevated DNA indices. The normal ovary square symbols represent the oncoprotein levels in elements predicted to be normal cells in tumour specimens where this component constituted more than 25% of the whole specimen. carcinoma giving rise to an alteration or partial occlusion of the epitope recognized by the antibody and a possible increase in the susceptibility of the protein to proteolysis in neoplastic cells in the preparation for the assay. There is a small shred of evidence that post-translational protein modification may occur in cervical carcinoma. Maximum binding was observed at different antibody concentrations in the normal and malignant cells which might indicate a change in binding constant. An interesting feature of the cervix study was the apparent absence of aneuploidy. However, 30% of neoplastic specimens had a positive skew to the diploid spike which could have been due to a small proportion of cells with a 5 to 10% increase in DNA content although in no specimen was there a well defined second peak. These may have represented aneuploid components which the method was not able to resolve in these particular specimens.
366
APPLICATIONS IN ONCOLOGY
We have seen in section 15.2.1 that DNA index can be a bad prognostic factor in a number of tumour types but not all patients with diploid tumours have a good prognosis. Part of our work to quantitate oncoproteins simultaneously with DNA was attempting to help with this distinction and indeed highly significant differences in p62c~myc levels were observed between good and bad prognostic groups of testicular cancer patients. However, inspection of figure 15.6 reveals considerable overlap and it would not be possible to assign patients with certainty to good and bad prognostic groups with these data even though 'p was less than 0.001. As can be seen the problem lies with the low values which completely overlap in the good and bad prognostic group. The results obtained in ulcerative colitis (figure 15.8) are more encouraging where a considerable increase in p62c~myc levels occurred with progression from mild to severe dysplasia which from a clinical standpoint is exactly where the physician would like to be alerted that something is going wrong. However, we have to ask if the p62 c ~ myc levels are telling us anything we don't already know. I suspect that they are not as the histological distinction between mild and severe dysplasia is relatively easy to make histologically. Perhaps we should look in detail at the mild dysplasias with high p62 c ~myc levels in prospective studies to see if this gives us an indication that the mucosa is in the process of turning to severe dysplasia. Nevertheless, these results were encouraging. The ovarian cancer results of Slamon et al. (1989) with immunoperoxidase staining for HER-2/neu are also encouraging. However, there are many more parameters which could be measured. These include a whole battery of nuclear-associated oncogene-encoded proteins, quite apart from p62 c ~mycf and cell surface receptor status (EGFr and oestrogen receptor; Sainsbury et al, 1985) which may provide additional data in a number of tumour types to make more reliable distinctions between good and bad prognostic groups of patients.
15.3 Therapy selection It is quite clear from the types of studies and results carried out to date, and outlined in the previous two sections, that multi-parametric information with multi-factorial analysis will be required to effect a sufficiently reliable predictive discrimination between good and bad prognostic groups to influence clinical therapeutic judgements. I do not believe it is justifiable at present, or that it will be in the future, to base therapy judgements merely on univariate analysis of DNA index data. Moreover, even when we can distinguish absolutely between good and bad prognostic groups, and I believe we will be able to do this, it's not entirely clear what we are going to do with the patients in the bad prognostic groups as, apart from some rare exceptions, we tend to use our most aggressive therapy at the outset and treat to established normal tissue tolerance. If assays, or assay systems, are developed which can tell us that a particular 'biochemical profile' of a tumour with a particular therapy regime is going to give us close to 100% success then there is no need to change the treatment. However, this is probably not a
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realistic possibility for the majority of human cancers with the currently available treatment strategies. It seems to me to be a relatively pointless exercise in becoming better and better at predicting the good prognostic groups of patients whose numbers will become smaller and smaller if we cannot improve therapy for the bad prognostic groups whose numbers will become bigger and bigger as a consequence of the improved classification. Reclassification does not, in itself, improve results as, by definition, it just places patients in different categories. This may make us feel more comfortable when we look at the results from the good prognosis groups but less comfortable with the results from the bad prognostic groups which alerts us to the problem. One good example is the redefinition of the lymphomas into Hodgkin's and non-Hodgkin's categories and the substratifications into low and high grades. This gave rise to more aggressive chemotherapy for the high grade non-Hodgkin's tumours and somewhat less aggressive therapy for the low grade tumours in each major subdivision. If we are to make comparable advances in the more difficult 'solid' tumours, the big three Bs, breast, bronchus and bowel, we must think in terms of quantitative comparative subcellular biochemical measurements in normal and malignant cell not only for developing new drugs and therapy combinations but also in attempts to minimize administration of ineffective therapy. The latter would at least spare a large number of patients very considerable toxicity which many, usually the relatives, would consider a positive gain in a very negative environment. The assay systems described in the next three sections are possible ways in which these approaches could be addressed. 15.3.1 GSH metabolism Oxygen can be dangerous stuff when handled incorrectly. This also applies in aerobic biological systems as normal oxygen metabolism produces some peroxides and superoxides during energy releasing steps. These highly reactive short lived species can be very damaging to a number of cruicial targets, including DNA, and aerobic organisms have developed ways and means of coping with these potential threats. One of these mechanism is the tripeptide glutathione containing a sulphydryl group (—SH—) in the cysteine residue which 'mops-up' reactive radicles. Highly metabolically active cells can contain up to 15% of their total molar content as glutathione. Reduction of intracellular glutathione can increase sensitivity to not only radiation (Bump, Yu and Brown, 1982; Malaise, 1983; Clark et al, 1984; Schrieve, Denekamp and Mitchinton, 1985) but also cytotoxic agents (Babson, Abell and Reed, 1981; Roizin-Rowle etal, 1982; Ono and Schieve, 1986). These observations have potentially important clinical implications as exemplified by the very limited work we have carried out to date. The normal range for GSH estimation was established for lymphocytes from a number of normal individuals in our laboratories using mClB as described in section 14.2.4 and two patients with leukaemic central nervous system involvement have also been studied. These results are given in figure 15.11 where the peripheral lymphocytes from the two
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10
100
200
300
400
500
Time (seconds) Figure 15.11. Bluefluorescencedevelopment for the conjugation of GSH with monochlorobimane in normal lymphocytes (closed symbols with 2 standard error limits) and in peripheral lymphocytes from two patients with CNS leukaemic involvement refractory to irradiation. patients are compared with lymphocytes from the normal subjects. Both patients (open symbols) were well above the two standard error limits of the normal range. Both had had intensive chemotherapy previously and both were totally refractory to CNS radiation and died without exhibiting any response. These results are nothing to shout about yet but lymphatic leukaemia lymphocytes are usually sensitive to radiation. This begs the question: had the genes which encode the enzymes responsible to GSH production (y-glutamic acid transferase and glutathione synthatase) undergone adaptive amplification in response to the previous chemotherapy and produced increased intracellular levels of GSH and hence induced radiation resistance? This is a distinct possibility as gene amplification can occur very rapidly under some circumstances. Rice, Hoy and Schimke (1986b) have reported that even transient hypoxia can cause amplification of the dihydrofolate reductase gene. Perhaps in future it would be advisable to assay the lymphocytes of such patients for GSH at intervals during chemotherapy to monitor any changes that might occur and to assay for gene amplification if changes are noted. If this did occur and subsequent CNS involvement developed which required radiation then thiol depleting agents possibly could be employed.
15.3.2 Drug resistance The development of anti-cancer drug resistance was first described 40 years ago by Burchenal et al. (1950). Mechanisms in drug resistance include decreased cellular influx, increased efflux, increased catabolism, increases in competitive inhibitors, changes in the partitioning of drug within intracellular compartments, alteration of intracellular targets, reduction of DNA damage and gene amplification. Some of the transport and resistance mechanisms involving
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anthracyclines and methotrexate have been mentioned or considered in section 14.6 and mechanisms involving some of the other anti-cancer drugs are considered here. Goldenberg et al. (1970) demonstrated that transport of nitrogen mustard (HN2) into cells was mainly an active process mediated by a carrier molecule and their data suggested that HN2-resistant mutants were deficient in the carrier. It was then shown in HN2-sensitive and resistant cells that this was the carrier for choline (Goldenberg, Vanstone and Bihler, 1971). Study of cells sensitive and resistant to chlorambucil have revealed a resistance mechanism which is not related to transport as the kinetics of uptake were identical in the two cell types (Harrap and Hill, 1970). Drug uptake in both resistant and sensitive cell lines was temperature independent, directly proportional to concentration and unaffected by ouabane and metabolic inhibitors all of which strongly support passive diffusion as the means of transport (Hill, 1972). However, alkylating activity declined at over double the rate in the resistant cells with decreased binding to DNA, RNA and proteins (Hill, 1972) which are all indications of increased intracellular metabolism of the drug in resistant cells. Passive diffusion is also the means by which the nitrosoureas, CCNU, BCNU (Begleiter, Lam and Goldenberg, 1977) and chlorozotocin (Lam, Talgoy and Goldenberg, 1980) gain access to the cell interior as the uptake of each is unsaturable, independent of temperature and unaltered by metabolic inhibitors. The esterase inhibition kinetic assay described in section 14.2.7 is a potential means of assessing not only transport of nitrosoureas and related isocyanates across the external membrane but also the damage they do having gained access. Some cells are resistant to nitrosoureas but as yet we have scant knowledge of the mechanisms involved. Schabel et al (1978) have studied resistance to alkylating agents and cross-resistance with nitrosoureas. A cell line totally resistant to cyclophosphamide retained sensitivity to BCNU, CCNU and methyl-CCNU. BCNU-resistant cells exhibited no cross-resistance with cyclophosphamide or melphalan, but a melphalan-resistant line showed partial cross-resistance with chlorozotocin and cyclophosphamide, complete cross-resistance with ris-platin but no resistance to BCNU, CCNU or methyl-CCNU. The uptake of phenylalanine mustard (PAM, melphalan), a derivative of HN2, is an active process but it does not share the choline pathway with HN2. PAM cytotoxicity can be reduced by co-incubation with a number of amino acids, an effect first reported by Vistica, Toal and Rabinowitz (1976) with L-leucine and L-glutamine. This, and further evidence (Vistica, Toal and Rabinowitz, 1978) suggested that PAM and leucine share a common carrier molecule. Melphalan resistance has been noted in a colchicine-resistant clone of Chinese hamster ovary (CHO) cells, CHRC5, initially isolated by Ling and Thompson (1974). These cells were also cross-resistant with nitrogen mustard, chlorambucil, adriamycin and puromycin and Ling, Gerlach and Kartner (1984) used the term multi-drug resistance (MDR) to describe this phenotype. During the past 15 years cross-resistance or multi-drug resistance, which is
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thought to be a major cause of failure in cancer chemotherapy, has been recognized increasingly. The phenomenon is characterized clinically by good responses to primary cytotoxic chemotherapy but poor responses on relapse not only to the drugs used initially, but also to others not used in the primary therapeutic schedule. The development of 'classical' multi-drug resistance (MDR) as described by Ling et al (1984) occurred during in vitro selection and a number of mechanisms have been proposed. These include changes in the intracellular drug distribution (Supino et al, 1986), modified membrane transport (Skovsgaard and Nissen, 1982), reduced DNA cleavage (Glisson et al, 1986; Capranico, Dasdia and Zunino, 1986; Supino et al., 1988), altered drug target sites (Potmesil et al., 1988) and the capacity to secrete drugs using energy dependent active efflux mechanisms. The MDR phenotype described by Ling et al. (1984) correlated with the presence of a high molecular weight membrane-associated glycoprotein (Juliano and Ling, 1976; Carlsen, Till and Ling, 1976). Initially, it was postulated that resistance was conferred by reduced drug accumulation due to decreased influx (Ling and Thompson, 1974; See et al, 197A). However, the drugs involved in the MDR phenotype are very different and have different influx pathways all of which would have to be involved. Moreover, enhanced efflux of actinomycin-D, vincristine and vinblastine occurs in adriamycin-resistant P388 cells (Inaba and Sakurai, 1979). These various considerations suggested a common efflux pathway and that MDR may be due to increased efflux mediated via an energy-dependent carrier-mediated transport pathway involving the 170 kda membrane located glycoprotein, gp 170 . Anthracycline secretion has been studied extensively in both sensitive and resistant cells (Dano, 1973; Skovsgaard, 197Sa,b,c; Di Marco, 1978; Inaba et al, 1979) and gp 170 involvement has been confirmed in some (Riordan and Ling, 1985), but not all (Slovak et al, 1988; Mirski, Gerlach and Cole, 1987) cell lines exhibiting MDR. Energy-dependent active efflux is supported by studies with the calcium channel blocking agent verapamil which can partially overcome some resistance and cross-resistance (Tsuro et al, 1982; Twentyman, Fox and Bleehen, 1986a). In the latter studies it was shown that the degree of resistance to adriamycin was indirectly proportional to verapamil concentration. However, there may well be many drug-resistance pathways (Warr, Anderson and Fergusson, 1988) and Beck et al. (1986) have shown that vinka alkaloid resistance but not multi-drug resistance is reversed by verapamil in human leukaemic cells. The gp 170 is encoded by the mdr-1 gene and its expression varies considerably in different normal tissues (Fojo et al, 1987), perhaps reflecting variation in tissue requirements for excretion of toxic substances (Nelson, 1988). Amplification of this gene has been described in a multi-drug-resistant small-cell lung cancer cell line, H69/LX4, (Reeve, Rabbitts and Twentyman, 1989) which was developed in our laboratories from the parent NCIH69/P (Twentyman et al, 1986b). Hybridization techniques (Southern, 1975; Thomas, 1980) and Western blotting can be used to study gp 170 at the gene, message and protein levels; however, these methods have two major disadvantages. Firstly, they cannot assay
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for functional activity. Secondly, they cannot identify minority subsets in heterogeneous populations as only the grand average for the whole population can be determined. Chemotherapy may select for pre-existing multi-drug resistance in a minority subset within a tumour, a view supported by the work of Ross et al (1988) where highly multi-drug-resistant P388 cells were isolated from a drug-sensitive population by flow cytometric cell sorting. It is very unlikely that this minority subset would be apparent using blotting techniques. For example, if there was mdr-1 gene amplification of 10-fold in a minority subset comprising 1% of a tumour, which is not an unlikely scenario, we would obtain a 9% increase in hybridization signal in the tumour specimen compared with a control. Southern hybridization techniques could not hope to make this distinction. The same arguments apply to similar analysis of mRNA. Furthermore, message copy number need not relate quantitatively to the number of gp 170 molecules in the membrane as translation to protein could be rate limited particularly in the unfavourable environments in which tumour cells frequently find themselves. The need to develop techniques to overcome these problems is self-evident. However, apart from the requirement to measure the functional activity of gp 170 in minority subsets of heterogeneous samples it would also be desirable to be able to perform the assays on relatively small biopsy samples in viable cells under near physiological conditions. Two flow cytometric kinetic methods which meet these requirements are now available. One is 'indirect' and due to Morgan et al (1987, 1989) and the other is 'direct' and due to Herweijer, van den Engh and Nooter (1989). The 'indirect' assay involves the use of the bisbenzimidazole DNA dye Hoechst 33342 whose cellular uptake parallels that of a number of cytotoxic agents involved in multi-drug resistance and hence correlates with sensitivity to those agents (Lalande, Ling and Miller, 1981). Furthermore, Hoechst 33342 uptake is modified by verapamil (Krishan, 1987) and it is possible that the dye is secreted by cells via the gp 170 pathway. We saw in sections 8.4.3 and 11.8 that the fluorescence emission spectrum from the DNA/Hoechst 33342 complex varies in different cell types (Watson et al, 1985a; Smith et al, 1985). It is dependent on the dye: DNA—phosphate ratio and pH (Smith et al, 1985) and it has been used as a means of sorting viable cells on DNA content (Arndt-Jovin and Jovin, 1977; Hamori et al, 1980; Lydon et al, 1980). These considerations prompted an investigation of the possibility of using Hoechst 33342 as a reporter probe for MDR in viable cells by monitoring the fluorescence emission spectrum on an individual cell basis. It was anticipated that this analysis might be more demanding in MDR cells than in bone marrow or thymocytes (which it was, see sections 8.4.3 and 11.8) and the instrument was modified to give greater resolution. Data were collected from a minimum of three photomultipliers each guarded by 10 nm narrow band-pass filters for simultaneous analysis in the violet (395-405 nm), blue (495-505 nm) and red (595—605 nm) regions of the spectrum. Some studies also included the addition of the indigo (445—455 nm) and green (545—555 nm) channels and measurement
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on such narrow band-passes required the high-efficiency light collection flow chamber (Watson, 1985). Forward and 90° light scatter signals were also collected as a means of helping to identify debris and clumps of cells (Watson et al., 1985b). The cell throughput rates were reduced to between 250 and 350 cells per second and the data were collected list-mode on disc which were later processed with a VAX S600 computer. The photomultiplier voltages, amplifier gains and thresholds of the instruments were set using control samples stained for 1 hour so that the easily defined Gl peak was placed at the same scale position on each photomultiplier analysis channel. Subsequent fluorescence from the test samples could then be compared with the control on each analysis channel to give a measure of relative changes in the emission spectrum. A total of 10 4 cells was analysed for each data set. A number of multi-drug-resistant cell lines have been developed in our laboratories and these were used in the investigation. Single-cell suspensions were obtained by treating wth 0.4% trypsin plus 0.02% versene and the concentrations were adjusted to 2 x 105 cells ml""1 in growth medium. A stock solution of Hoechst 33342 was dissolved in distilled water at a concentration of l m M . Aliquots of cells were stained by adding 10 jil of the stock solution to 1 ml of the cell suspensions to give a final stain concentration of 10 |iM. The cells were then incubated at 37 °Cin the dark. Verapamil, when this was used, was added to give a final concentration of 3.3 |iM. Time courses for the development of violet (400 nm, left panel) and red (600 nm, right panel) flourescence in the H69/P and LX4 cell lines are shown in figure 15.12 where the closed and open symbols represent the results from the sensitive (H69/P) and resistant (LX4) cell lines respectively. Note there is very much faster 400 nm
120
80
40
20
40 60 Time (minutes)
0
600 nm
r Y 20
40 60 Time (minutes)
Figure 15.12. Time courses for the development of violet (400 nm) and red (600 nm) fluorescence in the H69/P and LX4 cells lins. The closed and open symbols represent the results from the parent (H69/P) and resistant (LX4) cell lines respectively. The error bars were drawn at the 95% confidence limits.
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1-2r O O
0.8
o (0
o 0.4 o
2o LL
0
20 40 Time (minutes)
60
Figure 15.13. Red: violetfluorescenceratios calculated from the data in figure 15.12 where the closed and open symbols again represent the sensitive (H69/P) and resistant (LX4) cells. The lower ratio in LX4 is a manifestation of the violet bias, and hence lower dye: DNA-phosphate ratio, in these cells. development of fluorescence in the parent and a considerable violet (400 nm) bias in LX4 compared with its red {600 nm) fluorescence. The instrument was set up with the parent cell line as the control and any differences in total fluorescence intensity arising from differences in cellular DNA content can be 'normalized' by taking the red: violet ratio. This is shown in figure 15.13 with the closed and open circles again representing the sensitive (H69/P) and resistant (LX4) cells. The lower ratio in the latter clearly demonstrates the considerable violet bias to the emission. Figure 15.14 shows a time course for the development of fluorescence at three wavelengths (600 nm, circles; 500 nm, triangles; and 400 nm, squares) for H69/P and LX4 in left and right panels respectively where verapamil was added to both after 25 minutes exposure to Hoechst 33342. The solid symbols represent the results following verapamil treatment. There was no difference in the sensitive cell line (left panel) but there was a pronounced change in the LX4 multi-drug-resistant cell line (right panel) with considerable increase in fluorescence at all wavelengths. The red: violet ratios calculated from the data of figure 15.14 are shown in figure 15.15 where the red shift after verapamil addition in the LX4 cells (triangles) is very apparent; however, there was no change in the sensitive parent (circles). This technique for assessing gp 170 MDR depends on only two basic factors, namely the violet bias to the fluorescence emission from the DNA/Hoechst 33342 complex at low dye: DNA-phosphate ratios and the postulate that the dye is pumped out of cells by gp 170 . Cells with increased numbers of gp 170 molecules in the membrane should, therefore, maintain a lower intracellular Hoechst 33342
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LX4
H69
Verapamil 140
Verapamil 140
100
20
40 60 Time (minutes)
20
40 60 Time (minutes)
Figure 15.14. The time course for the development of fluorescence at three wavelengths (600 nm, circles; 500 nm, triangles; and 400 nm, squares) for H69/P and LX4 in the left and right panels respectively. Verapamil was added after 25 minutes exposure to Hoechst 33342. The solid symbols represent the results following verapamil exposure.
c
o o §0.8
c 0.4 0) o 0
20 40 Time (minutes)
60
Figure 15.15. Red: violet ratios from the data in figure 15.14. The red shift after verapamil addition in the LX4 cells (triangles), due to an increase in the dye: DNA-phosphate ratio, is very apparent; however, there was no change in the sensitive parent (circles).
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concentration for a given extracellular concentration. Consequently, the fluorescence emission will be violet biassed compared with cells containing lower numbers of membrane gp 170 molecules. Verapamil, which blocks calcium channels and reduces the activity of gp 170 , will decrease the efflux of dye in cells with elevated gp 170 levels. This results in a higher intracellular dye concentration, greater binding to DNA and a relative red shift to the emission spectrum. Cells with very low numbers of gp 170 molecules will show little or no emission spectrum shift with verapamil. We have not shown directly that Hoechst 33342 is actively transported out of cells by the gp 170 pathway, but the evidence pointing to this conclusion is compelling. Firstly, the cellular uptake of Hoechst 33342 parallels that of cytotoxic agents involved in MDR (Lalande, Ling and Miller, 1981). Secondly, the intracellular content of this agent is modified by verapamil (Krishan, 1987, and see above). Thirdly, the predicted red shift in the emission spectrum due to verapamil only occurs in gp 170 elevated MDR cells. Finally, of three MDR cell lines investigated, the phenomenon was only seen in LX4 cells in which the mdr-1 gene was found to be amplified (Reeve et al, 1989). It was not found in MDR cells without mdr-1 gene amplification. The technique has been applied in a very limited number of patients with smallcell lung cancer to date, but this has already demonstrated the feasability of the approach. The illustrating example from a small sample of a biopsy specimen was disaggregated with trypsin/versene, stained and assayed both with and without verapamil. In each of the panels in figure 15.16 violet fluorescence (400RF AREA) is plotted on the X-axis obliquely from left to right with red fluorescence (600RF AREA) on the Z-axis from right to left. The origins are furthest from the eye with frequency on the Y-axis in these three-dimensional data spaces. The top two panels show the results obtained from a disaggregated small-cell lung cancer biopsy at 2 and 5 minutes after staining with Hoechst 33342 (left and right respectively) where a number of subsets can be seen and there was a considerable violet bias to the emission of the major population at these short incubation times. The bottom left panel shows the results obtained within the same experiment from the verapamil pre-treated drug-sensitive cell line H69/P analysed 2 minutes after staining which was identical to the non-verapamil treated sample as was expected from the data in figure 15.15. This panel represents a reference standard where cells in the other three panels which are angled further to the right than the data in this panel are classified as violet biassed. The bottom right panel shows the results from the biopsy after 5 minutes staining where the cells were pretreated with verapamil. Note the better defined peaks compared with the non-verapamil treated cells (top right panel) where the major spike (checked with ethidium bromide staining) represents aneuploid tumour cells. There has been both an increase in total fluorescence and a relative shift towards the red (600RF AREA) fluorescence axis. The degree of shift in the aneuploid component is comparable to that shown in figure 15.15 and indicated the possibility of MDR.
BIOPSY z
mn%
8I0PSV 5
u
z
BIOPSY
L• Figure 15.16. Small-cell lung cancer patient biopsy assayed on the violet (400RF AREA) and red (600RF AREA) channels at short times after staining with Hoechst 33342. The origins are furthest from the eye with violet fluorescence scored from top left to bottom right and red fluorescence scored from top right to bottom left. Results from verapamil treated H69 cells at 2 minutes after staining, which act as a reference standard, are shown in the bottom left panel. The two top panels show the biopsy results at 2 and 5 minutes respectively after staining with Hoechst 33342. In both panels the major population is angled to the right compared with the H69 data indicating a violet bias. The data in the bottom right panel were obtained from biopsy cells pretreated with verapamil and stained for 5 minutes. These show a dramatic shift in the major spike compared with the top right panel. The latter has increased in fluorescence intensity on both the red and violet channels but the former is relatively greater than the latter indicating a red shift due to verapamil.
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The 'direct' method of Herweijer et al (1989) is very similar except that they used daunorubicin as the reporter probe for MDR with verapamil and cyclosporin-A as the efflux modifiers in sensitive and resistant human ovarian cancer cell lines. The resistant line, A2780/R, was maintained continuously in medium containing daunorubicin at a concentration of 2 uM but the cells were incubated in drug-free medium for 48 hours prior to analysis. Time courses for the uptake of daunorubicin were then performed for the sensitive (A2780/S) and resistant lines and the efflux modifiers were added to the resistant cells after 30 minutes. The results with verapamil are shown in figure 15.17 where three different concentrations of the efflux modifier were used. It is clearly apparent that there was a verapamil concentration dependent increase in daunorubicin fluorescence in the resistant cells. Hepes-buffered Hanks' salt solution was added to the sensitive cells at 60 minutes to act as a control. These results, I'm sure, represent the processes being observed in the biology as they exhibit the same effect as seen in figure 15.15. This, of course, assumes that we were correct (Morgan et al, 1989) as the control in figure 15.17 from Herweijer et al (1989) is not adequate. Verapamil should have been added to both cell types at 30 minutes to exclude the possibility of similar changes in the sensitive cells. Comparable results using cyclosporin-A as the efflux modifier are shown in figure 15.18. Again varying doses of cyclosporin-A were added at 30 minutes, and on a molar basis this agent was considerably more efficient in modifying efflux than verapamil, compare with figure 15.17. However, again I would challenge the control as no cyclosporin-A was administered to the sensitive cells at 30 minutes.
4500n
A2780/S O C 4) O 0)
30
60 Time (minutes)
90
Figure 15.17. Daunorubicin time course uptake in sensitive (A2780/S) and resistant (A2780/R) cell lines. Verapamil increased the uptake of daunorubicin in the resistant cell line.
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4500n
A2780/S 0)
o
0(iM
30
60 Time (minutes)
90
Figure 15.18. Similar experiment to that in figure 15.17 where cyclosporin was used as the daunorubicin efflux modifier. Both this and the previous figure were redrawn from Herweijer et al. (1989).
A non-kinetic method for improving the detection of MDR in daunorubicintreated cells has been proposed by Ross et al. (1989). This involves measuring daunorubicin fluorescence and cell volume, which enable intracellular concentration to be calculated which is lower in MDR cells. Antibodies are available to both the internal and external domains of gp 170 and these can be used to estimate the number of molecules per cell. An example obtained with H69 and LX4 is shown in figure 15.19 where there is greater fluorescence associated with the resistant LX4 cell line. This type of assay may be useful in some circumstances; however, it is measuring total quantity of gp 170 and this may not correlate with its functional activity which is the important parameter to quantitate in any attempt to assay for MDR. Nevertheless, combinations of these types of techniques can, and have, been applied directly to patient biopsies (Morgan et al, 1987, 1989; Watson, Morgan and Smith, 1989) and with further refinements they should be able to detect a 1:1000 drug-resistant minority subset within the sample. This may be very useful as it could tell us if we need to administer efflux modifiers in combination with drugs which are known to either induce or select for multi-drug resistance. A further avenue for exploitation is in the general area of drug transport into cells. It was shown in section 14.2.7 that esterase inhibition by carbamoylation with nitrosoureas and related isocyanates can be assayed flow cytometrically and comparisons between agents can be made using the I50 value which is the dose required to induce 50% inhibition of activity. An example of BCNU inhibition was given in that section and similar assays were performed with a number of drugs using both flow cytometry for intact cells and conventional spectrofluorimetry
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Figure 15.19. Two cell lines, H69 parent (middle panel) and MDR LX4 (bottom panel) stained for DNA (630RF AREA, top left to bottom right) simultaneously with immunofluorescence for gp 170 (520RF AREA, bottom left to top right). The top panel is the fluorescence control data set. A few H69 cells exhibit some gp 170 fluorescence but the LX4 cells which have MDR-1 gene amplification show considerable fluorescence.
3S0
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Table 15.1. Iso values (M) Drug CHI CCNU BCNU CEI TCNU ACNU CHLOZ GANU
Intact cells
Sonicates
Ratio
1.1 x 10"' 3.8x10"' 5.0x10"' 1.0 x 10"' 1.8 xlO" 4 7.3 x l O " 3 >1.5xlO"2 > 1.5 xlO" 2
2.6x10"' 8.3x10"' 9.2x10"' 1.6x10"' 9.9x10"' 3.2 x l O " 3 2.4 x l O " 3 2.4 x l O " 3
0.423 0.458 0.543 0.625 1.818 2.281 > 6.250 > 6.250
with sonicated preparations and the I50 values for the two methods are compared in table 15.1 together with the ratio of results from intact cells to those in sonicates. The results in this table are interesting. The I 50 ratios for CHI, CCNU, BCNU and CEI indicate that only about half the concentration of drug is required to obtain 50% esterase activity inhibition in whole cells compared with sonicates. With TCNU and ACNU this is reversed with double the drug concentration required in whole cells compared with sonicates; however, with chlorozotozin and GANU this has increased to greater than six-fold. These results almost exactly parallel the hydrophilicity of the agents. CHI, CCNU, BCNU and CEI are lipophilic, but chlorozotozin and GANU are hydrophilic, readily soluble in water at physiological pH and temperature and would not be expected to cross the external cell membrane without an active transport mechanism. We have seen earlier that nitrosoureas enter cells by passive diffusion, thus we would not expect chlorozotozin and GANU to enter cells. This conclusion would seem to be substantiated by the data in table 15.1 and the method seems capable of assessing not only the ability of such agents to cross the external cell membrane, but also their capabilty of inducing damage having entered the cell. This technique, like those described above for MDR, could also readily be applied to small biopsies taken directly from a tumour. 15.3.3 Tumour growth rate Surgery and radiotherapy were the mainstays of cancer therapy until the late 1950s when chemotherapy was introduced. A number of landmarks can be identified in radiotherapy, the first of which was that it was ever used at all for cancer therapy, and the second was that it was used so soon after the discovery of radium (Curie and Curie, 1899). It is also worth remarking that hormone manipulation for breast cancer by oophorectomy was introduced three years earlier by Beatson (1896). The next major 'contribution' to radiotherapy was the introduction of external beam fractionated radiation in which multiple small doses were delivered on a daily basis over a number of weeks. In fact, this was entirely serendipitous. The early X-ray machines had a very low radiation output and
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frequently overheated and had to be switched off intermittently or they broke down completely. Thus, it was logistically easier for staff and patients to treat a number of patients each for a short time and let the machines cool off between treatments rather than have one patient there all day and wait between treatments. However, it was not until the late 1950s and early 1960s that it was shown why this approach can actually work. A further landmark was the introduction of high energy radiation (super-voltage) in the 1950s where the maximum absorbed dose occurs at some depth into the tissues thus sparing the skin from damage. The recognition that cells are relatively more resistant to radiation under anaerobic conditions (Crabtree and Cremer, 1933; Mottram, 1935) and that tumours contain hypoxic cells which are resistant to radiation at critical distances from blood vessels was another important step (Thomlinson and Gray, 1955). This lead to radiation treatment in hyperbaric oxygen (van den Brenk, Madigan and Kerr, 1968) and the introduction of electron-afBnic chemical sensitizing agents (Adams and Cooke, 1969). One of the greatest problems with all non-surgical cancer treatments is the complete non-specificity and all tumours of a given type tend to be treated identically and in radiotherapy this involves irradiation on a three or five fraction per week schedule with no therapy at the weekend. Unfortunately, tumours don't know that they should stop growing at the weekend when nobody is around to treat them and the same applies to chemotherapy schedules with extended intervals (2-4 weeks) between courses. The net rate constant for growth of a tumour (K) is dependent on the excess of the rate constant for cell production (KP) compared with the rate constant for cell loss (KL) where K= KP — KL. If a tumour has a very high rate of cell production which is only partially arrested by each week of fractionated radiotherapy or by each course of chemotherapy there is a distinct possibility that it could grow back to its original size or beyond during the treatment intervals. However, some breaks in treatment are necessary to allow the normal tissues to recover as these too are damaged by the therapy. A fractionated course of cancer therapy, which could be either radio- or chemotherapy, is depicted in figure 15.20. This may look a little complicated at first sight but it's really very simple and a considerable underestimate of the complexity of the reality. Five therapy fractions are depicted by the arrows. Just before fraction 1 both the tumour and the treatment target volume containing the tumour have an initial 'surviving fraction' of unity. If chemotherapy is being used the target volume is the whole patient. For the sake of simplicity we will assume that the dose given at each fraction kills 50% of the tumour cells. It is highly probable that this same dose will kill relatively more of the critical normal cells within the treatment volume and, again for simplicity, I've chosen this as 60%. Thus, after the first fraction the tumour will be reduced to 50% of its initial cell content (solid triangle) and the normal cell component will be reduced to 40% (solid circle) and at this point we have killed relatively more of the patient than the tumour. What happens next is critical to understanding why fractionated therapy works. Normal tissues have the capacity to recover rapidly by repairing damage at the cellular level, regenerating within the target volume and by repopulating from without the
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Jo.50,4
Time—• Figure 15.20. Representation of the response of a tumour to fractionated therapy. target volume if the latter is localized (i.e. radiotherapy). This is depicted by the dotted line from the solid circle at 0.4 at fraction 1 to the open circle at 1.0 at fraction 2. The normal tissues will not recover to above 1.0 due to the normal homeostatic mechanisms. The tumour does not recover so rapidly but it does regrow, from the solid triangle at 0.5 at fraction 1 to the open triangle at 0.6 at fraction 2. When the second therapy fraction is delivered the normal cells are again reduced to a surviving fraction of 0.4 (solid circle at fraction 2) and the tumour is reduced to 0.5 of 0.6, i.e. 0.3 (solid triangle at fraction 2). This is the point at which the first net gain is achieved. The normal tissues again recover to 1.0 (dotted line) and the tumour again regrows. Although the proportional increase in the latter is the same as previously (exponential growth) the absolute increase is less than between fractions 1 and 2 and it regrows to less than 0.4, the open triangle at fraction 3. This process continues with increasing numbers of therapy fractions and the tumour volume declines exponentially as shown by the dot-dash-dot curve as long as the fractions are spaced as shown. However, if fractions 2,3 and 4 had been omitted the tumour would have regrown, represented by the dashed curve, to its original size (solid square) just before fraction 5 (which would now be fraction 2) and such a spacing of therapy fractions could not hope to contain tumour growth. Thus, the optimum interval between treatment fractions is critical and primarily dependent on the rate of tumour growth which, in turn, is dependent on the rate of cell production by the tumour. There was no realistic means of assessing tumour cell production rate until Begg et al. (1985) produced a very elegant method which I would place along side, or
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383
even above, the oxygen effect and sensitizers in terms of potential importance to radiotherapy. That importance lies in the simple fact that for the very first time we are able to measure something in a tumour which has direct relevance to the speed at which the tumour is growing and prescribe treatment specifically for that tumour. Because of its potential importance I'll describe it in some detail though the reader should be encouraged to read the original paper (Begg et al, 1985) and the follow-up correspondence (White and Meistrich, 1986). The potential doubling time, T pot, of a tumour is given by the expression,
where t$ and LI are the duration of S-phase and labelling index respectively and where 1 is a correction factor for the position of S-phase in the cell cycle of exponentially growing populations (Steel, 1968). The value for k is always likely to be between 0.9 and 1.0 in human tumours although it could have a wider range for cells growing in tissue culture, hence, to a reasonable approximation, a value for the potential doubling time, T pot, can be obtained by knowing the S-phase duration and labelling index (proportion in S-phase). The importance of T pot is shown by the relationship, KP = log e 2/T pot where KP is the rate constant for cell production. Hence, by measuring the S-phase duration and LI simultaneously we can obtain the rate constant for cell production in a tumour. Begg et al. (1985) solved this problem by suggesting that a single dose of bromodeoxyuridine should be administered to patients, then at a defined interval later (about 4 hours) a single biopsy should be taken from the tumour. Part of this would be used for the normal histological diagnosis and part for disaggregation and double staining for total DNA (propidium iodide) and BrdU (fluorescein) for flow cytometric analysis as described in section 11.5.5. We have already seen in figure 12.10 that such data sets can be gated to obtain the proportion of cells which have taken up BrdU (the labelling index). Moreover, we can also determine the proportion of cells initially labelled with BrdU which have halved their BrdU content at mitosis and have divided to appear in Gl at an interval after BrdU was administered. Let us suppose for simplicity that 50% of cells have halved their BrdU content and entered Gl 4 hours after administration. It's not too difficult to appreciate that the remaining 50% will also take about 4 hours to halve their BrdU content and enter Gl giving a total S-phase duration of about 8 hours. Similarly, if after 4 hours only 25% of labelled cells have halved their BrdU content and entered Gl then there will be three more cohorts of 25% of the total each of which will require about 4 hours to complete DNA synthesis. Thus, to a first approximation the S-phase duration will be about 16 hours. In principle it really is as simple and as elegant as that and as a radiotherapy and flow cytometry person I wish I'd thought of it and I bet many other people do too! This technique is now being used in clinical trials at Mount Vernon Hospital, Northwood, to assign patients with high rate constants for cell production, KP
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APPLICATIONS IN ONCOLOGY
calculated from Tpot/ to hyper-fractionated radiotherapy schedules (multiple fractions per day) and those with low values of KP to conventional single daily fraction schedules. The difference between this clinical trial and all the others is that the two arms of the study are designed around a highly relevant biological parameter, the cell production rate, which is actually being measured within the tumour and flow cytometry is the only means of doing this.
15.4
Future prospects
It is always foolhardy to attempt to predict the future, except perhaps in nuclear physics where some spectactular predictions were later found to be true, and I'm not going to fall into this trap in oncology. However, at the beginning of this chapter I asked a number of questions and was somewhat scathing (I hope) about some of the basic premises on which anti-cancer clinical trials have been carried out. There is never any justification for destructive negative criticism about anything and if we are to be critical we should only be so in a constructive and positive sense. It is clear from the examples in the chapter that flow cytometry could help us in these matters. A number of assays are now available which give prognostic information (DNA index, S-phase fraction, oncoprotein quantitation) but, as I have pointed out, this really doesn't help us very much in the design of therapy strategies. However, help is also at hand here and, in an ideal world, every patient who is about to undergo either attempted curative or diagnostic surgery for cancer should have a prior injection of BrdU so that an estimate of the rate constant for cell production can be obtained. This might enable us to develop fractionated therapy regimes for chemotherapy similar to those studies now being carried out at Mount Vernon Hospital for radiation which are designed for a particular tumour. Furthermore, whenever therapy with radiation and drugs is to be contemplated the cells from the tumour biopsy should be assayed for GSH levels, methotrexate uptake and MDR using both functional assays described. This would be particularly important for breast cancer where many adjunctive chemotherapy regimes using adriamycin and methotrexate are frequently employed. By carrying out prior biochemical assays on the tumour cells under near-physiological conditions we should be able to predict if there is likely to be a subpopulation of cells which is drug or radiation resistant and employ suitable modifying agents where necessary. It goes without saying that all of these suggestions should be carried out under carefully controlled clinical trials where the basic premises of those trials are based on sound biochemical measurements to stratify patients into subgroups which need special attention as opposed to the overall empiricism applied to all patients with a particular tumour type which is the general rule at present.
16 Epilogue
If you have read the whole of this book I salute you. If you are not primarily involved in this field, have read the whole book and have understood everything, then I salute both of us. The intention was an introduction and, indeed, that is all that it is as, on the applications front, I have omitted very considerably more than IVe included. The problem with writing about flow cytometry is that it covers the whole of biological science and it is not possible to include everything, thus a considerable degree of selection must be employed. However, I hope that the first 10 chapters, which were intended to show how these instruments work, how they can be used and some of the associated problems, were not only intelligible but also prove to be useful. The last five chapters were intended to show where they can be used in a number of fields in cell biology including oncology. However, the biggest applications omission is the whole of immunology which, if it had been included, would have more than doubled the size of the book. The technology is also being used increasingly in microbiology, plant biology and in the aquatic sciences and none of these have even been mentioned up till now. The last of these is assuming increasing importance and in recognition of this the September 1989 issue of Cytometry, containing 21 papers and over 600 references, was devoted to this topic. There has been a simply phenomenal revolution in the biological sciences over the past 40 years which, I believe, represents a Renaissance equivalent to those in art and literature in the fifteenth and sixteenth centuries, mathematics, physics and chemistry in the sixteenth and seventeenth centuries and physics and astronomy in each of the decades either side of the turn of this century. Chemistry and physics respectively did not really begin until the chemical balance and measurement systems (length and time) were invented. Biology is considerably more complex than chemistry and physics as it includes both of these disciplines. The current revolution in biology is due, in part, to our capacity to recognize and measure cellular and subcellular constituents and to relate these to function of both individual cells and complex interactions between cells in multi-cellular cooperative organ systems. The methods by which those measurements are made is the means by which the revolution has taken place and flow cytometry has been part of that revolution for the past 20 years. It would seem to me that these instruments together with those of image analysis coupled with techniques in biochemistry and
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molecular biology have given us an unprecedented capacity to quantitate in all aspects of cell biology. We are no longer inhibited in our capacity to measure in the biological sciences and for those who have the courage to use their imagination there would seem to be no limit to what can be achieved. That is the only real message I would like this book to convey.
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Index
aberrations, 20-1, 23-7, 29 astigmatic, 29 chromatic, 20-1, 25-7 spherical, 23-4 absorption, 34-6, 49, 51, 160-5, 168, 175, 185 filters, 34-6, 51, 160-5, 168, 175 fluorochromes to plastic tubes, 185 spectra, 49 accuracy, see precision acetoxy-methyl esters, 133, 146-7 acid denaturation of DNA, 135-6 acridine orange, 50, 185, 204-7, 243, 247-56, 283-5, 350 BrdU quenching, 250 cell cycle subsets, 250-6 metachromatic fluorescence, 50, 204-7 multi-parameter analysis with, 283—5 precipitation with, 206 screening with, 350 staining with, 50, 206, 247-51 structure of, 205 actinomycin-D, 251, 276, 370 ADC, see analogue-to-digital conversion adjunctive chemotherapy, 384 age distribution theory, 211—13 agglutinating fixatives, 122-3 air line filtration, 155 Airy disk, 33 alkaline phosphatase, 324 allophycocyanin, 50 amino-methyl coumarin acetic acid (AMCA), 50, 125, 128, 282-3 amplification, 68-70, 129-31, 154, 159-60, 169, 171-2, 241 electronic, 66-70, 154, 159-60, 171-2 differential, 68-70 linear, 66, 171-2 logarithmic, 66-7, 154, 159-60, 171-2 fluorochrome, 129-33, 169, 241 biotin: streptavidin, 130-1, 169, 241 liposomes, 130-1, 169 polyclonal antibodies, 129
analogue-to-digital conversion, 72—3, 76, 17 A, 176
offset, 72, 173, 176 resolution of, 72 analysis of data, see data analysis aneuploidy, see DNA, index angle of incidence, 18-19, 26-31 antibodies, 125-33, 237-8, 269-73, 282-3 bromodeoxyuridine, 23 7-8 combination staining, 127-9, 282-3 labels for, 125 monoclonal, 128 polyclonal, 129 staining with, 126-33, 269-73 structure of, 127-9 fragments, 128 heavy chains, 127 light chains, 127 recognition site, 127 variable regions, 127 synthetic peptide induced, 128, 132, 271, 282-3 anomalous diffraction, 62 antigens, 123, 131-2, 247, 268-87, 297-8, 358-6, 364 cell surface, 123, 285 cytoplasmic, 131-2, 283-7 nuclear antigens, 132, 247, 268-83, 297-8, 358-6, 364 histones, 247, 268-9 interchromatin granules, 269 Ki-67, 269 p53, 269, 358 p55c~fos, 269-70, 282, 283 p62c~myc, 269-82, 358-6 p62c~myc, staining, 270-1 problems, 132 staining and quantitation, 269—3 topoisomerases, 269, 274, 297-8 turnover measurements, 273, 364 AO, see acridine orange aperture, numerical, 40 applications in oncology, 345-84
432
INDEX
applications in oncology (cont.) adjunctive chemotherapy, 384 bladder cancer, 350, 355 breast cancer, 351-2, 384 Brenner tumour, 352 bromodeoxyuridine, 356, 383 Burkitt's lymphoma, 354 cancer diagnosis, 348—51 carbamoylation, 379 cell loss, 381 cell production rate, 381-2 cervical cancer, 362 chlorambucil, 369 chloroethylnitrosoureas, 369, 380 CIN, 362 clinical trials, 347 colonic adenomata, 353, 357, 362 colorectal cancer, 351, 353, 361 cyclosporin-A, 377 cytological prescreening, 349-51 acridine orange, 350 bladder, 350 gynaecological, 350—1 nuclear-to-cytoplasmic ratio, 350 slit-scanning, 350 cytoskeleton, 358 daunorubicin, 377 diagnosis, 348-51 leukocyte classification, 349 drug resistance, 340-2, 368-80, 384 active efflux, 370 adriamycin resistance, 370 cross resistance, 369 drug resistance pathways, 370 glutathione, 325-8, 367-8, 384 gp 170 , 370-1, 373, 375, 379 Hoechst 33342, 371, 373 MDR-1 gene, 369, 371 mechanisms, 368-9 multi-drug resistance, 369-78, 384 DNA index, 242-4, 351-6 efflux modifiers, 377 electron affinic sensitisers, 381 ENT tumours, 354 esterase inhibition, 378 fractionated radiotherapy, 380-1 future prospects in oncology, 384 glutathione, 325-8, 367-8, 384 hereditary tumours, 357 HER2/neu, 358-60, 366 homeostatic mechanisms, 382 hyperbaric oxygen, 381 hyperfractionation, 384 hypoxic cells, 381 leukaemia, 367 lung cancer, 354 malignant melanoma, 355, 357
medulloblastoma, 355 methotrexate, 384 monochlorobimane, 325, 367 multi-variate analysis, 355 neuroblastoma, 355 nitrogen mustard, 369 non-Hodgkin's lymphoma, 351, 354 oncogenes, 356-66 oophorectomy, 380 ovarian borderline malignancy, 352 ovarian cancer, 352, 363 phenylalanine mustard, 369 potential doubling time, 383 prognosis, 351-66 archival biopsies, 351 DNA index, 351-6 oncogenes, 356-66 p21c~ras, 358 p53, 358 p62c~myc, 358-66 p62c~myc turnover, 364 receptor status, 366 renal adenocarcinoma, 355 retinoblastoma suppressor gene, 358 retro viruses, 356 reverse transcriptase, 356 S-phase fraction, 352, 354-5 Testicular cancer, 360-1 therapy selection, 366-84 tumour growth rate, 356, 380—4 tumour suppressor genes, 357 verapamil, 372, 375, 377 archival biopsies, 120-2, 132, 351-6,
358-66 dewaxing 121 digestion, 121 nuclear extraction, 121—2 problems, 132 arc lamps, deuterium, mercury and xenon, 56 argon lasers, 57, 148 arrays, see data arrays astigmatism, 29 AT specific dyes, 50, 51-2, 133, 148-9, 185, 201-2, 256-66 AT:GC composition, 293 autofluorescence, 152, 158 back flushing, 185 background compensation, 100—1 background current, 155 background fluorescence, 151-2 background subtraction, 68-70, 92, 100-1 base-pair composition, 293 band-pass filters, 37, 51, 148, 161, 175, 282-3, 371 base-line DC current, 155
INDEX beam geometry, 58-60 beam splitter, 168 Bernoulli, 5-6 binding site modulation, 134—5, 243—4 biotin, 130-1, 169, 241 bridge, 130-1 streptavidin, 130-1, 169, 241 biotinolated antibodies, 130-1 biotinolated nucleotides, 241 binomial statistics, 14, 113-14 bisbenzimidazoles, 50, 52-1, 133, 148-9, 185, 201-3, 256-66, 292, 371 structure of, 203 bits, bytes and binary, 72-6 bit-mapping, 86-92 2-dimensional, 86 multi-dimensional, 88-92 bivariate (two-dimensional) data, 81, 195-8, 283-5 bladder cancer, 350, 355 bleach, 185 bleaching, 49, 53, 167, 173 blocking bar, 41 bone marrow analysis, 148-9 BrdU, BrdUrd see bromodeoxyuridine breast cancer, 351-2, 384 Brenner tumour, 352 brightness, 55 bromodeoxyuridine, 235-41, 250, 276-82, 293, 356, 383 acridine orange quenching by, 250 antibodies to, 237-8 growth kinetics with, 238-9, 279-82 incorporation, 238-41 quenching with, 235, 250 stoichiometry, 239 tumour growth rate, 239-41, 356, 380-4 boundary layer, 7-8 building vibration, 154 Burkitt's lymphoma, 354 calcium, 50, 133, 147, 336-9 measurement of, 337-8 probes for, 50, 147 calibration, 146-7, 158-9, 176, 244-6, 337-8 biological standards, 244-6 calcium 337-8 chicken, red cells, 244-6 coincidence in, 176 fluorescent microbeads, 159 labelled antibodies, 158-9 pH, 146-7 trout red cells, 244-6 cancer, see application in oncology cancer diagnosis, 348-51 capillary bore, 156
433
carbamoylation, 379 carboxyfluorescein, 131, 146 Casperson, 2 cell cycle, 207-8, 223-41, 250-6, 273-82, 356, 383 after Howard and Pelc, 208 kinetics, 223-41, 273-82 bromodeoxyuridine, 235-41, 250, 279-82, 356, 383 FPI analysis, 233-5 mitotic selection, 225-7 modelling population kinetics, 228-41 PLM curve, 207-8 stathmokinetic analysis, 224-5 modulation, 273-82 subsets, 250-6 cell loss, 381 cell production rate, 381-2 cell separation, 106-16 electrostatic sorting 107-16, see cell sorting iron particles, 106 magnetic beads, 106 sedimentation, 106 cell size, 64, 186-91 cell sorting, 106-16 droplet charging, 107-9 droplet deflection, 108-10 droplet generation, 107 efficiency, 115-16 electrostatic sorting, 107-16 high speed, 303 ink-jet writing, 106 one-droplet sort, 112 pre-sorting enrichment, 114 problems, 116, 134 purity, 110-14 statistics, 112-14 sorting yield, 110-14 three droplet sort, 112 times, 110 centromere, 297, 301 centromeric indices, 139, 301 cervical cancer, 362 chamber design, seeflowchambers chicken red cells, 244-6 chicken thymocytes, 259-62 chlorambucil, 369 chloroethylnitrosoureas, 332-4, 369, 380 chromatic aberration, 20-1, 25-7 chromatin, 268-9 charged couples devices, 66, 140 chromatic compensation focussing, 26-31 chromomycin A3, 50, 201-2, 292-3 structure of, 202 chromosome analysis, 115, 139, 283-5, 288-308
434
INDEX
chromosome analysis {cont.) applications, 303-8 diagnosis, 302-4 genomic libraries, 304-5 gene mapping, 305-8 radiation bio-dosimetry, 308 banding, 302 bivariate karyotype, 295-6 bromodeoxyuridine, 293 centromeric indices, 139, 301 chromosome-associated proteins, 297-8 dual-beam excitation, 283-5, 293 harvesting mitotic cells, 225-7, 288-9 high-speed sorting, 303 karyotype analysis, 299-300 one dimensional (monovariate), 299 two-dimensional (bivariate), 300 in situ hybridization, 299, 305 preparation, 290—1 hexylene glycol, 290 hypotonic PI detergent, 291 magnesium sulphate, 291 Ohnuki buffer, 291 polyamine, 290 slit-scanning, 301 staining, 292-3 base composition, 293 partial sequence specificity, 297 total DNA, 292 univariate karyotype, 115, 295-6 CIN, 362 clinical trials, 347 clumping, 136, 175 coaxial streaming, 6 coefficient of variation, 72, 143-4, 165, 170-1 coincidence, 13-17, 176-9 correction for, 177-9 probability of, 16 use of, 176 coincident focussing, 28-31 colcemid, 224, 283, 289 coordinate coding, 7 7-SO collagenase, 119 colonic adenomata, 353, 357, 362 colorectal cancer, 351, 353, 361 combination staining, 51-3, 128, 266, 282-3 AMCA/FITC/PI, 128, 282-3 antibodies, 282-3 Hoechst/FITC, 266 spectral considerations, 51-3 compensation, 26-31, 68-70, 99-101 chromatic, 26-31 data, 99-101 electronic, 68-70 computing, 72-105
conic section, 23 conjugate distances, 23—4 conjugate foci, 45—6 contamination, 154-5, 185 air lines, 155 fluorochromes in feed tubes, 185 sheath, 154-5 continuous interrupted sampling, 310 continuous time, 182-5, 311-12 contour maps, 81-2, 85, 89-90, 195-8, 284-5 core, 11-14 diameter, 11, 13-14 position, 12 stability, 12 coumarins, 50, 125, 128, 282-3, 330-2 counting within gates, 92-4, 277-81 Crosland-Taylor, 10, 107 crossed cylindrical lenses, 27-31, 153, 179, 186 cuvette flow chamber, 41, 42-3 light collection from, 42-3 cyanin dyes, 51, 146—7 cyclosporin-A, 377 cylindrical lenses, 25 cytological prescreening, 349-51 cytokeratins, 285-6 cytoplasmic antigens, 283-7 cytoplasmic enzymes, 310, 320-8 cytoskeleton, 285-7, 358 dansyl chloride, 50 DAPI, 51, 201-2, 292 dark current, 155 data analysis, 81-2, 85-105, 195-8, 213-23, 283-5 background compensation, 100—1 deconvolution of distributions, 96-8, 213-23 distribution assessment, 94-100 distribution shape analysis, 97-100 gating, 81-2, 85-94, 195-8, 283-5 Gaussian distribution, 97—100 'skewed-normal' distribution, 98, 100 data acquisition see data capture data arrays, 76 one-dimensional, 76 multi-dimensional, 76 two-dimensional, 76 data capture, 73, 178 buffering, 73 dedicated memory, 73 FIFO, 73, 178 list-mode, 73 data display, 80-90, 94, 195-8, 283-5 contour maps, 81-2, 85, 89-90, 195-8, 283-5
INDEX dot-plots, 81 hidden surface elimination, 83-4 multi-parameter, 85-6 one-dimensional, 81, 94 stereo-perspective graphics, 84 three-dimensional, 84 two-dimensional, 81, 195-8, 283-5 data processing, 76-92, 96-8, 102-5, 195-8, 283-5 arrays, 76 bit-mapping, 86-92 bit-shifting, 79, 102-5 coordinate coding, 77-9, 88 decoding coded data, 79 distribution deconvolution, 96-7 integer arithmetic, 75-6 multi-parameter, 76-80, 85-92, 195-8, 283-5 ranking coded data, 79 daunorubicin 377 denaturation, 122-3, 135-6, 249-50 DNA, 135-6, 249-50 acid, 135-6 heat, 249-50 proteins, 122-3 agglutinating fixatives, 122-3 cross-linking fixatives, 122—3 dedicated memory, 73 detection limit, 169-70 detectors see photodetectors de waxing, 121 dichroic mirrors, 37-9, 168 dichroic combinations, 38-9 serial, 38 serial/parallel, 39 dicyanodihydroxybenzene (DCDHB), 50, 146-7 dielectric interface, 18 differential amplifiers, 68-70 diffraction, 31-4, 62 diphenyl hexatriene, 125, 133 DIPI, 50, 201, 293 dirty optics, 156 disaggregation, 117-21 enzymatic, 118-22 cleavage sites, 118-20 collagenase, 119 elastase, 119 factors influencing, 118 glycosaminoglycans, 118 hyaluronidase, 119 lysosyme, 119 pepsin, 118 pronase, 120 protease, 120 trypsin, 118 mechanical, 117
435
chopping, 117 syringing, 117—18 wax embedded material, 120-1 disc of least confusion, 24 discrimination between populations, 170-2 distribution assessment, 94-100 mean, 94 median, 95 mode, 95 shape, 97-100 distribution deconvolution, 96—8 discrimination, 96-7, 144-5, 171-2 between distributions, 144-5 labelled and unlabelled, 96-8 rare events, 144—5 with log amplifiers, 171—2 double sheath, 12 double threshold, 177-9 DNA, 50-3, 68-9, 134-6, 148-9, 160, 201-65, 276-82, 293, 352-6, 371, 373, 375, 380-4 binding site modulation, 134—5, 243—4 bromodeoxyuridine, 235-41, 250, 276-82, 293, 356, 383 antibodies to, 237-8 growth kinetics with, 238-9, 279-82, 356, 380-4 incorporation, 238—41 stoichiometry, 239, 243 tumour growth rate, 239-41, 356, 380-4 denaturation, 135-7, 239 acid, 135-6 heat, 135, 249-50 chromosomes, see chromosome analysis dyes, see nucleic acid stains emission spectrum analysis, 148-9, 259-65, 371, 373, 375 histogram, 76, 159, 208-11 histogram analysis, 211-13 age distribution theory, 211-13 rectilinear integration, 213 multiple Gaussian, 214-15 polynomial, 215-16 single Gaussian, 216-23 TCW analysis, 223 index, 241-4, 351-6 stains, see nucleic acid stains standards, 244—6 stoichiometry, 243 drug resistance, 340-2, 368-80, 384 drug transport, 339-43 adriamycin, 340-1 CNUs, 332-3 methotrexate, 342—3 dual-beam focussing, 26—31 dyes, see fluorochromes
436
INDEX
dynamic cellular events, 309-44 alkaline phosphatase, 324 calcium, 336-9 continuous interrupted sampling, 310 continuous time, 311—12 cytoplasmic enzymes, 310, 320-8 discontinuous sequential sampling, 310 drug transport, 339-43 adriamycin, 340-1 CNUs, 332-3 methotrexate, 342-3 dual substrate analysis, 330—2 esterases, 310, 312-17, 320-4 enzyme kinetics, 317, 335 esterase inhibition, 322-33 fluorescence quantitation, 320-1 p-galatosidase, 328 P-glucuronidase, 322, 325 y-glutamyl transpeptidase, 324, 328 glutathione, 325-8f 367-8, 384 glutathione S-transferase, 326 incorporation of time, 310-17 inhibition kinetics, 332-3 leucine amino-peptidase, 322 light absorption quantitation, 319 membrane enzymes, 328-30 membrane potential, 336-7 Michaelis-Menten hyperbola, 322 mitochondrial function, 339 peroxidases, 320—1 progress curves, 323, 327, 329, 333 short time scale kinetics, 312-17, 333-5 substrates, 317-25, 328, 330-2 fluorescein diacetate, 180, 185, 322-4, 330-2 methylumbelliferyl acetate, 330-2 monochlorobimane, 50, 325, 367 3-o-methyl fluorescein phosphate, 328 verapamil, 341, 372, 375 dynamic range, 66-8, 72-3, 95, 154, 159-65 A-to-D converters, 72-3 log amplifiers, 66-8, 154, 159-60 neutral density filters, 160 variable gain, 160-5 dynode chain, 65
ADC offset, 73, 173, 176 resolution, 72 noise, 151—4 photodetectors, 65-6, 140 photomultipliers, 65 sequential illumination triggering, 71 signal processing, 66-70 solid-state devices, 66 triggering, 70-1, 177 voltage thresholds, 71, 177-9 electron affinic sensitizers, 381 electronic amplification, 66-70, 154, 159-60, 171-2 electrostatic sorting, see cell sorting emission spectrum, 49, 145—9, 259—65 emission spectrum analysis, 145-9, 259-65, 371, 373, 375 pH, 146-7 calcium, 147 DNA, 148-9, 259-65, 371, 373, 375 ENT tumours, 354 enzymatic disaggregation, 118—22 factors influencing, 118 enzyme cleavage sites, 118-20 enzyme progress curves, 323, 327, 329, 333 eosin, 1 esterases, 310, 312-17, 320-4 esterase inhibition, 322-33, 378 ethidium bromide, 50, 175, 203-4, 288, 290, 292 structure of, 204 Euler, 5-6 excitation, 54-60 conventional sources, 56 brightness, 56 deuterium arc, 56 focussing geometry, 54-5 mercury arc, 56 xenon arc, 56 size, 54 lasers, 57-60 beam geometry, 58—60 focussing, 22-31, 58-9 pulse shape, 60 excited state, 134-5
eddy currents, 7 efflux modifiers, 377 elastase, 119 electronics, 65-73, 77, 140, 151-4, 159-60, 171-2, 176-9 amplification, 66-70, 154, 159-60, 171-2 differential, 68-70 linear, 66, 171-3 logarithmic, 66-8, 154, 159-60 analogue-to-digital conversion, 72-3, 76, 17 A
filtration, 34-9, 51, 136, 148, 155, 160-5, 167-8, 175, 267-8, 282-3 optical, 34-9, 51, 148, 160-8, 282-3 absorption, 34-6, 160-5, 168, 175 band-pass, 37, 51, 148, 161, 175, 282-3, 371 dichroic mirrors, 37, 168, 281-3 dichroic combinations, 38—9, 282—3 for AMCA/FITC/PI, 282-3 for Hoechst/FITC, 267-8 long-pass, 34-6, 51, 168, 175
437
INDEX neutral density, 35, 160-5 short-pass, 36, 168 sample, 136 sheath, 155 air lines, 155 filter breakthrough, 51-4 fixation, 122-3 acetone, 122 ethanol, 122 formaldehyde (formalin), 122-3 gluteraldehyde, 122-3 methanol, 122 paraformaldehyde, 122-3 epitope modulation by, 123 flow chambers, 41-7, 107, 372 cuvette, 41 light collection efficiency of, 43, 372 diverging refraction from, 42 modified cuvette, 43-4 spherico-ellipsoidal, 45—7 stream-in-air, 41-3, 107 flow karyotyping, 295-6, 299-300 flow rates, 12-17 calculation of, 12-14 Poisson statistics, 15-17 fluid dynamics, 5—17 Bernoulli, 5 boundary layer, 7 coaxial streaming, 6-10 Crosland-Taylor, 10 Euler, 5-6 flow rates, 12-17 hydrodynamic focussing, 8-12 laminarflow,6—8 pressure profile, 6 Reynolds number, 6 turbulent flow, 7-8 fluorochrome amplification, 129-31, 169, 241 biotin:streptavidin, 130-1, 169, 241 liposomes, 130-1, 169 fluorochrome combinations, 51—3, 57 fluorochromes, 50-3, 123, 125, 128-9, 131, 133, 146-9, 169, 175, 179-80, 185, 191, 196-7, 201-7, 243, 247-66, 269, 282-3, 288, 290-3, 322-5, 328, 330-2, 367, 371, 373 absorbance to tubing, 185 acetoxy-methyl ester derivatives, 133, 146-7 acridine orange, 50, 185, 204-6, 243, 247-56 allophycocyanin, 50 amino-methyl coumarin acetic acid (AMCA), 50, 125, 128, 282-3 bisbenzimidazoles, 50, 51-2, 133, 149-9, 185, 201-3, 256-66, 292, 371
carboxyfluorescein, 132, 146 chromomycin A3, 50, 201-2, 292-3 combinations of, 51 coumarins, 50, 125, 128, 282-3, 330-2 cyanins, 50, 146-7 dansyl chloride, 50 DAPI, 50, 201-2, 292 dicyanodihydroxybenzene (DCDHB), 50, 146-7 diphenyl hexatriene, 125, 133 DIPI, 50, 201, 293 ethidium bromide, 50, 175, 203-4, 288, 290, 292
fluorescein, 50-3, 125, 128-9 fluorescein diacetate, (FDA), 180, 185, 322-4, 330-2 fluorescein isocyanate (FITC), 50, 125, 133, 169 fura-II, 50, 148 Hoechst 33258, 50, 201-3, 292 Hoechst 33342, 50, 52-3, 148-9, 185, 256-66, 371, 373 Indo-1, 50, 147 3-o-methylfluoresceinphosphate (MFP), 338 4-methyl umbellferyl acetate (MUA), 330-2 mithramycin, 50, 191, 201-2 monochlorobimane, 50, 325, 367 naphthol derivatives, 50 olivomycin, 201-2 oxanoles, 50, 205 phenanthridinium, 49-52, 133, 175, 179, 196-7, 203-4, 269, 288, 290-2 phycoerythrin, 50, 125, 129 polyanion, 204-7 propidium iodide, 49-52, 123, 179, 196-7, 203-4, 269, 291-2 pyronine-Y, 50, 205, 256-9 quin-II, 50, 147 resorufin, 50 rhodamine, 50, 125, 169 rhodamine-123, 133 SITS, 50 Texas red, 50 thiazole orange, 50, 207 thioflavine T, 50, 207 tricyclic antibiotics, 50, 201-2 tricyclic heteroaromatic, 204-7 fluorescence, 49-60, 145-9, 169, 259-65, 371, 373, 375
absorption spectra, 49 auto, 152, 158 breakthrough, 51-3 emission spectra, 49 excitation, 54-60 liposomes, 169
438
INDEX
fluorescence (cont.) nature of, 47 quenching of, 49, 54-5, 134-5, 167, 235, 250 resonant energy transfer, 54 spectrum analysis, 145-9, 259-65, 371, 373, 375 fluorescein, 50-3, 125, 128-9 fluorescein diacetate (FDA), 180, 185, 322-4, 330-2 fluorescein isocyanate (FITC), 50, 125, 133, 169 fluorescent microbeads, 159 focussing, 8--12, 22-31, 54, 153, 179, 186 chromatic compensation in, 26-31 conjugate distances, 22-4 crossed cylindrical lenses, 25, 27—31, 153, 179, 187 focal length, 22-4 hydrodynamic, 8-12 multiple beams, 26-31 spherical lens, 22-7, 29-30, 54 single beam, 25-6 forward light scatter, 61-3, 186-91 fractionated radiotherapy, 380-1 fura-II, 50, 147 (3-galatosidase, 32S gating, 81-2, 85-94, 195-8, 283-5 one-dimensional, 94 multi-dimensional, 86-92, 283-5 two-dimensional, 82, 85, 89, 195-8, 283-5 Gaussian, 57-60, 97-100, 143, 170-1, 231 distribution, 97-100, 231 profile, 51-60 statistics, 98-100, 143, 170-1 gene constructs, 276-7 gene mapping, 305-8 gene switching, 255-6 genomic libraries, 304-5 p-glucuronidase, 322, 325 y-glutamyl transpeptidase, 324, 328 glutathione, 325-8, 367-8, 384 glutathione S-transferase, 326 glycosaminoglycans, 118 haematoxylin, 1 helium-neon (HeNe) lasers, 57 helium-cadmium (HeCd) lasers, 57 hereditary tumours, 357 HER2/neu, 358-60, 366 homeostatic mechanisms, 382 Hooke, Robert, 32 high-speed sorting, 303 high-tension voltage, 151, 161-4, 173-5 hidden surface elimination, 83-4
histogram, 60, 76, 81-3, 97-100, 208-23 analysis, 211-13 deconvolution, 97-9, 213-23 DNA 76, 60, 208-11 mono-dimensional, 81 two-dimensional, 82-3 histones, 247, 268-9 Hoechst 33258, 50, 201-2, 292 Hoechst 33342, 50, 51-3, 148-9, 185, 256-66, 371, 373 Huygens principle, 32, 61 hyaluronidase, 119 hydrodynamic focussing, 8-12 double sheath, 12 factors involved in, 9—10 Reynolds number, 6 single sheath, 11 stability of, 11 hydrostatic pressure, 5 hyperbaric oxygen, 239-40, 381 hyperfractionation, 384 hypoxic cells, 381 illumination variation, 58-60 immunofluorescence staining, 50, 126-32 amplification, 129-31 cell surface, 126-7 combination, 127-9 intracellular antigens, 131-2 dyes, 50 incandescent light sources, see arc lamps indo-1, 50, 147 ink-jet writing, 106 information extraction, 3, 76, 80, 92 instrument hygiene, 185 instrument performance, 150-85 integer arithmetic, 75-6 interchromatin granules, 269 intermediate filaments, 285-7 intermitotic phase times, 227 interference, 31-4, 36-7 filters, 36-7 nature of, 32-3 thin films, 33 Young's experiment, 32 interference filters, 33, 36-7, 51, 148, 161, 175, 282-3, 371 construction of, 37 principles of, 33 uses of, 37, 51, 148, 161, 175, 282-3, 371 intracellular antigens, 268-87 cytoplasmic, 283-7 nuclear, 268-83 inverse square law, 54 ionophore, 146-7
INDEX jet-in-air, 41-3, 107 light collection from, 42-3 Ki-67, 269
krypton lasers, 57, 148 laminar flow, 6-8 lasers, 58-60, 148, 156 argon, 57, 148 beam geometry, 58-60 dye, 57 helium-neon (HeNe), 57 helium-cadmium (HeCd), 57 krypton, 57 lasing lines, 57 noise 156 stabilization, 57, 156 current, 156 light, 156 TEM output modes, 58 laws of, 5, 54 conservation of energy, 5 inverse square, 54 motion, 5 lens formula, 22 lenses, 22-31, 54, 153, 179, 186 crossed cylindrical, 27-31, 153, 179, 186 cylindrical, 25 spherical, 22-4, 26-7 thick, 29-30 thin, 23-5, 54 leucine amino-peptidase, 322 leucine zipper, 270 leukaemia, 367 leukocyte classification, 349 light, 18-66, 134-5, 140, 167, 175, 235, 250, 372 absorption, 34, 47-9 bleaching, 49, 53-4, 167 collection, 39-47 collection efficiency, 40-7, 167, 175, 372 colour, 20 detectors, 65-6, 140 diffraction, 31-4, 62 energy transfer, 49, 53-4 filtration, 34-9 flux, 23, 54, 167 fluorescence, 47—54 focussing, 23—31 interference, 31—4 luminescence, 47 phosphorescence, 47 quantum phenomena, 49 quenching, 49, 54-5, 134-5, 167, 235, 250 reflection, 18, 62 refraction, 18-19, 62
439
resonant energy transfer, 54 stabilization, 57 thin films, 33 wave nature of, 32 light flux, 23, 54, 167, 169 light collection, 39-47, 372 cone -|-angle, 40-1 efficiency, 40-7 flow chamber design in, 41—7 cuvette, 41 collection efficiency of, 43, 372 diverging refraction from, 41 modified cuvette, 43-4 spherico-ellipsoidal, 45-7 stream-in-air, 41—3 numerical aperture, 40 light scatter, 18-19, 31-4, 60-4, 141-2, 151-2, 167, 183-200 anomalous diffraction, 62 applications, 183-200 dual-angle scatter, 191-4 forward, 186-91 multi-angle scatter, 198-200 viability determination, 194-8 white cell discrimination, 183 diffraction, 31-4, 62 forward, 61-3, 186-91 Maxwell, 61 Mie scattering, 61 multi-angle, 141-2 Rayleigh scattering, 62-3 reflection, 18, 62 refraction, 18-19, 62 right angle, 64, 151-2, 167, 191-4 sweep scanning, 142 linear amplification, 66, 171-2 linearity, 173-6 A-to-D converters, 173 amplifiers, 173 measurement of, 174-5 photomultipliers, 174—5 liposomes, 131 list-mode data, 73 logarithmic amplification, 66-8, 154, 159-60, 171-2 log-normal distributions, 49, 53, 229 long-pass filters, 51, 168, 175 luminescence, 47 lung cancer, 354 lysosyme, 119 malignant melanoma, 355, 357 mean, 94 measurement range, 66-8, 72-3, 155, 159-65 A-to-D converters, 72-3 log amplifiers, 66-8, 154, 159-60
440
INDEX
measurement range (cont.) neutral density filters, 160 variable gain, 160—5 mechanical disaggregation, 117-18 mechanical vibration, 154 building, 154 laser cooling water, 154 optical mounts, 154 median, 95 medulloblastome, 355 methotrexate, 384 3-o-methyl fluorescein phosphate, 328 4-methyl umbelliferyl acetate (MUA), 330-2 membrane enzymes, 328-30 membrane potential dyes, 50, 133, 146-7 metachromasia, 51, 204—6 Michaelis-Menten hyperbola, 322 microbeads, 159 Micrographia, 33
mithramycin, 50, 191, 201-2 structure of, 202 mitochondrial dyes, 133 mitotic selection, 225-7, 288-9 mode, 95 modified cuvette, 41-4 monochlorobimane, 50, 325, 367 mono-dimensional (univariate) data, 81 multi-angle scatter, 141-2, 198-9 multi-beam focussing, 26—31 multi-detectors, 39, 142, 198 multi-drug resistance, 340-2, 369-78, 384 multi-parameter data and analysis, 76-80, 85-92, 195-8, 283-5 multi-parameter display, 81-6 multi-variate analysis, 355 Muscovy glass, 33 naphthol derivatives, 50 neuroblastoma, 355 neutral density filters, 35, 160-5 Newton, 3, 20-1, 33 nigericin, 146-7 nitrogen mustard, 369 noise, 150-8 biological, 158 dirty optics, 156 electronic, 151-4 fluidic, 154 light sources, 156 mechanical, 154 oscilloscope traces in, 151-2 preparative, 157 stray light, 155-6 non-Hodgkin's lymphoma, 351, 354 non-linear response, 174-6 nuclear antigens, 132, 247, 268-83, 297-8, 358, 364
antibody staining and quantitation, 269-73 histones, 247, 268-9 interchromatin granules, 269 Ki-67, 269 myc constructs, 276-7 p53, 269, 358 p55c~fos, 269-70, 282-3 p62c~myc, 269-82 p62 c-mK staining, 270-1 problems, 132 topoisomerases, 269, 274, 297-8 turnover measurements, 273, 364 nucleic acids and protein, 266—87 non-viable cells, 268-87 viable cells, 266-8 nucleic acid stains, 49-53, 133, 148-9, 175, 179, 185, 196-7, 201-7, 243, 227-66, 269, 283-5, 288, 290-2, 350, 371 DNA specific, 50, 52-3, 133, 148-9, 185, 201-3, 256-66, 292, 371 bisbenzimidazoles, 52-3, 133, 148-9, 185, 201-3, 256-66, 292, 371 phenylindoles, 201-2 tricyclic antibiotic, 50, 201-2 non-specific poly-anion, 50, 185, 204—7, 243, 247-59, 283-5, 350 acridine orange, 50, 185, 204-6, 243, 247-56, 283-5, 350 tricyclic heteroaromatic dyes, 204-7 nucleic acid specific, 49-52, 133, 175, 179, 196-7, 203-4, 269, 288, 290-2 phenanthridinium, 49-52, 133, 175, 179, 196-7, 203-4, 269, 288, 290-2 RNA part-specific', 50, 185, 204-6, 243, 247-59, 283-5, 350 acridine orange, 50, 185, 204-7, 243, 247-56, 283-5, 350 pyronine-Y, 259-60 thioflavine T, 50 nuclear-to-cytoplasmic ratio, 138, 350 numerical aperture, 40 obscruation bar, 43 off-axis aberration, 30 off-scale data, 96 oligonucleotide hybridization, 2, 299, 305 olivomycin, 201-2 oncogenes, 356-66 oophorectomy, 380 opticalfiltration,34-9, 51, 148, 160-5, 168, 175, 282-3 absorption, 34-6, 168, 175 band-pass, 37, 51, 148, 161, 175, 281-3 coloured glass, see absorption dichroic mirrors, 37, 168
INDEX dichroic combinations, 38-9, 282-3 interference, 36 long-pass, see absorption neutral density, 35, 160-5 short-pass, see interference oscilloscope traces, 38 ovarian borderline malignancy, 352 ovarian cancer, 352, 363 oxanoles, 51, 204 p21 c ~ ras , 358 p53, 271, 358 p62c~myc, 358-66 p62c~myc, turnover, 364 paraxial lens formula, 22 pepsin, 120-2, 351 archival material, 120-2, 351 specificity, 118 peroxidases, 320-1 permeabilization, 122-5 detergent, 123-4 fixation, 122—4 freeze—thaw, 124—5 hypotonic lysis, 123 lysolecithin, 125 pH, 133, 146-7 measuremnt of, 146-7 probes for, 146-7 phenanthridinium dyes, 49-52, 133, 175, 179, 196-7, 203-4, 269, 288, 290-2 phenylalanine mustard, 369 phenylindole dyes, 201—2 phosphorescence, 47 photocathode, 65 photodetectors, 65-6, 140 photolysis, 53 photomultiplier noise, 151-3 photomultipliers, 65-6, 151-2, 161-3, 167, 173-5 cathode, 65 high-tension voltage, 65, 151-2, 161-2, 167, 173-5 linearity, 173-5 noise, 151-3 sensitivity, 65 signal-to-noise ratio, 150, 167 spectral response, 65-6 phycoerythrin, 50, 125, 129 PLM curve, 228-31 ploidy, see DNA, index polyanion stains, 204—7 Poisson statistics, 15-17, 110-14, 143, 177 potential doubling time, 383 precision, 13-17, 72, 173-6 ADC offsets, 72, 173, 176 ADC resolution, 72 non-linear response, 174-6
441
coincidence, 13-17, 176 preparation of samples, 117-35, 206, 243-4, 246-59, 269-73, 282-3 enzymatic disaggregation, 118-22 mechanical disaggregation, 117-18 permeabilization, 122-5 staining, 125-35, 206, 243-4, 246-59, 269-73, 282-3 wax embedded material, 120-1 pressure profile, 6 prognosis in cancer, see applications in oncology pronase, 120 propidium iodide, 49-52, 123, 179, 196-7, 203-4, 269, 291-2 structure of, 204 prospects in cancer, see applications in oncology protease, 120 protein A, 131 protein turnover measurement, 273, 364 primary data space, 84—92 Ptolemy, 18-19 pulse shape analysis, 179-80 pyronine-Y, 50, 204, 256-9 quantum phenomena, 49 quality control, 176-85 coincidence correction, 177-9 inspection, 177 pulse shape analysis, 179-80 time, 182-5 quenching, 49, 54, 134-5, 167, 235, 250 quin-II, 50, 147 radio-immuno assay, 158-9 rate-event analysis, 143-5 discrimination in, 144-5 statistics, 143 resorufin, 50 Rayleigh scattering, 62-3 receptor status, 366 reflection, 18, 62 refraction, 18-19, 22-4, 62 converging, 22-4 diverging, 22-4 measurement of, 19-20 refractive index, 18-21 renal adenocarcinoma, 355 resolution, 170-2 resonance cavity, 36—7 resonant energy transfer, 54 retinoblastoma suppressor gene, 358 retro viruses, 356 reverse transcriptase, 356 Reynolds number, 6 rhodamine, 50, 125, 169
442
INDEX
rhodamine-123, 133 ribonuclease, 50 right angle scatter, 151-2, 168, 179 RNA and DNA staining, 246-59 S-phase fraction, 352, 354-5 sample contamination, 116, 154—5 sample filtration, 136 scatter, see light scatter screening, see applications in oncology secondary data space, 84-92 sensitivity, 34-9, 40-7, 166-70, 372 bleaching, 167 excitation intensity, 166 exposure time, 166 fluorochrome amplification, 169 light collection efficiency, 40-7, 167, 372 measurement of, 160-70 optical filtration, 34-9, 167-9 sequential illumination, 30 sequential illumination triggering, 71-2 sheath contamination, 154-5 sheath filtration, 155 short-pass filter, 36, 168 'skewed-normal' distribution, 98, 100 side scatter, see right angle scatter signal processing, 66-71 signal-to-noise ratio, 150, 166, 336 SITS, 50 slit-scanning, 137-41, 291, 301, 350 chromosome analysis, 138-9, 291, 301 cytological prescreening, 137—8, 350 image plane, 140—1 object plane, 137-40 Snell's Law, 18 solid-state devices, 66, 107, 140, 142 sorting efficiency, 115-16 sorting purity, 110—14 sorting times, 110 sorting yield, 110-14 sources of variation, 165 spherical aberation, 23-4 S-phase probability distribution, 218-19, 233 spherical lenses, 22—4, 26—7 spherico-ellipsoidal flow chamber, 45—7 spectral, 49, 145-9, 259-65 absorption, 49 emission, 49, 145-9, 259-65 staining, 125-36, 243-4, 246-59, 262-4, 269-73, 282-3 antibody combination, 127-9, 282-3 cytoplasmic antigens, 131—2 DNA, see nucleic acid stains factors influencing, 134-5, 243-4, 262-4 fluorochrome amplification, 129-31 interactive stains, 132-3
liposomes, 131 non-interactive stains, 136 nuclear antigens, 132-3, 269-73 RNA, 246-59 surface antigens, 126-7 standards, 159, 244-6 statistics, 14-17, 97-100, 110-14, 143, 170-1 binomial, 14, 113-14 Gaussian, 97-100 Poisson, 15-17, 110-14 rare event, 143 Student's-T, 97, 170-1 stoichiometry, 134—5, 239 stereo-perspective graphics, 84 stray light, 155-6 stream-in-air, see jet-in-air streptavidin, 130-1, 169, 241 sweep-scanning, 142 SV-40 large T, 269, 283 synthetic peptide antibodies, 132 tertiary data space, 84-92 testicular cancer, 360-1 Texas red, 50 therapy selection in oncology, see applications in oncology thiazole orange, 50, 207 thick lenses, 29-30 thinfilms,33 thin lenses, 23-5 thioflavine T, 50, 207 three-dimensional (trivariate) data, 84-6 time, 182-5, 310-17, 320-35 in quality control, 182-5 incorporation into data base, 310-17 continuous, 311-13 continuous interrupted sampling, 310 computer clock, 181, 311 discontinuous sequential sampling, 310 short time scales, 312-17, 333-5 kinetics with, 310, 312-17, 320-35 topoisomerases, 269, 274, 297-8 transverse emission mode (TEM), 57 tricyclic antibiotics, 51, 201—3 tricyclic heteroaromatic dyes, 204—7 triggering, 177-9, 191 trivariate (three-dimensional) data, 84-6 trout red cells, 244-6 trypsin, 118 tryptophan, 132 tubulin, 283, 287 tumour growth rate, 239-41, 356, 380-4 tumour suppressor genes, 357 turbulent flow, 7-8 two-dimensional (bivariate) data, 81, 195-8, 283-5
INDEX
443
tyrosine, 132
vortex, 10
variable gain, 160-5 •1-,^-f ,«., , we . ,„« verapamil, 341, 372, 375, 377 viability, 194-8 vibration, 154 voltage thresholds, 177-9
L J J J L • I ^™ n ^C-T ^ wax embedded material, 120-2, 351-6, 358
"6
Young's experiment, 32