How to measure your microscope’s HPF. A critical guide for residents
Mitoses can signal biological aggressiveness. Most drugs used in oncology inhibit cell proliferation (unfortunately, not only that of the tumor), and therefore it is wise to limit the use of these drugs in patients who might benefit from them. In most cases, chemotherapy – neoadjuvant or adjuvant – is given in high-grade tumors and we see results since many grading systems use mitotic count . In the beginning, mitotic count was reported as the total number of mitoses counted over a surface expressed in number of high-power fields (HPF). The problems with mitotic count are multiple and well-established . Given that mitoses are identified and recognized , quite a few variables can ruin your count: among them delayed fixation can reduce mitotic activity, tumor heterogeneity can limit reproducibility, and thicker slices can increase the count. However, the most discussed variable is the surface area evaluated. Digital pathology will at least solve this problem , but since it is not implemented in most centers, many pathologists still peer with their own eyes HPFs of different surfaces.   KNOW THYSELF How to consistently assess the same surface area? Most of the Blue Books by the WHO report a table that converts diameter to surface . Useful, if you forgot how to compute the area of a circle starting from the diameter , but you know the diameter of your field of view with an accuracy of 10 μm. Every medical student or pathology resident approaching the microscope for the first time wrestles with the calculation of field diameter. Some win, and timidly write the numbers with a permanent marker on the microscope base, many others – encouraged by prominent textbooks, popular guidelines and older colleagues – wave their hands and approximate. Here we will review three ways to accomplish this task. THE RULER As pathologists we are used to measure stuff. Ruler and scale are necessary even for autopsies. In surgical pathology, size matters more than weight and residents and pathologist’s assistants measure, ruler at hand, fragments, surgical specimens and tumors. Can we use a ruler under the microscope? Sure! Some tasks – such as measuring the tumor size – can be done with precision under the microscope by sliding a transparent ruler together with the slide . Okay, but we need to measure fractions of millimeters. What if we had a teeny-tiny ruler on a glass slide to measure the diameter of the field of view? That would be awesome! Good news, they do exist and they are cheap too! Try to put “stage calibration slide micrometer ruler” in your favorite search engine and you will see an image similar to . Before you buy it, check whether someone in your department already has it, hidden and forgotten in a drawer. Once you hold the slide in your hand, the game is clear. Put it under the microscope (you will see ), and do what your – pathologically trained – eyes are doomed to do: meaure with precision the size of your HPF. Slide the last tick to the end of the visible field and count the ticks. Let’s say you counted 0.52 mm, now you can plug this value into the formula to compute the area of a circle starting from the diameter (or use the ) and voilà you have the surface of your microscope HPF (in our example 0.2124 mm 2 ). A BIT OF PHYSICS Our diagnoses are made by slamming photons into tissue, sometimes using quantum properties of light . Therefore, understanding a bit of optics can be useful. The width of the field under the microscope is a function of the eyepiece’s width and the objective’s magnification. These data have been under your nose the whole time. Look at the eyepiece . There are two numbers: the first, followed by an “X”, indicates the magnification of the lens; the second, after a “/” is the width of your eyepiece in mm. Now look at your 40X objective . You can see quite a few numbers, but you already know the magnification factor! To calculate the diameter (d) in mm you just need to divide the width of your eyepiece (in mm) – called field number (f n ) – by all the magnification factors. Often the only one present is the magnification of the objective (m o ) so: d = f n /m o . For example, for a 22 mm eyepiece and a 40X objective, in the absence of any further magnification, the diameter of the field is 0.55 mm and the surface is therefore 0.238 mm 2 . STARGAZING Have you ever seen an astronomical quadrant? It has something in common with your microscope (and calipers). It is the Vernier scale (named after the French mathematician Pierre Vernier). Look at the stage of the microscope, you will see two opposing rulers – on two of the four sides. Look closer . The shorter ruler is not perfectly aligned to the longer one, it is fine. This is the Vernier scale. It allows you to measure lengths with the precision of 0.1 mm. How does it work? Align the two 0 on the two rulers, the tenth tick of the shorter ruler will be on the ninth tick of the longer one. The latter is a regular ruler with the ticks in millimeters. The shorter one shows the ticks at 0.9 mm, therefore when the zeros are aligned, the tenth tick falls on the ninth tick of the longer ruler (9 mm). Gently move the stage and the rulers will misalign . Now to understand how much you moved, you have to see where the zero of the short ruler falls (this will be the millimeters you moved) and which tick of the short ruler aligns with the tick of the long one (this will be the tenth of mm you moved). Although this method might help you when navigating with an astronomical quadrant, it is the most complicated presented and also the least accurate (only to 0.1 mm).   How to consistently assess the same surface area? Most of the Blue Books by the WHO report a table that converts diameter to surface . Useful, if you forgot how to compute the area of a circle starting from the diameter , but you know the diameter of your field of view with an accuracy of 10 μm. Every medical student or pathology resident approaching the microscope for the first time wrestles with the calculation of field diameter. Some win, and timidly write the numbers with a permanent marker on the microscope base, many others – encouraged by prominent textbooks, popular guidelines and older colleagues – wave their hands and approximate. Here we will review three ways to accomplish this task.   As pathologists we are used to measure stuff. Ruler and scale are necessary even for autopsies. In surgical pathology, size matters more than weight and residents and pathologist’s assistants measure, ruler at hand, fragments, surgical specimens and tumors. Can we use a ruler under the microscope? Sure! Some tasks – such as measuring the tumor size – can be done with precision under the microscope by sliding a transparent ruler together with the slide . Okay, but we need to measure fractions of millimeters. What if we had a teeny-tiny ruler on a glass slide to measure the diameter of the field of view? That would be awesome! Good news, they do exist and they are cheap too! Try to put “stage calibration slide micrometer ruler” in your favorite search engine and you will see an image similar to . Before you buy it, check whether someone in your department already has it, hidden and forgotten in a drawer. Once you hold the slide in your hand, the game is clear. Put it under the microscope (you will see ), and do what your – pathologically trained – eyes are doomed to do: meaure with precision the size of your HPF. Slide the last tick to the end of the visible field and count the ticks. Let’s say you counted 0.52 mm, now you can plug this value into the formula to compute the area of a circle starting from the diameter (or use the ) and voilà you have the surface of your microscope HPF (in our example 0.2124 mm 2 ).   Our diagnoses are made by slamming photons into tissue, sometimes using quantum properties of light . Therefore, understanding a bit of optics can be useful. The width of the field under the microscope is a function of the eyepiece’s width and the objective’s magnification. These data have been under your nose the whole time. Look at the eyepiece . There are two numbers: the first, followed by an “X”, indicates the magnification of the lens; the second, after a “/” is the width of your eyepiece in mm. Now look at your 40X objective . You can see quite a few numbers, but you already know the magnification factor! To calculate the diameter (d) in mm you just need to divide the width of your eyepiece (in mm) – called field number (f n ) – by all the magnification factors. Often the only one present is the magnification of the objective (m o ) so: d = f n /m o . For example, for a 22 mm eyepiece and a 40X objective, in the absence of any further magnification, the diameter of the field is 0.55 mm and the surface is therefore 0.238 mm 2 .   Have you ever seen an astronomical quadrant? It has something in common with your microscope (and calipers). It is the Vernier scale (named after the French mathematician Pierre Vernier). Look at the stage of the microscope, you will see two opposing rulers – on two of the four sides. Look closer . The shorter ruler is not perfectly aligned to the longer one, it is fine. This is the Vernier scale. It allows you to measure lengths with the precision of 0.1 mm. How does it work? Align the two 0 on the two rulers, the tenth tick of the shorter ruler will be on the ninth tick of the longer one. The latter is a regular ruler with the ticks in millimeters. The shorter one shows the ticks at 0.9 mm, therefore when the zeros are aligned, the tenth tick falls on the ninth tick of the longer ruler (9 mm). Gently move the stage and the rulers will misalign . Now to understand how much you moved, you have to see where the zero of the short ruler falls (this will be the millimeters you moved) and which tick of the short ruler aligns with the tick of the long one (this will be the tenth of mm you moved). Although this method might help you when navigating with an astronomical quadrant, it is the most complicated presented and also the least accurate (only to 0.1 mm).   TO ERR IS HUMAN Now you have the size of your field of view. You might ask: “ How far off-target was I? ” The terms of the problem were stated by Ellis and Whitehead. In 1981 they surveyed all the microscopes marketed at the time and hypothesized a grim scenario by comparing the performance of the two extreme microscopes resulting in a 6-fold difference . This result led them to question the value of mitotic count as a marker of malignancy (in the context of smooth muscle tumor). The paper is often cited as seminal in recognizing the problem of HPF , an it is thus useful to give it a look. Gazing at the plotted numbers, they are not so bad. Seventy percent of the marketed microscopes have a median field of view equal to 0.38 mm with an interquartile range (IQR) of 0.35-0.45 mm – note that the upper limit is close to the modern microscopes . The remaining 8 marketed microscopes depart from the previous group, with a median field of view of 0.66 mm (IQR 0.6-0.7 mm). They were outliers at the time and would be outliers today as well. Let’s use the data at hand: in their example of 5 mitoses per mm, it is true that the extreme microscopes would give very different counts (4 vs. 21), but if we do a simple summary statistics of the counts instead of comparing the extremes, numbers are not so grim (median is 8 mitoses and IQR 5-14; i.e. half of the counts differ at most by 9 mitoses), and today they would be even less so - with less variation among the marketed microscopes. Moreover, what is most reassuring is that outliers are rare in the market: the bulk of the microscopes out there are alike and therefore the scenario is further tempered. THE GIST OF COUNTING Today, with less variation among marketed microscopes, problems might instead arise when the numbers of HPFs reported in papers and books are naively applied without converting them in mm 2 . Since the error is multiplicative, the worst case scenario is when you repeat it the most. The mitotic figures in gastrointestinal stromal tumors (GISTs) are counted over 5 mm 2 , although even recent papers on prominent journals report the surface in 50 HPF . We read that books and guidelines tell you to approximate 5 mm 2 counting between 20 and 25 HPF. If you are not aware of the trick you might also be tempted to count 50 HPF. Now, the bright line in GIST is 5 mitoses/5 mm 2 : there would be no difference in counts when approximating, whereas using the wrong counting strategy, that uses naively 50 HPF, overestimates the number of mitoses, reporting 5 of them when there were 3 instead . This may be a problem. MAYBE NOT Mitoses are just part of the picture. They are combined with size and site to compute the risk class . This is true also for other pathologies: mitoses do notdetermine grading on their own. To understand the impact let’s look at an example. is a Montecarlo simulation of 10,000 GISTs. First, the simulation generated random sites respecting the proportion reported in literature ; similarly, it generated mitoses ; lastly the simulation produced the sizes as a function of mitoses (easy to imagine why) and the sites (with the idea that an esophageal GIST tends to be smaller because symptoms will appear sooner). Now that we have the largest GIST dataset ever built (just good for this example), let’s play with it and compute the risk class – according to Miettinen and Lasota – for each count. As expected, if you approximate there is almost perfect agreement. The punchline is that even in the worst case scenario (counting 50 HPF instead of 23.5 HPF) there is only a 0.2-fold increase in the high risk class whereas the others are under-diagnosed by a factor of 0.1, with a substantial agreement between the two counting strategies (see caption for more details). Not too bad. NOT JUST COUNTING Since we will soon be confronted with machines, it is time to be precise and accurate. To do this with your peers, you need to know the size of your HPF. Now you know how to measure it. Do it now! Lastly, even in the worst case scenario, the results are not so grim, and pathology is not just counting.   Now you have the size of your field of view. You might ask: “ How far off-target was I? ” The terms of the problem were stated by Ellis and Whitehead. In 1981 they surveyed all the microscopes marketed at the time and hypothesized a grim scenario by comparing the performance of the two extreme microscopes resulting in a 6-fold difference . This result led them to question the value of mitotic count as a marker of malignancy (in the context of smooth muscle tumor). The paper is often cited as seminal in recognizing the problem of HPF , an it is thus useful to give it a look. Gazing at the plotted numbers, they are not so bad. Seventy percent of the marketed microscopes have a median field of view equal to 0.38 mm with an interquartile range (IQR) of 0.35-0.45 mm – note that the upper limit is close to the modern microscopes . The remaining 8 marketed microscopes depart from the previous group, with a median field of view of 0.66 mm (IQR 0.6-0.7 mm). They were outliers at the time and would be outliers today as well. Let’s use the data at hand: in their example of 5 mitoses per mm, it is true that the extreme microscopes would give very different counts (4 vs. 21), but if we do a simple summary statistics of the counts instead of comparing the extremes, numbers are not so grim (median is 8 mitoses and IQR 5-14; i.e. half of the counts differ at most by 9 mitoses), and today they would be even less so - with less variation among the marketed microscopes. Moreover, what is most reassuring is that outliers are rare in the market: the bulk of the microscopes out there are alike and therefore the scenario is further tempered.   Today, with less variation among marketed microscopes, problems might instead arise when the numbers of HPFs reported in papers and books are naively applied without converting them in mm 2 . Since the error is multiplicative, the worst case scenario is when you repeat it the most. The mitotic figures in gastrointestinal stromal tumors (GISTs) are counted over 5 mm 2 , although even recent papers on prominent journals report the surface in 50 HPF . We read that books and guidelines tell you to approximate 5 mm 2 counting between 20 and 25 HPF. If you are not aware of the trick you might also be tempted to count 50 HPF. Now, the bright line in GIST is 5 mitoses/5 mm 2 : there would be no difference in counts when approximating, whereas using the wrong counting strategy, that uses naively 50 HPF, overestimates the number of mitoses, reporting 5 of them when there were 3 instead . This may be a problem.   Mitoses are just part of the picture. They are combined with size and site to compute the risk class . This is true also for other pathologies: mitoses do notdetermine grading on their own. To understand the impact let’s look at an example. is a Montecarlo simulation of 10,000 GISTs. First, the simulation generated random sites respecting the proportion reported in literature ; similarly, it generated mitoses ; lastly the simulation produced the sizes as a function of mitoses (easy to imagine why) and the sites (with the idea that an esophageal GIST tends to be smaller because symptoms will appear sooner). Now that we have the largest GIST dataset ever built (just good for this example), let’s play with it and compute the risk class – according to Miettinen and Lasota – for each count. As expected, if you approximate there is almost perfect agreement. The punchline is that even in the worst case scenario (counting 50 HPF instead of 23.5 HPF) there is only a 0.2-fold increase in the high risk class whereas the others are under-diagnosed by a factor of 0.1, with a substantial agreement between the two counting strategies (see caption for more details). Not too bad.   Since we will soon be confronted with machines, it is time to be precise and accurate. To do this with your peers, you need to know the size of your HPF. Now you know how to measure it. Do it now! Lastly, even in the worst case scenario, the results are not so grim, and pathology is not just counting.      