iBiology

Bringing the World's Best Biology to You

Home » Courses » Microscopy Series » Contrast Generation for Transmitted Light

Differential Interference Contrast (DIC) Microscopy

00:00:12.10 I'd like to begin this talk
00:00:14.12 by asking you to look at these
00:00:16.13 three images of isolated spindles,
00:00:19.05 and the object here in the middle
00:00:26.06 is a phase contrast image of the spindle,
00:00:29.11 and as discussed in the phase contrast lecture,
00:00:33.28 the contrast that we see,
00:00:35.08 the dark contrast,
00:00:37.24 is based on the difference in the refractive index,
00:00:41.10 that being slightly greater refractive index,
00:00:44.11 of the specimen objects here,
00:00:48.11 which... most of these dots are
00:00:50.04 clusters of ribosomes to the background,
00:00:52.18 and these are the chromosomes at the metaphase plate,
00:00:55.17 these are spindle fibers here
00:00:57.23 that make up the central spindle,
00:01:00.01 and these are the astral microtubules rays
00:01:04.05 on either side of this metaphase spindle.
00:01:07.04 And on the right-hand side, which...
00:01:12.05 I have to move over here a little bit...
00:01:13.27 this is the image of the same spindle
00:01:16.16 that we see in polarization microscopy
00:01:20.00 that we've discussed in
00:01:21.28 the polarization microscopy lecture,
00:01:23.24 and here those ribosome globs are invisible,
00:01:27.23 and what we see are
00:01:31.21 the submicroscopic contrast
00:01:36.11 generated by the aligned microtubules
00:01:38.15 that make up the central spindle fibers,
00:01:40.20 and the microtubules that are in the aster of the spindle,
00:01:43.16 because they're optically anisotropic,
00:01:47.06 they have a refractive index
00:01:51.18 for the electric field vibration
00:01:55.09 along the axis of the spindle...
00:01:57.26 is greater than the refractive index
00:02:02.04 for vibration in the normal direction.
00:02:04.28 And this generates birefringence,
00:02:07.04 which is turned into contrast in a polarizing microscope, as...
00:02:13.22 and that will become important in our DIC talk,
00:02:20.06 because the DIC image that you see over here
00:02:22.10 is actually made with a polarizing microscope.
00:02:26.25 And so, to understand DIC
00:02:31.01 image contrast generation,
00:02:32.18 you first have to have some understanding
00:02:35.26 of how a polarization microscope
00:02:37.26 converts birefringence retardation
00:02:40.08 of two orthogonally vibrating waves
00:02:46.03 into contrast,
00:02:47.27 because that's used
00:02:50.14 in a different optical configuration
00:02:53.07 in DIC microscopy
00:02:55.07 to make this image, here,
00:02:57.03 which highlights the edges of objects.
00:02:59.05 And so, if you look at the image here,
00:03:00.22 you'd say, wow,
00:03:02.25 it looks like somebody shined a light from this side
00:03:05.08 and we have oblique illumination,
00:03:07.19 and this clump of ribosomes here
00:03:09.26 is scattering light off this side,
00:03:12.19 but because the light is obliquely illuminating
00:03:14.20 it looks dark on the other side.
00:03:16.23 And it turns out that that's completely wrong,
00:03:19.08 you know, it has nothing...
00:03:20.26 the illumination of the specimen
00:03:22.18 is uniform across the specimen
00:03:24.25 and contrast is not generated
00:03:26.25 by a form of oblique illumination.
00:03:29.17 But you can see that in this case,
00:03:31.23 it's the edges that are highlighted
00:03:33.21 and not just the mass of the object,
00:03:37.05 such as in phase contrast.
00:03:39.11 And the birefringence is not visible,
00:03:42.19 but we do see the fibrous structure
00:03:45.14 of the clustering of microtubules in the asters
00:03:47.24 and the clustering of microtubules
00:03:50.10 that take place in the central spindle fibers.
00:03:53.21 So, I would like to ask you to
00:03:59.25 sort of look at this image,
00:04:01.00 which is a video-enhanced DIC image
00:04:03.08 of individual microtubules
00:04:05.07 that are only 25 nanometers in diameter.
00:04:08.07 They're made out of tubulin dimers
00:04:12.20 that are stacked head to tail
00:04:14.13 into protofilaments
00:04:15.26 and there are 13 of these protofilaments, here,
00:04:18.08 that make the cylindrical wall of a microtubule,
00:04:22.27 and so those microtubules, here,
00:04:24.29 are held on the surface of a glass coverslip
00:04:27.13 by the motor protein kinesin
00:04:30.22 that my host Ron Vale discovered,
00:04:34.07 with his colleagues,
00:04:38.04 using video-enhanced DIC microscopy
00:04:40.07 in the middle of the 1980s.
00:04:42.24 And this image is highly magnified
00:04:47.01 and, as a consequence,
00:04:48.26 it's a good one to ask about
00:04:50.29 what the 6 major features are of a DIC image.
00:04:53.09 And I want to start having you look
00:04:56.19 at tiny particles,
00:04:59.08 like this one over here
00:05:02.10 and then there's another one down over here,
00:05:05.17 whoops, here we go,
00:05:06.27 there's one right down here,
00:05:08.13 and there's one right there, alright?
00:05:10.22 And if you look at these tiny little particles
00:05:13.23 -- they may have a size that's even less than
00:05:17.01 the microtubule, right? --
00:05:18.18 they all have the same sort of image structure --
00:05:21.24 one side has got a bright spot,
00:05:26.17 the other side has a dark spot --
00:05:28.06 and if you look at each one,
00:05:29.25 they all have a light-dark spot
00:05:31.19 lined up in the same direction
00:05:33.23 and that direction, here,
00:05:37.09 is roughly running
00:05:39.21 from about 10 o'clock to 4 o'clock,
00:05:41.05 in the axis that bisects the light
00:05:44.08 and the dark spot,
00:05:46.05 and that direction is called the shear direction
00:05:48.23 of the DIC image --
00:05:50.10 it's the direction of highest contrast.
00:05:53.13 Alright?
00:05:54.20 And the brightness of the bright spot
00:05:56.25 or the dark spot
00:05:58.21 depends on how much scattered light is produced
00:06:01.25 by the specimen,
00:06:02.27 which depends on the protein density there,
00:06:04.14 and that could be different for the
00:06:06.17 different little, tiny spots.
00:06:08.12 The protein density for the microtubules
00:06:10.20 is fairly uniform along the length,
00:06:12.08 and so the image that you see for microtubules
00:06:14.04 looks rather constant
00:06:16.18 along the length of the microtubule,
00:06:18.15 but it differs for different directions.
00:06:20.13 So, if... what these bright and dark spots are
00:06:24.21 are actually two Airy disks,
00:06:26.25 so the DIC image is made up of two...
00:06:29.18 instead of a single Airy disk
00:06:31.16 defining each image point
00:06:33.07 from a point in the specimen,
00:06:34.21 there are two Airy disks
00:06:36.25 defining an image point
00:06:40.02 from a single point in the specimen,
00:06:42.23 and one of those Airy disks is highlighted,
00:06:44.27 in normal DIC,
00:06:47.02 as brighter than the background
00:06:48.14 and the other Airy disk is highlighted
00:06:50.09 as darker than the background.
00:06:53.09 So, if you think about that,
00:06:55.12 you could say, well,
00:06:56.27 each one of these tubulin dimers
00:06:58.20 is scattering light,
00:07:00.06 so if we look at a microtubule over here...
00:07:04.25 I'm going to first point at this particle,
00:07:06.09 and you can see it's black and white this way,
00:07:08.09 and so if we look at this microtubule right here,
00:07:11.28 you can see this left...
00:07:13.11 this edge here on the left is black
00:07:14.26 and this right edge is white,
00:07:16.11 and all along the length of this...
00:07:19.02 right, we have black, white,
00:07:21.04 duhduhduhduhduhduh,
00:07:23.08 all the way up to this point here,
00:07:26.02 which probably it came up off the coverslip,
00:07:27.27 so you don't get to see it, alright?
00:07:30.10 And so it's just simply that
00:07:33.18 all these individuals scatterers, here,
00:07:35.28 are all producing this paired white/black image,
00:07:40.04 they're all stacked linearly on each other
00:07:43.08 and that then defines the axis of the microtubule,
00:07:45.22 okay?
00:07:47.26 On the other hand, if we go look at a microtubule
00:07:50.13 that's oriented in the direction
00:07:52.28 of this shear direction between these two Airy disks,
00:07:56.15 and there's one right here, see it?
00:07:59.25 You can barely see the microtubule,
00:08:01.25 and that's because black,
00:08:04.06 and then the overlay is white,
00:08:06.20 overlay is black, overlay is white,
00:08:07.28 overlay is black, overlay is white,
00:08:09.22 and the net sum of those two, alright,
00:08:12.11 when added together,
00:08:13.26 gives you very little contrast relative to the background.
00:08:16.21 And so contrast is maximal
00:08:19.04 in the direction of shear, alright?
00:08:21.26 And if we look at this larger object, over here, right there,
00:08:26.09 which is a blob of membrane
00:08:31.02 or a vesicle of some sort
00:08:32.26 that's settled on the coverslip surface, there,
00:08:34.20 in this preparation,
00:08:36.22 you can see that the right edge, again, is bright,
00:08:40.02 the left edge is dark,
00:08:41.25 but in the middle you have the same intensity as the background light.
00:08:46.22 So what is highlighted is the edge,
00:08:49.15 not the middle,
00:08:51.21 and again we can take the same analogy, here.
00:08:53.28 If you take one of these particles, right,
00:08:57.14 and think of that as like a unit scatterer in this vesicle,
00:09:01.12 right here,
00:09:03.08 we still have black, white, black, white,
00:09:06.07 and then here, all of a sudden,
00:09:08.14 we now have black and white overlapping each other,
00:09:10.24 overlapping each other,
00:09:12.04 overlapping each other,
00:09:13.22 overlapping each other,
00:09:14.14 alright, so we get the same contrast as the background,
00:09:17.11 and then finally when we get to the left edge,
00:09:19.24 we now have blacks that don't have
00:09:22.28 corresponding whites to overlap them,
00:09:24.15 and so on the periphery of the left edge
00:09:26.18 we now get black contrast, right?
00:09:31.02 So, fundamentally,
00:09:32.15 it's the same mechanism
00:09:34.17 that generates contrast at this tiny little point, here, object,
00:09:39.02 is the same mechanism that generates
00:09:40.22 the edge contrast that you see in the DIC.
00:09:43.03 So, then we need to understand
00:09:45.03 how those two images are made,
00:09:48.04 how their contrasts relative to the background are generated,
00:09:52.18 and how this is done in the polarizing microscope.
00:09:56.00 And in the next slide, here,
00:09:58.01 I've summarized the major features, again,
00:10:00.18 that we've just discussed,
00:10:02.09 which are: contrast is directional,
00:10:04.22 it's a maximum in one direction and a minimum in the orthogonal direction;
00:10:07.17 contrast highlights edges,
00:10:09.21 uniform areas have brightness of the background;
00:10:12.04 in the direction of contrast,
00:10:14.10 one edge is brighter,
00:10:16.07 the other darker than the background;
00:10:18.27 each point in the object is represented
00:10:21.02 by two overlapping Airy disks
00:10:23.05 in the image,
00:10:24.28 one brighter and one darker than the background,
00:10:27.16 the way DIC is normally set up to be used;
00:10:31.11 the direction of the Airy disk separation,
00:10:34.08 this light/dark pair,
00:10:36.29 is the shear direction
00:10:39.07 and the direction of maximum contrast;
00:10:42.29 and the peak-to-peak separation
00:10:45.11 of the two black/white Airy disks
00:10:46.25 is the amount of shear,
00:10:49.08 shear being a term for the separation of those two images,
00:10:54.23 and it's typically chosen to be about 1/2,
00:10:58.03 sometimes 2/3,
00:10:59.20 but usually 1/2 of the radius of the Airy disk,
00:11:02.08 so that you can approach
00:11:05.21 the maximum resolution possible of the objective,
00:11:07.26 even though you're making up the image
00:11:10.03 out of two Airy disks.
00:11:13.24 Okay, so how do we make such an image?
00:11:16.21 So, a DIC microscope
00:11:18.13 is a polarizing microscope,
00:11:21.01 so to understand DIC
00:11:22.23 you need to understand
00:11:24.14 the fundamental aspects of
00:11:27.13 polarization microscopy.
00:11:28.24 So, before you go any further in this talk,
00:11:31.10 you really need to go back
00:11:33.01 and listen to the talks
00:11:34.18 that were given by Shinya Inoue and by myself
00:11:38.07 on polarization microscopy,
00:11:40.27 and I'm assuming that you've listened to those two talks
00:11:42.22 in what I'm going to say now. Okay?
00:11:44.27 So, to set up a microscope for DIC,
00:11:50.05 what you're really doing
00:11:51.25 is making a dual-beam interferometer
00:11:53.16 in which the two beams
00:11:55.05 are very close together --
00:11:57.01 that is, in a sense, they're only separated
00:11:58.13 by that shear amount, right,
00:12:00.29 that will eventually produce those two overlapping Airy disks.
00:12:04.08 And this is done by
00:12:07.24 aligning your microscope and objectives and condensors
00:12:11.13 for Koehler illumination
00:12:13.11 and then, in addition,
00:12:15.22 you have the normal setup
00:12:18.25 for polarization microscopy.
00:12:20.16 We have a polarizer
00:12:22.19 near the condenser/diaphragm plane,
00:12:24.28 we have an analyzer above the objective,
00:12:27.23 the back focal plane and aperture
00:12:31.03 where we can get it in and out of the microscope path,
00:12:33.05 and in addition there's a compensator used in the system
00:12:37.16 that can either be before the analyzer
00:12:39.09 or just after the polarizer,
00:12:42.12 and that is a birefringent retardation plate
00:12:46.22 that can be used to advance one of the...
00:12:55.27 used in the system which I'll describe, here,
00:12:59.05 I think a little bit later.
00:13:01.04 And then, in addition,
00:13:03.17 there is a condenser DIC prism
00:13:07.22 that's going to split the initial beam of light
00:13:10.23 into two beams
00:13:12.12 that are going to pass through the specimen,
00:13:14.28 and then there's
00:13:17.19 a conjugate DIC prism for the objective
00:13:20.23 that will recombine these beams
00:13:22.26 and then send the recombined beams
00:13:24.24 through the compensator
00:13:26.18 and then the analyzer
00:13:28.07 and then contrast will come back up at the analyzer.
00:13:30.29 So, the contrast that you get out of this system, here,
00:13:33.26 depends basically on how we get contrast
00:13:37.07 from birefringent retardation
00:13:38.23 in polarization microscopy,
00:13:40.15 which is why you need to look at those
00:13:42.16 other two lectures.
00:13:44.19 Alright. And so...
00:13:48.01 how do we make the two beams?
00:13:50.11 And this is done with
00:13:53.07 the DIC prism in the condenser.
00:13:56.19 Initially, one version of the DIC system,
00:14:00.19 when it was first invented back in the 60s,
00:14:06.00 used what's called a Wollaston prism,
00:14:10.22 and this was put in the condenser front focal plane,
00:14:14.01 and this one was made out of quartz,
00:14:16.08 which is a birefringent crystal,
00:14:18.11 and, being birefringent,
00:14:20.14 it has two refractive indices.
00:14:23.23 One of them, here,
00:14:26.14 I've shown for the upper wedge,
00:14:29.21 has its vibration axis this way,
00:14:32.25 and the other one is going to be into the board,
00:14:34.20 and these two wedges are cut
00:14:40.13 so that they're what's called
00:14:44.05 the optic axis of the crystal...
00:14:45.25 and in the case of quartz,
00:14:49.12 it's the axis that has the
00:14:51.06 extraordinary refractive index
00:14:55.21 and it has an electric field vibration
00:14:58.12 in the direction of this axis,
00:15:02.13 and it's the larger value for quartz,
00:15:04.24 compared to the one that's perpendicular to it,
00:15:07.01 which is shown here by a dot,
00:15:11.02 which is the...
00:15:13.08 would be called the ordinary ray for quartz.
00:15:14.22 So, in the bottom wedge
00:15:16.18 I think is where we define these things.
00:15:18.02 And so, for the bottom wedge,
00:15:20.02 this axis of symmetry
00:15:22.03 is into the plane of the board, here,
00:15:25.00 alright, and so the...
00:15:28.07 n-sub... what's called n-sub-e value,
00:15:31.06 in the direction of the axis of symmetry
00:15:33.15 of the quartz crystal,
00:15:34.25 is into the board,
00:15:36.20 and that's this one,
00:15:38.02 and that has a higher refractive index,
00:15:40.00 and the n-sub-o value for quartz,
00:15:43.28 which is produced as
00:15:46.25 a wave perpendicular to it,
00:15:48.05 is in the plane of the board,
00:15:50.03 and these prisms in the microscope
00:15:51.28 are inserted into the microscope
00:15:54.05 at 45...
00:15:56.14 with their axes at 45 degrees to the polarizer direction,
00:15:58.19 and so in this drawing I've put the polarizer...
00:16:03.20 polarized light coming from the polarizer, here,
00:16:06.11 at 45 degrees to the direction of
00:16:09.11 these vibration axes in the crystal.
00:16:11.06 Now, when you take plane polarized light
00:16:14.27 and, coming along through space,
00:16:17.21 and you hit a birefringent crystal,
00:16:20.06 instantly the energy from the electric field
00:16:25.00 is resolved into two
00:16:27.27 orthogonally plane polarized light beams,
00:16:29.20 one vibrating in the n-sub-e direction
00:16:31.26 and one vibrating in the n-sub-o direction,
00:16:34.00 right?
00:16:35.01 And so, for the bottom quartz wedge,
00:16:37.21 if I start with plane polarized light
00:16:39.23 and I'm going through the air,
00:16:42.05 which has a low refractive index
00:16:43.27 and I hit the crystal,
00:16:45.07 then once I'm in the crystal
00:16:47.27 the frequency of vibration is the same
00:16:49.20 because it's transparent,
00:16:51.04 but one wave goes slow
00:16:53.15 and the other wave goes fast.
00:16:54.29 The slow one has a higher refractive index
00:16:57.16 and the fast one has the smaller refractive index.
00:17:00.25 And I've shown that in the drawing here
00:17:03.06 by this dot, here...
00:17:08.21 is the wave that's vibrating into the board
00:17:12.15 and it's going slower
00:17:14.29 compared to the wave
00:17:17.16 that's vibrating perpendicular to that.
00:17:20.13 These two vibrations
00:17:23.17 are orthogonal to each other
00:17:25.15 and electric fields that are orthogonal to each other
00:17:29.01 cannot interfere,
00:17:30.23 so we're generating, across this wave front, here,
00:17:35.08 coming from the polarizer,
00:17:37.15 by using this first wedge,
00:17:39.17 is we're generating
00:17:43.12 two orthogonally plane polarized light beams
00:17:45.06 that are vibrating...
00:17:46.29 the electric fields are vibrating
00:17:49.01 in the direction of the crystallographic axes,
00:17:52.07 right, and in the lower wedge
00:17:54.07 you can see that the n-sub-e one
00:17:57.21 is slow compared to the n-sub-o one,
00:18:00.22 and then we hit the wedge boundary,
00:18:03.09 in which the axes directions of the crystal
00:18:06.17 are reversed.
00:18:07.26 This causes a refraction at the boundary
00:18:10.20 so that the wave...
00:18:15.21 one wave is bent away
00:18:17.28 and moves off to the right,
00:18:20.17 that's this one here,
00:18:22.26 and the other wave is bent the other way
00:18:24.17 and moves off to the left,
00:18:26.26 and so this looks like the two wave fronts
00:18:29.05 then diverge from each other,
00:18:30.21 based on the angle of this wedge
00:18:33.07 and on the differences in refractive index, alright?
00:18:36.03 So, what we have coming from the wedge
00:18:38.16 are these two wave fronts.
00:18:40.23 There's one I've drawn, here,
00:18:42.20 that's going... uhh...
00:18:43.27 let's see if I can do this, here...
00:18:45.05 this is a little hard,
00:18:46.22 but you can see one is tilted to the right
00:18:48.18 and the other wave front
00:18:52.11 is tilted to the left
00:18:53.29 and heading out towards the condenser lens
00:18:55.29 as it moves away from this Wollaston prism.
00:19:01.24 Now, in a microscope...
00:19:07.03 let's consider first this lower drawing...
00:19:09.17 we'll consider the wave fronts
00:19:11.15 that are coming right from the center of the prism,
00:19:16.18 in which the thickness of the lower prism
00:19:19.01 is equal to the thickness of the upper prism,
00:19:21.03 and because those two thicknesses are the same,
00:19:23.17 even though the wave fronts are diverging from each other,
00:19:27.01 they are in phase with each other...
00:19:29.27 okay...
00:19:32.12 in terms of their propagation coming...
00:19:36.01 I've got to actually do it this way...
00:19:39.01 in terms of their propagation going through the microscope.
00:19:42.01 So, you can see that the dot, here,
00:19:45.13 for this wave front,
00:19:48.06 and the bar, here, for that wave front,
00:19:51.10 are actually right in line with each other.
00:19:54.02 But if we go to the top of the prism,
00:19:57.03 because the lower prism is thicker than the higher prism,
00:20:00.15 then one wave gets way behind the other wave,
00:20:05.00 alright,
00:20:06.11 but because they're coming from...
00:20:08.08 and then you'd have the same sort of drawing,
00:20:10.19 but equal and opposite
00:20:12.19 for the other end... for the other side of the prism,
00:20:16.01 but I only drew just one of these...
00:20:17.20 but note that for both of these waves,
00:20:20.03 this one here and the one coming from
00:20:23.05 near the outer aperture of the...
00:20:26.00 entering into the outer aperture of the condenser,
00:20:28.19 because they're coming from the front focal plane,
00:20:31.06 they then get converted into parallel beams
00:20:34.22 that move through the specimen,
00:20:37.12 and those beams are separated
00:20:39.03 by the shear separation,
00:20:42.02 as reflected in the specimen plane.
00:20:44.28 And that will be roughly the same for either...
00:20:47.09 whether this is a parallel beam
00:20:48.26 or whether it's a high numerical aperture beam
00:20:52.08 that's moving through the specimen.
00:20:53.23 Now, the objective
00:20:57.06 and then the objective prism
00:21:00.18 are chosen to be conjugate, in effect,
00:21:04.17 to produce an equal and opposite effect in what was done, here,
00:21:08.13 by the condenser prism and the condenser lens itself,
00:21:11.17 so that these two beams
00:21:14.03 are then focused back together again
00:21:16.12 at what would be the back focal plane in this alignment, right?
00:21:22.04 And then... what happened here?
00:21:24.27 What happened to the two beams up here?
00:21:27.11 You get an equal and opposite effect, here,
00:21:29.10 and if everything is perfectly matched...
00:21:33.09 I'm going to have to move my finger this way, alright...
00:21:37.11 if everything is perfectly matched,
00:21:39.14 the two beams will come out,
00:21:42.11 although vibrating orthogonally to each other,
00:21:44.20 exactly in phase with each other.
00:21:47.09 This will be true for here,
00:21:49.19 this will be true for here,
00:21:51.12 this would be true for here,
00:21:53.06 true for here...
00:21:54.23 if everything is equally matched.
00:21:56.23 And so, as we'll talk about a little later,
00:22:02.28 DIC prisms are selected
00:22:04.18 so that they match each other
00:22:06.11 in order that you can get
00:22:08.19 a perfect match and be able to extinguish the light...
00:22:11.23 have these two beams be in phase with each other
00:22:15.05 all across the aperture of the objective, alright?
00:22:18.20 Now, these beams
00:22:22.10 then hit the analyzer,
00:22:25.05 which is this next guy, right here, alright...
00:22:29.08 and if they're in phase with each other,
00:22:31.27 then what you end up having is
00:22:34.08 this same initial plane-polarized light
00:22:37.05 that came out of the polarizer.
00:22:40.04 And because the analyzer transmission vibration direction
00:22:45.12 is perpendicular to the polarizer
00:22:47.12 in the way we align the DIC scope,
00:22:50.29 it will essentially allow...
00:22:54.02 these two beams will interfere with each other,
00:22:56.13 but give no net light transferred through the analyzer,
00:22:59.21 and so we say that the light has been extinguished,
00:23:02.13 alright?
00:23:03.19 Because both of these beams
00:23:05.06 suffered the same net retardation
00:23:08.23 or the same...
00:23:09.25 they have the same optical path
00:23:11.24 going through the specimen,
00:23:13.10 and the prisms did an equal
00:23:16.00 and opposite
00:23:18.17 advancement or retardation of the two beams
00:23:21.07 as we went through, alright?
00:23:22.23 So, to see what happens
00:23:26.11 if we put a specimen in there
00:23:28.04 such that we modify what happens to one beam
00:23:30.13 relative to the other
00:23:32.11 by changes in the optical path,
00:23:33.28 I've made up a specimen down here,
00:23:37.01 which is sort of trapezoidal in shape,
00:23:41.23 and it's got a refractive index larger than the background,
00:23:45.06 and I defined regions A, B, C, and D,
00:23:48.29 and then I'm only considering
00:23:51.24 the beam that's coming
00:23:54.05 right up along the optic axis
00:23:56.13 and for this case
00:24:01.23 the o wave is drawn as a semi-dotted line, here,
00:24:06.04 and it's been translated to the right-hand side,
00:24:14.26 and the e wave, which is a solid line,
00:24:17.22 is translated to the left-hand side,
00:24:19.13 as you can see way over here,
00:24:24.29 right there, see?
00:24:26.04 The e wave ends there and the o wave ends there, alright?
00:24:27.18 So, that's the wave front that's going to
00:24:30.18 come down the microscope axis,
00:24:32.02 come up through the specimen,
00:24:34.12 and as that wave front just passes through the specimen,
00:24:38.29 because this has a higher refractive index,
00:24:41.20 both wave fronts are going to be slowed down
00:24:45.01 because of being in the specimen,
00:24:46.25 and they'll be slowed down
00:24:48.26 in proportion to the refractive index
00:24:50.18 times the thickness of the specimen, alright?
00:24:53.22 So, it's the thickness of the specimen times,
00:24:57.00 in parentheses,
00:24:59.19 the refractive index of the specimen
00:25:01.17 minus the refractive index of the background.
00:25:02.29 And so you can see this as sort of
00:25:05.25 an embossing of the shape of the specimen
00:25:07.14 on the two wave fronts, right there.
00:25:10.04 So, those two wave fronts
00:25:12.17 are then collected by the objective
00:25:17.11 and then passed through the
00:25:21.14 objective Wollaston prism,
00:25:23.01 and the objective Wollaston prism
00:25:26.06 realigns the wave fronts to each other...
00:25:30.28 you can see the o is shifted to the left
00:25:35.20 and the e is shifted to the right,
00:25:39.18 and for me shifting to the left
00:25:42.10 is not easy to do,
00:25:44.07 so I'm not going to do it,
00:25:45.24 but you can see by looking at the endpoints of these lines,
00:25:48.08 right there,
00:25:50.22 that they now line up, here,
00:25:52.29 and then over there they're now lined up.
00:25:56.21 But look what happens at the edges
00:25:59.15 -- that shifting by the objective Wollaston prism
00:26:05.04 shifts the retardations of the edges for the two wave fronts
00:26:11.23 away from each other,
00:26:13.11 so now that where we had edges,
00:26:14.24 we now have a retardation difference
00:26:18.10 between the two edges.
00:26:20.14 Now, each of these,
00:26:24.04 the e wave and the o wave,
00:26:26.08 these orthogonally vibrating waves
00:26:28.24 that go through specimen,
00:26:31.07 alright,
00:26:32.27 that go through the prism and then the specimen and so forth, right,
00:26:35.02 they have the same amplitude,
00:26:37.28 but at this stage, in the background,
00:26:40.00 in the region corresponding to A,
00:26:42.14 they have no retardation difference,
00:26:46.25 so when we go to A,
00:26:48.05 which is over here, right,
00:26:49.20 because there's no retardation difference
00:26:52.04 we get plane-polarized light,
00:26:53.26 which is canceled by the analyzer,
00:26:56.04 and we get blackness.
00:26:57.16 But at this edge, there is a retardation difference
00:26:59.10 between the two waves,
00:27:00.26 and so that retardation difference
00:27:03.03 allows light to get through the analyzer,
00:27:05.03 and we see a bump at B, alright?
00:27:08.26 At C, where we had a constant thickness of the specimen,
00:27:11.29 there's no retardation difference
00:27:14.00 between the two wave fronts,
00:27:15.15 and so for C, here,
00:27:17.10 you can see that we go back to
00:27:20.18 having the same intensity as the background,
00:27:23.11 at A, and at D, again,
00:27:26.10 we now have the retardation difference
00:27:29.00 and so at D we now have a bump again,
00:27:33.08 and then we get back to the background over here,
00:27:36.14 so we go back to being black again.
00:27:38.04 So, this is a darkfield microscopy
00:27:41.09 made in DIC, alright,
00:27:42.21 and it's not a very easy image to look at
00:27:45.01 and it's a very dark image,
00:27:47.10 and so we normally use
00:27:50.01 a compensator in the DIC microscope
00:27:53.17 to advance one of the wave fronts over the other
00:27:59.28 in order to brighten up the background.
00:28:02.08 So, if we go back,
00:28:04.27 here we've got the embossment that takes place at the image.
00:28:07.27 We now...
00:28:09.23 I mean, down here...
00:28:13.04 then we go through the Wollaston prism,
00:28:15.10 we now have realigned the two wave fronts,
00:28:18.05 but at the same time,
00:28:20.16 as we've realigned the two wave fronts,
00:28:22.03 we've split apart the images of the edges,
00:28:27.11 right, which is what produces the two Airy disks,
00:28:30.06 right, and this will now show you
00:28:35.12 why one is dark and one is white.
00:28:37.18 So, in the images that we were analyzing to begin with,
00:28:41.14 of the microtubules and the particles,
00:28:43.23 we had a compensator in the light path,
00:28:46.24 and the compensator was adjusted
00:28:49.19 such that the right-hand edge, here...
00:28:55.09 we were advancing one of the wave fronts over the other,
00:28:57.20 so that the right-hand edge
00:29:00.03 essentially has no retardation difference,
00:29:02.23 but the background,
00:29:05.03 if you look here
00:29:07.04 or you look at constant regions of the specimen,
00:29:09.11 or if you look at the background over here in A,
00:29:12.07 they all have the retardation that's been produced
00:29:15.19 by our compensator
00:29:17.09 and as a result produce light.
00:29:19.18 So, if we come way over here and go up through the analyzer,
00:29:22.19 that retardation produces light, right?
00:29:26.04 And in fact it further advances
00:29:29.15 the retardation difference between...
00:29:31.10 on the left-hand edge,
00:29:32.27 so we get a brightness that's brighter than the background
00:29:36.18 for the left-hand edge,
00:29:39.12 then in the constant region of the specimen
00:29:40.23 we get the background light intensity, again,
00:29:42.22 and then in the left-hand edge,
00:29:44.10 because there's no retardation difference,
00:29:46.09 we get darkness,
00:29:47.22 and finally we go back to the background level of intensity.
00:29:51.02 And that's what produces the light-dark image
00:29:53.24 in DIC microscopy.
00:29:55.12 Now, you can...
00:29:57.28 compensators can be used in
00:30:00.15 both additive and subtractive mode --
00:30:01.20 you can reverse whether or not
00:30:04.24 you advance the e wave over the o wave,
00:30:06.11 or you advance the o wave over the e wave,
00:30:08.16 and by doing that
00:30:10.15 you can decide to make the left-hand edge dark
00:30:13.10 and the right-hand edge bright,
00:30:15.23 and in fact that will
00:30:19.10 produce the same sort of image,
00:30:21.17 and we've done the same thing,
00:30:23.01 except for we've made the two wave fronts
00:30:28.09 actually become in phase with each other
00:30:32.04 on the left-hand edge
00:30:33.18 and enhanced the retardation of them, here, on the right-hand edge.
00:30:37.17 What kind of compensators are used to do this?
00:30:39.05 In the original designs for DIC,
00:30:41.02 one was called the Smith design,
00:30:42.26 which used these Wollaston prisms,
00:30:44.27 and they were actually built into the objective
00:30:47.26 in the objective back focal plane,
00:30:49.18 so when you bought the objective it said,
00:30:52.28 'DIC', and it had the prism in it,
00:30:54.16 so you couldn't use the objective
00:30:56.11 for other things,
00:30:58.20 because the prism was built into the objective,
00:31:00.12 and the Wollaston prism for the condenser
00:31:07.19 pretty much could be put pretty close to the condenser diaphragm plane,
00:31:10.22 so that wasn't necessarily
00:31:13.01 built into the condenser,
00:31:14.29 but because this was built into the objective
00:31:17.26 and because this was to some extent
00:31:22.04 stationary in the condenser,
00:31:24.05 there was no other way
00:31:27.28 to be able to change
00:31:30.14 the retardation of the e and the o wave
00:31:33.21 for compensation purposes,
00:31:35.05 and so an additional compensator
00:31:38.27 was added to the system,
00:31:40.11 and that's typically a de Sénarmont-type compensator,
00:31:43.19 which is made out of a quarter-wave plate retarder
00:31:47.08 and a rotatable polarizer,
00:31:49.27 or a quarter-wave plate retarder over here,
00:31:53.10 can be put other here,
00:31:55.28 and a rotatable analyzer,
00:31:57.09 and the combination of those two
00:31:59.04 allows you to rotate the polarizer or the analyzer,
00:32:03.07 and it turns out the amount of retardation
00:32:06.16 between the two orthogonal wave fronts
00:32:11.00 is proportional to the degree of that rotation.
00:32:14.16 So... and, in fact, nowadays,
00:32:18.15 de Sénarmont compensation
00:32:20.17 is very commonly used in polarization microscopy.
00:32:24.11 Nomarski modified the design
00:32:27.00 of the Wollaston prisms
00:32:30.12 to make the axis of one of the wedges different,
00:32:33.11 and this allowed him to put the prism
00:32:36.01 outside of the objective,
00:32:37.27 and in Zeiss' initial...
00:32:40.01 and they still do this in Zeiss...
00:32:41.28 in their initial implementation of this,
00:32:43.26 because this is outside the objective,
00:32:45.13 they could then put a mechanical screw mechanism on it
00:32:48.14 and translate the Wollaston back and forth
00:32:51.17 to either positively or negatively compensate...
00:32:57.15 to advance or retard the e and the o wave
00:32:59.26 relative to each other,
00:33:02.23 and you didn't need the de Sénarmont compensator.
00:33:07.01 And nowadays that's still basically
00:33:10.09 the two kinds of schemes that are used.
00:33:13.28 Now, the Nomarski prism,
00:33:17.05 as I mentioned earlier,
00:33:20.19 has one of the wedges cut with the optic axis,
00:33:26.03 the crystallographic axis of the wedge,
00:33:30.01 at an oblique angle,
00:33:31.15 and that was a clever thing on his part,
00:33:35.00 because that then put the effective
00:33:39.03 focal point for the prism
00:33:41.10 where the two beams,
00:33:43.15 the e and the o beams,
00:33:46.20 would come together
00:33:49.03 into the back focal plane of the objective,
00:33:50.11 while the prism itself
00:33:52.15 was outside of the objective,
00:33:54.04 and then the same thing was done on the condenser side,
00:33:56.05 so you didn't necessarily
00:33:58.14 have to have the prism
00:34:00.29 right exactly at the front focal plane of the condenser.
00:34:03.20 Now, there are other schemes
00:34:05.19 for how to build these prisms, today,
00:34:07.08 that the different manufacturers have developed
00:34:09.24 because there's licensing problems, right?
00:34:11.21 And so you can kind of get to the same result
00:34:14.10 as I diagrammed here,
00:34:16.04 for the basic concepts,
00:34:18.02 but use slightly different prism arrangements,
00:34:22.16 but the overall effect of it is the
00:34:26.28 same effects that I described in image formation.
00:34:29.10 Okay.
00:34:31.05 Now, the addition of retardation
00:34:35.16 between the two beams,
00:34:37.07 either in the plus or the minus direction,
00:34:40.03 is kind of...
00:34:42.05 the equations for it are down here,
00:34:44.06 because the prisms and the compensator
00:34:47.15 have their crystallographic axes at 45 degrees,
00:34:50.08 in the analyzer or polarizer direction,
00:34:52.14 then the equation for the intensity through the analyzer
00:34:56.07 are given by this sine squared
00:34:58.13 of the retardation of the compensator
00:35:00.26 plus the retardation of the specimen edge
00:35:03.09 divided by two,
00:35:05.10 and the background light intensity
00:35:08.24 is just the sine squared
00:35:10.22 of the retardation of the...
00:35:15.06 measured in radians
00:35:16.26 -- that's what delta means,
00:35:18.23 measured in radians --
00:35:20.13 divided by 2.
00:35:21.23 And so I've made a plot, here,
00:35:23.17 of this sine squared function.
00:35:25.19 The solid line, here,
00:35:28.20 is the background light intensity
00:35:32.08 and the dotted line is the intensity for an edge,
00:35:36.26 and if it's a right-hand edge
00:35:38.23 it's brighter than the background
00:35:40.11 and if it's a left-hand edge,
00:35:41.27 you can see over here
00:35:44.05 that it's darker than the background,
00:35:46.02 and this is the variation that you get in light intensity
00:35:48.09 as you add more or less compensation.
00:35:51.21 Now, it turns out that with our cameras
00:35:53.22 and the way they work,
00:35:55.00 what's usually best to get the highest contrast...
00:35:58.09 is to take one of the edges
00:36:01.11 and make it maximally dark,
00:36:03.28 and then use your contrast enhancement capabilities
00:36:07.08 of your computer or camera or electronics
00:36:11.01 to brighten up the bright side of the image,
00:36:16.17 and that's the way this image was done, here,
00:36:19.20 and it took about a tenth of a wavelength
00:36:22.19 or a twentieth of a wavelength of retardation
00:36:25.11 in green light, 550 nanometers,
00:36:29.22 to make this image of my cheek cell.
00:36:35.15 And now you can see that
00:36:39.03 there are no halos anymore.
00:36:39.29 We have the dark and light edge of the nucleus
00:36:42.19 and we now can start to see
00:36:46.12 a lot of the very fine structures,
00:36:47.25 the tiny little particles
00:36:49.23 and so forth and so on
00:36:51.19 that high-resolution DIC offers us.

This Talk
Speaker: Ted Salmon
Audience:
  • Researcher
Recorded: July 2012
More Talks in Microscopy Series
All Talks in Microscopy Series

Talk Overview

Share

Differential Interference Contrast (sometimes known as Normarski microscopy) is a variation of polarization microscopy which generates a high contrast “shadow” image of a specimen. The mechanism of the DIC (Wollaston) prisms is discussed along with how to generate optimal contrast.

Questions

  1. A differential interference contrast microscope consists of a polarizer and analyzer and a single DIC prism located above the objective. True or False
  2. Which major feature of a DIC image is incorrect?
    1. In the direction of contrast, one edge of an object is bright and the other is dark
    2. Contrast is directional; orientations of the specimen that achieve minimal and maximal contrast occur with a rotation of 90 degrees (orthogonal).
    3. The center of a large uniform refractive index specimen will appear much brighter than the background.
    4. Each point is represented by two overlapping Airy disks; separation is typically ½ to 2/3rd of the Airy disk diameter
  3. The Wollaston Prism:
    1. Is located at the front plane of the condenser lens
    2. has its fast and slow axes oriented 45 degrees to the polarizer
    3. Resolves the plane polarized light into two orthogonal beams that traverse the specimen.
    4. Is used to change the wavelength of light
    5. A, B, C
    6. A, B, C, D
  4. A compensator in DIC microscopy:
    1. compensates for loss of light traveling through the DIC prisms
    2. Increases the brightness of the background and generates black and white contrast
    3. Extinguishes light that is phase shifted by the specimen
    4. Protects the camera from excess illumination
    5. Is usually located in the illumination path before the objective.

Answers

View Answers

Speaker Bio

Ted Salmon

Ted Salmon

Ted Salmon is a Distinguished Professor in the Biology Department at the University of North Carolina. His lab has pioneered techniques in video and digital imaging to study the assembly of spindle microtubules and the segregation of chromosomes during mitosis. Continue Reading

Playlist: Microscopy Series

Reader Interactions

Leave a Reply

Your email address will not be published. Required fields are marked *