Last updated: Fri Sep 8 16:51:48 HST 2000
Don Mickey
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This sketch shows part of the IVM optics. At the left is the field stop at the telescope focal plane. A square aperture 4.77 mm on a side, it selects an area on the sky that is 280 arc sec square. Behind (to the right in the figure) the field stop is a field lens which images the telescope aperture onto the collimator lens, at the right edge of this figure. Toward the center of the figure are the two liquid-crystal variable retarders (LVRs). The first one is oriented with its fast axis vertical, parallel to the sides of the field stop. The second retarder is rotated 45 degrees clockwise (as seen from the field stop, looking toward the right in this drawing). The analyzer, not shown here, is a polarizing beam splitter with its transmission axis vertical for the Data camera beam.
The LVRs are located in the f:12.8 diverging beam from the telescope focus, so rays from any field point fill a cone with a half-angle of about 0.04 radians. The telescope secondary obscuration means that the central part of the LVRs is not illuminated. In addition, the chief ray from a given field point has an angle of up to 0.003 radians from the optical axis of the system.
The LVRs consist of a layer of liquid crystal material a few microns
thick, contained between two fused silica plates. The elongated molecules
of the liquid crystal are aligned parallel to each other and nearly parallel
to the substrate, in their quiescent condition. The asymmetry of the molecules
causes the material to be birefringent. The construction of the retarders
is described in the Meadowlark
catalog page, which also has a cartoon cross section of the device.
When a voltage is applied, the molecules in the liquid crystal are rotated
about the fast axis of the retarder, reducing their apparent asymmetry
as seen by the incident light and thus reducing the birefringence. The
birefringence, however, depends on the angle of incidence, as shown in
the following drawing. This is a view from above, looking at two rays incident
on the first LVR.
The ray labeled A sees a larger birefringence than does the ray labeled
B.
Each image is scaled to the expected value, +/- 0.57735, plus and minus
a range of 0.04.
When these sets are demodulated, we get a 4 x 4 array of calibration
images, as shown below.
Some of the images here contain no information: the upper left one is an
arbitrary scale factor, and is set to all ones. The remainder of both the
first row and column contain zeros here, since we are interested in the
QUV terms at this point. The QQ, UU, VV diagonal terms are shown as 0.577
+/- 0.02; the rest are shown as 0.0 +/- 0.02. There is some field position
dependence in all the terms, particularly in the UV and VU terms which
reach amplitudes of about +/- 0.04 at the edges. The actual observed IVM
calibration matrix is very similar to this model.
Here
are the individual frames in the calibration set, scaled the same as above,
i.e. a range of 0.08 from black to white with a mean of 0.57735.
The derived cal matrix looks like this:
The main difference is that the diagonal terms now have essentially no
field variation, and the remaining field dependence is either horizontal
or at 45 degrees to the horizontal, i.e. along the slow axis of one of
the retarders.
The solution may be to arrange the retarders in a location where the
pupil is collimated, so that for any field point the chief ray is normal
to the retarder surface. Then even though the retardance varies over the
pupil, the variation is symmetric, averages to zero, and is the same for
all field points.