Dish Surface Holography and Dish Surface Optimization System
Tests
Hiroshige Yoshida
Caltech Submillimeter Observatory
The AUG11 and later versions of the Dish Surface Optimization System
(DSOS) control software provide various ways to modify the shape of
the primary mirror to test the FTS and OoF holography systems, as well
as the DSOS itself. After preparing and initializing the DSOS in the
standard way, a script
HOLOtester can be used to operate and
modify the behavior of the DSOS. Without any argument,
HOLOtester is identical to one of the regular observing scripts
DSOSfastagent. Optional arguments allow for the target length
of the standoffs to be changed from that determined by the past FTS
holography measurements for a particular elevation angle, either
relatively to the model or absolutely from the baseline length. The
change can be applied to each standoff, quadrant, or entire dish
surface using the Zernike polynomials (SEP11 and after). A few
examples are shown below.
To push out the standoff 52 by 25 μm, execute the
HOLOtester
script as follows:
-
HOLOtester 52@L+=25
To push out the quadrant 3 entirely by 25 μm, execute the
following:
-
HOLOtester Q3@L+=25
To add the defocus term of the Zernike polynomials (Z
20) with the
amplitude of 25 μm, execute the following:
-
HOLOtester Z2,0@L+=25
Note that all the relative correction terms, including the Zernike
polynomials, are additive. So for example, the above three
deformation can be combined as follows:
-
HOLOtester 52@L+=25 Q3@L+=25 Z2,0@L+=25
Please consult the help text of the
DSOScontrol program for
other argument options by executing the following:
-
DSOScontrol -h
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On 21 Feb 2012, 13:19.