[Raytrace] Raytracing mirror support distortions (active optics)
Peter Chen
chen@stars.gsfc.nasa.gov
Fri, 07 Dec 2001 12:58:08 -0500
Hi:
Thought to tell the list of another project I'm interested in, although
I'm not sure how well it will work out. David Lewis has written an
excellent program called PLOP which is available from his site
http://www.eecg.toronto.edu/~lewis/. PLOP computes the optical surface
shape of a telescope under various support schemes (3 points, 9 points,
multiple rings, etc). It is an excellent program and very user friendly.
I thought it might be interesting to do raytracing for mirror under a
variety of support schemes. This is called 'active optics'. It is
especially applicable to large thin mirrors (a la Mel Bartels?). Acitve
support is the technique used by the European Southern Observatory in its
four 8 meter Very Large Telescopes, currently the biggest in the
world. The mirrors are thin and therefore very sensitive to how they are
supported. In fact, the VLT supports are cleverly designed to compensate
for astigmatism, spherical aberrations, and coma.
I wrote to David Lewis some time ago, and he kindly modified a PLOP
program to output mirror shapes in Zernike terms. I'm trying to see if it
is possible to use the PLOP generated Zernike terms and import them into
Zemax (or other programs) and do a raytrace. The ultimate aim, of course,
is to be able to adjust the support forces on a mirror to keep it at
optimal shape during observations.
Wish me luck. I'll try to keep the list informed of my progress.
P.C. Chen