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Proceedings Paper

Deformable secondary mirrors for the LBT adaptive optics system
Author(s): H. M. Martin; G. Brusa Zappellini; B. Cuerden; S. M. Miller; A. Riccardi; B. K. Smith
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Paper Abstract

We describe the manufacture of thin shells for the deformable secondary mirrors of the LBT adaptive optics system. The secondary mirrors are thin shells, 910 mm in diameter and 1.6 mm thick. Each mirror will have its shape controlled by 672 voice-coil actuators. The main requirement for manufacture of the shell is smoothness on scales too small to be adjusted by the actuators. An additional requirement is that the rear surface match the reference body within 30 μm peak-to-valley. A technique was developed for producing smooth surfaces on the very aspheric surfaces of the shells. We figure the optical surfaces on a thick disk of Zerodur, then turn the disk over and thin it to 1.6 mm from the rear surface. Figuring is done primarily with a 30 cm diameter stressed lap, which bends actively to match the local curvature of the aspheric surface. For the thinning operation, the mirror is blocked with pitch, optical surface down, onto a granite disk with a matching convex surface. Because the shell may bend during the blocking operation and as its thickness is reduced to 1.6 mm, figuring of the rear surface is guided by precise thickness measurements over the surface of the shell. This method guarantees that both surfaces of the finished shell will satisfy their requirements when corrected with small actuator forces. Following the thinning operation, we edge the shell to its final dimensions, remove it from the blocking body, and coat the rear surface with aluminum to provide a set of conductive plates for capacitive sensors.

Paper Details

Date Published: 27 June 2006
PDF: 10 pages
Proc. SPIE 6272, Advances in Adaptive Optics II, 62720U (27 June 2006); doi: 10.1117/12.672698
Show Author Affiliations
H. M. Martin, Steward Observatory, Univ. of Arizona (United States)
G. Brusa Zappellini, Large Binocular Telescope Observatory, Univ. of Arizona (United States)
B. Cuerden, Steward Observatory, Univ. of Arizona (United States)
S. M. Miller, Steward Observatory, Univ of Arizona (United States)
A. Riccardi, INAF, Osservatorio Astrofisico di Arcetri (Italy)
B. K. Smith, Steward Observatory, Univ. of Arizona (United States)

Published in SPIE Proceedings Vol. 6272:
Advances in Adaptive Optics II
Brent L. Ellerbroek; Domenico Bonaccini Calia, Editor(s)

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