Share Email Print
cover

Proceedings Paper

First light on an edge-matched segmented adaptive mirror at the McMath Telescope
Author(s): Anthony D. Gleckler; James Roger P. Angel; Donald W. McCarthy; Bobby Lee Ulich; Kent P. Pflibsen; Peter L. Wizinowich
Format Member Price Non-Member Price
PDF $14.40 $18.00

Paper Abstract

The first astronomical results using a seven segment edge-matched adaptive mirror are presented. The mirror is a prototype for adaptive secondary mirrors, consisting of seven flat hexagonal mirrors, with inductive edge sensors to measure piston errors, and piezoelectric actuators. A Hartmann- Shack wavefront sensor uses the visible light for centroiding information while the IR image is formed on a 58 X 62 InSb array at 2.2 microns. In addition, a number of mathematical models are presented that illustrate how well the system should perform when correcting atmospheric turbulence.

Paper Details

Date Published: 31 May 1994
PDF: 13 pages
Proc. SPIE 2201, Adaptive Optics in Astronomy, (31 May 1994); doi: 10.1117/12.176072
Show Author Affiliations
Anthony D. Gleckler, Kaman Aerospace Corp. (United States)
James Roger P. Angel, Univ. of Arizona Steward Observatory (United States)
Donald W. McCarthy, Univ. of Arizona Steward Observatory (United States)
Bobby Lee Ulich, Kaman Aerospace Corp. (United States)
Kent P. Pflibsen, Kaman Aerospace Corp. (United States)
Peter L. Wizinowich, W.M. Keck Observatory (United States)


Published in SPIE Proceedings Vol. 2201:
Adaptive Optics in Astronomy
Mark A. Ealey; Fritz Merkle, Editor(s)

© SPIE. Terms of Use
Back to Top