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Proceedings Paper

University of Hawaii adaptive optics system: I. General approach
Author(s): Francois J. Roddier; J. Elon Graves; Daniel L. McKenna; Malcolm J. Northcott
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Paper Abstract

The adaptive optics system being developed to sharpen images produced by telescopes at Mauna Kea is discussed. An approach based on new components developed and optimized for astronomical applications is described. The approach is limited to low-order wavefront compensation and is used for image stabilization. Avalanche photodiodes were used as sensors and reference stars were employed for sensing wavefront errors in a novel sensing technique based on wavefront curvature measurements. The instrument is described and expected performance is discussed.

Paper Details

Date Published: 1 December 1991
PDF: 6 pages
Proc. SPIE 1542, Active and Adaptive Optical Systems, (1 December 1991); doi: 10.1117/12.48812
Show Author Affiliations
Francois J. Roddier, Univ. of Hawaii/Manoa (United States)
J. Elon Graves, Univ. of Hawaii/Manoa (United States)
Daniel L. McKenna, Univ. of Hawaii/Manoa (United States)
Malcolm J. Northcott, Univ. of Hawaii/Manoa (United States)

Published in SPIE Proceedings Vol. 1542:
Active and Adaptive Optical Systems
Mark A. Ealey, Editor(s)

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