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Proceedings Paper

Wavefront reconstruction methods for a natural guide star adaptive optics application to the Keck Telescope
Author(s): Mark H. Milman; Laura Needels; David C. Redding
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Paper Abstract

This paper investigates and compares wavefront sensing options for a proposed natural guide star adaptive optics upgrade for the Keck telescope. The methods of curvature sensing and slope sensing with a Hartmann sensor are compared. A curvature sensor model is developed that includes nonlinear, diffraction, and noise effects. The analytical model is validated in simulation using the Keck optical prescription parameters. A comprehensive treatment of estimation/reconstruction is presented and used for the Hartmann sensor/curvature sensor comparisons.

Paper Details

Date Published: 31 May 1994
PDF: 12 pages
Proc. SPIE 2201, Adaptive Optics in Astronomy, (31 May 1994); doi: 10.1117/12.176037
Show Author Affiliations
Mark H. Milman, Jet Propulsion Lab. (United States)
Laura Needels, Jet Propulsion Lab. (United States)
David C. Redding, Jet Propulsion Lab. (United States)


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

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