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Proceedings Paper

Adaptive optics: a general purpose system for astronomy
Author(s): Jean-Jacques Roland; Jean-Paul Gaffard; Pascal Jagourel; Corinne Boyer; Patrick Gosselin
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Paper Abstract

Since approximately 5 years, several experimental Adaptive Optics Systems have been tested on different astronomical sites. This paper describes a general purpose AOS designed for new or existing telescopes for diameters ranging from 2 to 4 meters. Investigations on actually available Adaptive Mirrors and Wavefront sensors are made. The use of a bimorph mirror and simplified Shack Hartmann is proposed. Results of simulation to evaluate the Strehl ratios for different wavelengths are given versus seeing conditions and star magnitudes. This leads to the conclusion that low cost, turn key AOS are a new attractive possibility for Astronomy.

Paper Details

Date Published: 31 May 1994
PDF: 19 pages
Proc. SPIE 2201, Adaptive Optics in Astronomy, (31 May 1994); doi: 10.1117/12.176083
Show Author Affiliations
Jean-Jacques Roland, Laserdot Groupe Aerospatiale (France)
Jean-Paul Gaffard, Laserdot Groupe Aerospatiale (France)
Pascal Jagourel, Laserdot Groupe Aerospatiale (France)
Corinne Boyer, Laserdot Groupe Aerospatiale (France)
Patrick Gosselin, Laserdot Groupe Aerospatiale (France)


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

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