Use of a neural network to control an adaptive optics system for an astronomical telescope

Details Use of a neural network to control an adaptive optics system for an astronomical telescope Use of a neural network to control an adaptive optics system for an astronomical telescope

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991natur.351..300s&link_type=abstract

Nature (ISSN 0028-0836), vol. 351, May 23, 1991, p. 300-302. Research supported by USAF and U.S. Navy.

Physics

Optics

20

Adaptive Optics, Neural Nets, Seeing (Astronomy), Telescopes, Atmospheric Turbulence, Point Spread Functions, Reference Stars, Wave Front Reconstruction

Scientific paper

A neural network has been applied to measure optical phase distortion induced by atmospheric turbulence in images of Vega obtained with the 1.5 m single-mirror telescope at the Starfire Optical Range near Albuquerque. The experimental results agree well with phase reconstructions obtained simultaneously with a conventional wave-front sensor.

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