Laser and Natural Guide Star Measured Turbulent Wavefront Correlation

Ruy Deron; Sylvain Laurent; Marc Séchaud; Gérard Rousset

doi:10.1364/ADOP.1995.FA1

Adaptive Optics
Technical Digest Series (Optica Publishing Group, 1995),
paper FA1
•https://doi.org/10.1364/ADOP.1995.FA1

Laser and Natural Guide Star Measured Turbulent Wavefront Correlation

Ruy Deron, Sylvain Laurent, Marc Séchaud, and Gérard Rousset

Adaptive Optics 1995

Garching Germany
2–6 October 1995
ISBN:

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Adaptive Optics Experimental Results (FA)

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R. Deron, S. Laurent, M. Séchaud, and G. Rousset, "Laser and Natural Guide Star Measured Turbulent Wavefront Correlation," in Adaptive Optics, Technical Digest Series (Optica Publishing Group, 1995), paper FA1.

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Abstract

The laser guide star concept was proposed for the application of adaptive optics in astronomy in order to overcome the problem of natural star requisite brightness which significantly limits the sky coverage [1, 2]. Recently, the adaptive optics compensation of turbulent wavefront using laser guide star has been demonstrated [3,4].

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