Modeling Laser Guide Star Aberrations

Richard M. Clare; Marcos A. van Dam; Antonin H. Bouchez

doi:10.1364/AOPT.2007.ATuB5

Adaptive Optics: Analysis and Methods/Computational Optical Sensing and Imaging/Information Photonics/Signal Recovery and Synthesis Topical Meetings on CD-ROM
OSA Technical Digest (CD) (Optica Publishing Group, 2007),
paper ATuB5
•https://doi.org/10.1364/AOPT.2007.ATuB5

Modeling Laser Guide Star Aberrations

Richard M. Clare, Marcos A. van Dam, and Antonin H. Bouchez

Adaptive Optics: Methods, Analysis and Applications 2007

Vancouver Canada
18–20 June 2007
ISBN: 1-55752-838-1

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Tomographic Wavefront Sensing (ATuB)

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R. M. Clare, M. A. van Dam, and A. H. Bouchez, "Modeling Laser Guide Star Aberrations," in Adaptive Optics: Analysis and Methods/Computational Optical Sensing and Imaging/Information Photonics/Signal Recovery and Synthesis Topical Meetings on CD-ROM, OSA Technical Digest (CD) (Optica Publishing Group, 2007), paper ATuB5.

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Abstract

When using a laser guide star (LGS) adaptive optics system, quasi-static aberrations are observed between the measured wavefronts from the LGS wavefront sensor (WFS) and the natural guide star WFS. We model these LGS aberrations.

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