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Proceedings Paper

Automatic determination of atmospheric turbulence wind profiles using wavelets
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Paper Abstract

Adaptive optics devices in astronomy compensate the distortions introduced by the atmosphere in the quality and resolution of images taken by ground-based telescopes. The proper knowledge of the spatial and temporal behaviour of the atmospheric turbulence is crutial for optimizing the design of multiconjugate adaptive optics systems to satisfy the excellent image quality requirements of the new generation of large and extremelly large telescopes. Atmospheric turbulence monitoring is being carried out at astronomical sites using different techniques, being generalized SCIDAR one of the most popular. Generalized SCIDAR technique provides enough information to derive the vertical structure of the atmospheric turbulence (C2N(h)) as well as the velocity of the turbulent layers (Vtur(h)). In this work, we present a new and automatic method to derive Vtur(h) from generalized SCIDAR data based on wavelet analysis.

Paper Details

Date Published: 23 June 2006
PDF: 9 pages
Proc. SPIE 6267, Ground-based and Airborne Telescopes, 62671W (23 June 2006); doi: 10.1117/12.671267
Show Author Affiliations
B. García-Lorenzo, Instituto de Astrofísica de Canarias (Spain)
J. J. Fuensalida, Instituto de Astrofísica de Canarias (Spain)


Published in SPIE Proceedings Vol. 6267:
Ground-based and Airborne Telescopes
Larry M. Stepp, Editor(s)

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