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Proceedings Paper

Simulation of pupil-plane observation of angle-of-arrival fluctuations in daytime turbulence
Author(s): Amokrane Berdja; Abdenour Irbah; Julien Borgnino; Francois Martin
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Paper Abstract

High angular resolution observations of the sun are limited by atmospheric turbulence. The MISOLFA seeing monitor (still under construction) is developed to obtain spatial and temporal statistical properties of optical turbulence by analyzing local motions observed on solar edge images. The solar flying shadows used for angle-of-arrival spatio-temporal analysis are observed in the pupil plane image by mean of a rectangular thin slit positioned on the solar edge image. A numerical simulation of the light propagation in both the atmospheric turbulence medium and the MISOLFA optical system is carried out studying the relation of the measured intensity variations in the pupil plane to angle-of-arrival fluctuations in the non-isoplanatic case. First results are presented and discussed.

Paper Details

Date Published: 6 February 2004
PDF: 11 pages
Proc. SPIE 5237, Optics in Atmospheric Propagation and Adaptive Systems VI, (6 February 2004); doi: 10.1117/12.510997
Show Author Affiliations
Amokrane Berdja, CRAAG/Observatoire d'Alger (Algeria)
Abdenour Irbah, CRAAG/Observatoire d'Alger (Algeria)
Julien Borgnino, Univ. de Nice-Sophia Antipolis (France)
Francois Martin, Univ. de Nice-Sophia Antipolis (France)


Published in SPIE Proceedings Vol. 5237:
Optics in Atmospheric Propagation and Adaptive Systems VI
John D. Gonglewski; Karin Stein, Editor(s)

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