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29 January 2002 Estimation of turbulence parameters from solar observations
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Abstract
The one-dimensional point spread function for long-exposure frames of the whole system atmosphere - instrument is calculated from solar limb observations using data recorded at OCA Observatory (France). It is then compared to the theoretical one deduced from the Von Karman model and various wave-front structure functions. Good agreement is found allowing to deduce the spatial coherence outer scale L0 and the Fried parameter r0.
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Lyes Lakhal, Abdanour Irbah, Claude Aime, Julien Borgnino, and Francois Martin "Estimation of turbulence parameters from solar observations", Proc. SPIE 4538, Optics in Atmospheric Propagation and Adaptive Systems IV, (29 January 2002); https://doi.org/10.1117/12.454397
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