Paper
21 February 2001 PSF estimate in compensated systems
Manuel Perez Cagigal, Vidal F. Canales
Author Affiliations +
Proceedings Volume 4150, Optical Remote Sensing of the Atmosphere and Clouds II; (2001) https://doi.org/10.1117/12.416972
Event: Second International Asia-Pacific Symposium on Remote Sensing of the Atmosphere, Environment, and Space, 2000, Sendai, Japan
Abstract
The resolution limit attainable by large ground-based telescopes is limited by the refraction index fluctuations of the turbulent atmosphere. To overcome this limitation Adaptive Optics systems measure and compensate atmospheric-induced distortions. When working in the visible, only a partial compensation is possible. We analyze the image formation process in these conditions. We provide a model for the wave front statistics, which allows a simple estimate of the instantaneous PSF. New deconvolution techniques could be developed by using this approximation.
© (2001) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Manuel Perez Cagigal and Vidal F. Canales "PSF estimate in compensated systems", Proc. SPIE 4150, Optical Remote Sensing of the Atmosphere and Clouds II, (21 February 2001); https://doi.org/10.1117/12.416972
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KEYWORDS
Wavefronts

Point spread functions

Adaptive optics

Telescopes

Atmospheric optics

Zernike polynomials

Statistical analysis

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