Paper
18 December 2019 Features of spatial functions of image motion in crossed optical beams measured by large solar vacuum telescope
Author Affiliations +
Proceedings Volume 11208, 25th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics; 112082O (2019) https://doi.org/10.1117/12.2542282
Event: XXV International Symposium, Atmospheric and Ocean Optics, Atmospheric Physics, 2019, Novosibirsk, Russian Federation
Abstract
The spatial analysis of the wavefront distortions registered by the Shack-Hartmann sensor of the adaptive optics (AO) system of Large solar vacuum telescope have been performed. In the paper the results of analysis of spatial structure of the wavefront within the field of view ~35 arcsec are discussed. It is shown that the wavefront distortions formed within the field of view ~35 arcsec are not random. There are the repetitive hills of spatial crosscorrelation functions in the field of view at the same intervals for different space subapertures. It is shown that spatial crosscorrelation functions do not contain pronounced kernel for finding the exact position of the atmospheric layer contributing to significant distortions in the wavefront incident on the telescope aperture.
© (2019) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
P. G. Kovadlo and A. V. Kiselev "Features of spatial functions of image motion in crossed optical beams measured by large solar vacuum telescope", Proc. SPIE 11208, 25th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 112082O (18 December 2019); https://doi.org/10.1117/12.2542282
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KEYWORDS
Telescopes

Adaptive optics

Wavefront distortions

Wavefronts

Atmospheric optics

Atmospheric turbulence

Motion measurement

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