Paper
13 December 2018 "The first light" for the system of inputting the elements of AO into the optical path of LSVT
N. N. Botygina, D. Yu. Kolobov , P. G. Kovadlo , V. P. Lukin, S. A. Chuprakov, A. Yu. Shikhovtcev
Author Affiliations +
Proceedings Volume 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics; 108332S (2018) https://doi.org/10.1117/12.2504689
Event: XXIV International Symposium, Atmospheric and Ocean Optics, Atmospheric Physics, 2018, Tomsk, Russian Federation
Abstract
This paper describes the features of the two-mirror adaptive system for correcting atmospheric disturbances of the Large Solar Vacuum Telescope, developed with allowance for the correction of instrumental vibrations of telescopes in a wide amplitude-frequency range with an open siderostat supply mirror. Correction of the general slopes of the light wave front and its deformations is carried out separately. The adaptive optical system is designed to work with extended light sources (the Sun), which have a low contrast of image details.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
N. N. Botygina, D. Yu. Kolobov , P. G. Kovadlo , V. P. Lukin, S. A. Chuprakov, and A. Yu. Shikhovtcev ""The first light" for the system of inputting the elements of AO into the optical path of LSVT", Proc. SPIE 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 108332S (13 December 2018); https://doi.org/10.1117/12.2504689
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Cited by 2 scholarly publications.
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KEYWORDS
Mirrors

Telescopes

Image quality

Wavefronts

Adaptive optics

Sensors

Image sensors

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