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13 December 2018 Development of a model of atmospheric turbulence at Baikal Astrophysical Observatory site of the Large Solar Vacuum Telescope
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Proceedings Volume 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics; 108331P (2018) https://doi.org/10.1117/12.2504347
Event: XXIV International Symposium, Atmospheric and Ocean Optics, Atmospheric Physics, 2018, Tomsk, Russian Federation
Abstract
The Baikal Astrophysical Observatory of Institute Solar- Terrestrial Physics of Siberian Branch of Russian Academy Sciences is located at an altitude of about 700 meter above sea level on the shore of Lake Baikal, Russian Federation. Large Solar Vacuum Telescope (LSVT) is the main telescope of the Baikal Astrophysical Observatory. We develop models of vertical profile of atmospheric turbulence (the refractive-index structure constant) and wind speed at the BAO for adaptive optical system design of LSVT. We also presented vertical profile wind speed and the refractive-index structure constant is obtained from NCEP/NCAR Reanalysis base.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
L. A. Bolbasova, A. Y. Shikhovtsev , P. G. Kovadlo, F. A. Avdeev , and V. P. Lukin "Development of a model of atmospheric turbulence at Baikal Astrophysical Observatory site of the Large Solar Vacuum Telescope", Proc. SPIE 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 108331P (13 December 2018); https://doi.org/10.1117/12.2504347
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