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13 December 2018 Variations of the height optical turbulence profiles at the Baikal Astrophysical Observatory and the features of its deformations in latitudinal direction
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Proceedings Volume 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics; 1083318 (2018) https://doi.org/10.1117/12.2503829
Event: XXIV International Symposium, Atmospheric and Ocean Optics, Atmospheric Physics, 2018, Tomsk, Russian Federation
Abstract
The work discusses the optical turbulence structure and dynamics at the Baykal Astrophysical Observatory (BAO) site. The characteristics of the optical turbulence including Fried radius, isoplanatic angle are analyzed. Estimates of the variations of the height profiles of the air refraction index turbulent fluctuations at the Baykal Astrophysical Observatory are given. Using the mean height profile of the structure characteristic of the air refraction index turbulent fluctuations, diurnal variations of the Fried radius at the BAO site are estimated.
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A. Yu. Shikhovtsev, P. G. Kovadlo, A. V. Kiselev, D. Y. Kolobov, I. V. Russkih, V. E. Tomin, and M. Yu. Shikhovtsev "Variations of the height optical turbulence profiles at the Baikal Astrophysical Observatory and the features of its deformations in latitudinal direction", Proc. SPIE 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 1083318 (13 December 2018); https://doi.org/10.1117/12.2503829
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