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Proceedings Paper

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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Paper 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.

Paper Details

Date Published: 13 December 2018
PDF: 6 pages
Proc. SPIE 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 1083318 (13 December 2018); doi: 10.1117/12.2503829
Show Author Affiliations
A. Yu. Shikhovtsev, Institute of Solar-Terrestrial Physics of the SB RAS (Russian Federation)
P. G. Kovadlo, Institute of Solar-Terrestrial Physics of the SB RAS (Russian Federation)
A. V. Kiselev, Institute of Solar-Terrestrial Physics of the SB RAS (Russian Federation)
D. Y. Kolobov, Institute of Solar-Terrestrial Physics of the SB RAS (Russian Federation)
I. V. Russkih, Institute of Solar-Terrestrial Physics of the SB RAS (Russian Federation)
V. E. Tomin, Institute of Solar-Terrestrial Physics of the SB RAS (Russian Federation)
M. Yu. Shikhovtsev, Irkutsk State Univ. (Russian Federation)


Published in SPIE Proceedings Vol. 10833:
24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics
Gennadii G. Matvienko; Oleg A. Romanovskii, Editor(s)

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