Journal
RUSSIAN PHYSICS JOURNAL
Volume 63, Issue 11, Pages 1952-1958Publisher
SPRINGER
DOI: 10.1007/s11182-021-02256-y
Keywords
telescope; wavefront; Fried’ s radius; turbulence
Categories
Funding
- Russian Science Foundation [19-79-00061]
- Fundamental Scientific Research Program [II.16]
- [075-15-2019-628]
- Russian Science Foundation [19-79-00061] Funding Source: Russian Science Foundation
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This paper studies the optical turbulence structure at the Large Solar Vacuum Telescope of the Baikal Astrophysical Observatory, presenting results on wavefront distortions and discussing the possibilities of detecting layers with enhanced optical turbulence intensity in the atmosphere. Altitudes of the atmospheric turbulent layers within the boundary layer are estimated.
The paper studies the optical turbulence structure at the Large Solar Vacuum Telescope of the Baikal Astrophysical Observatory. Some results on the study of the wavefront distortions are given to expand the data archive. The possibilities of detecting layers with enhanced optical turbulence intensity in the atmosphere are discussed. The altitudes of the atmospheric turbulent layers within the boundary layer are estimated.
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