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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02 June 2021
A Correction to this paper has been published: https://doi.org/10.1007/s11182-021-02338-x
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 11, pp. 109–114, November, 2020.
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Kovadlo, P.G., Shikhovtsev, A.Y., Kopylov, E.A. et al. Study of the Optical Atmospheric Distortions using Wavefront Sensor Data. Russ Phys J 63, 1952–1958 (2021). https://doi.org/10.1007/s11182-021-02256-y
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DOI: https://doi.org/10.1007/s11182-021-02256-y