Development of the Model of Turbulent Atmosphere at the Large Solar Vacuum Telescope Site as Applied to Image Adaptation


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The work is aimed at the improvement of the model of a turbulent atmosphere at the Large Solar Vacuum Telescope site using the analysis of the energy turbulence spectrum in a wide range of frequencies and deformations of the vertical profile of the structure parameter of the refractive index of air in the atmospheric boundary layer (up to 1 km), depending on the energy of the surface turbulence.

作者简介

P. Kovadlo

Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences

编辑信件的主要联系方式.
Email: kovadlo2006@rambler.ru
俄罗斯联邦, Irkutsk, 664033

V. Lukin

V.E. Zuev Institute of Atmospheric Optics, Siberian Branch, Russian Academy of Sciences

编辑信件的主要联系方式.
Email: lukin@iao.ru
俄罗斯联邦, Tomsk, 634055

A. Shikhovtsev

Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences

Email: lukin@iao.ru
俄罗斯联邦, Irkutsk, 664033

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