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

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Abstract—

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.

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ACKNOWLEDGMENTS

Some results were obtained using the Large Solar Vacuum Telescope (http://ckp-rf.ru/usu/200615/) with funding of Basic Research program II.16. The analysis of the structural features of optical turbulence was supported by the Russian Foundation for Basic Research (project no. 18-35-00033). Optical and acoustic measurements were financially supported by the Russian Science Foundation (grant no. 17-79-20 077).

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Authors and Affiliations

  1. Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences, 664033, Irkutsk, Russia

    P. G. Kovadlo & A. Yu. Shikhovtsev

  2. V.E. Zuev Institute of Atmospheric Optics, Siberian Branch, Russian Academy of Sciences, 634055, Tomsk, Russia

    V. P. Lukin

Authors
  1. P. G. Kovadlo
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  2. V. P. Lukin
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  3. A. Yu. Shikhovtsev
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Corresponding authors

Correspondence to P. G. Kovadlo or V. P. Lukin.

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Translated by O. Ponomareva

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Kovadlo, P.G., Lukin, V.P. & Shikhovtsev, A.Y. Development of the Model of Turbulent Atmosphere at the Large Solar Vacuum Telescope Site as Applied to Image Adaptation. Atmos Ocean Opt 32, 202–206 (2019). https://doi.org/10.1134/S1024856019020076

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  • DOI: https://doi.org/10.1134/S1024856019020076

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