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.
Keywords:turbulence effective turbulence velocity effective turbulence height
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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