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Atmospheric and Oceanic Optics

2018 year, number 11

The development of the model of turbulent atmosphere on the astroplatform of Large Solar Vacuum Telescope as applied to image adaptation

P.G. Kovadlo1, V.P. Lukin2, A.Yu. Shikhovtsev1
1Institute of Solar-Terrestrial Physics of the Siberian Branch of the RAS, 664033, Irkutsk, 126a, Lermontova str
2V.E. Zuev Institute of Atmospheric Optics of Siberian Branch of the Russian Academy of Science, 1, Academician Zuev square, Tomsk, 634055, Russia
Keywords: турбулентность, эффективная скорость турбулентных течений, эффективная высота турбулентности, turbulence, effective turbulence velocity, effective turbulence height


The work is aimed at the improvement of the model of 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 characteristic of the air refraction index in the atmospheric boundary layer (up to 1 km) depending on the surface turbulence energy.