Enviar artigo por via de e-mail Development of the Model of Turbulent Atmosphere at the Large Solar Vacuum Telescope Site as Applied to Image Adaptation
- Autores: Kovadlo P.G.1, Lukin V.P.2, Shikhovtsev A.Y.1
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Afiliações:
- Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences
- V.E. Zuev Institute of Atmospheric Optics, Siberian Branch, Russian Academy of Sciences
- Edição: Volume 32, Nº 2 (2019)
- Páginas: 202-206
- Seção: Optical Instrumentation
- URL: https://journals.rcsi.science/1024-8560/article/view/188740
- DOI: https://doi.org/10.1134/S1024856019020076
- ID: 188740
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Resumo
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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Sobre autores
P. Kovadlo
Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences
Autor responsável pela correspondência
Email: kovadlo2006@rambler.ru
Rússia, Irkutsk, 664033
V. Lukin
V.E. Zuev Institute of Atmospheric Optics, Siberian Branch, Russian Academy of Sciences
Autor responsável pela correspondência
Email: lukin@iao.ru
Rússia, Tomsk, 634055
A. Shikhovtsev
Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences
Email: lukin@iao.ru
Rússia, Irkutsk, 664033
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