A Method of Determining Optical Turbulence Characteristics by the Line of Sight of an Astronomical Telescope.

Autor: Shikhovtsev, A. Yu.
Zdroj: Atmospheric & Oceanic Optics; Jun2022, Vol. 35 Issue 3, p303-309, 7p
Abstrakt: A modified method of determining vertical profiles of optical turbulence characteristics is proposed. Based on data of observations on the Large Solar Vacuum Telescope, vertical profiles of the dimensionless turbulence parameter and structure constant of air refractive index fluctuations are obtained. Optical turbulence profiles are analyzed. It is found that the effective turbulence height at the site of the Large Solar Vacuum Telescope is close to 2000 m. [ABSTRACT FROM AUTHOR]
Databáze: Complementary Index
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