Numerical simulation of angular distribution of the scattered solar radiation brightness in the Earth’s atmosphere
V.P. Galileyskii, A.I. Grishin, A.M. Morozov
V.E. Zuev Institute of Atmospheric Optics of Siberian Branch, 1, Academician Zuev square, Tomsk, 634021, Russia
Keywords: field brightness of the sky, the Earth's atmosphere, scattering in the atmosphere, numerical simulation
Abstract
This paper considers the computational model to calculate the field of sky brightness in the atmosphere, caused by a single-scattered solar radiation in the visible range of the spectrum. The numerical simulation model of homogeneous layers of the atmosphere with altitude distribution coefficients of molecular and aerosol scattering and absorption is used. The calculation is performed in three spectral bands R, G, B, comparable to human vision and photographic recording.
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