Paper
19 November 2015 Space-time transformation sky brightness at a horizontal position of the sun
Author Affiliations +
Proceedings Volume 9680, 21st International Symposium Atmospheric and Ocean Optics: Atmospheric Physics; 968017 (2015) https://doi.org/10.1117/12.2205339
Event: XXI International Symposium Atmospheric and Ocean Optics. Atmospheric Physics, 2015, Tomsk, Russian Federation
Abstract
This report discusses some simulation results of the angular distribution of brightness of the sky in the case of molecular scattering in the atmosphere for the benefit of the study of space-time changes of this distribution during the civil twilight.
© (2015) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Viktor P. Galileiskii, Alexey I. Elizarov, Dmitrii V. Kokarev, and Aleksandr M. Morozov "Space-time transformation sky brightness at a horizontal position of the sun", Proc. SPIE 9680, 21st International Symposium Atmospheric and Ocean Optics: Atmospheric Physics, 968017 (19 November 2015); https://doi.org/10.1117/12.2205339
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KEYWORDS
Sun

Atmospheric particles

Atmospheric modeling

Atmospheric optics

Scattering

Light scattering

Solar radiation models

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