Paper
19 November 2015 The formation of the sky brightness with horizon position of the sun
Author Affiliations +
Proceedings Volume 9680, 21st International Symposium Atmospheric and Ocean Optics: Atmospheric Physics; 96803L (2015) https://doi.org/10.1117/12.2205504
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 during the civil twilight with solar zenith angles 90 ° - 94 °.
© (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 "The formation of the sky brightness with horizon position of the sun", Proc. SPIE 9680, 21st International Symposium Atmospheric and Ocean Optics: Atmospheric Physics, 96803L (19 November 2015); https://doi.org/10.1117/12.2205504
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KEYWORDS
Sun

Solar radiation

Atmospheric optics

Atmospheric particles

Scattering

Atmospheric modeling

Earth's atmosphere

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