Modeling of radiation intensity fluctuations during stellar occultations by Earth's atmosphere

Dmitri A. Marakassov; Andrey N. Shesternin

doi:10.1117/12.497201

27 March 2003 Modeling of radiation intensity fluctuations during stellar occultations by Earth's atmosphere

Dmitri A. Marakassov, Andrey N. Shesternin

Proceedings Volume 5026, Ninth Joint International Symposium on Atmospheric and Ocean Optics/Atmospheric Physics. Part I: Radiation Propagation in the Atmosphere and Ocean; (2003) https://doi.org/10.1117/12.497201
Event: Ninth Joint International symposium on Atmospheric and Ocean Optics, 2002, Tomsk, Russian Federation

Abstract

Two methods of radiation intensity fluctuations modeling during stellar occultations by Earth's atmosphere are suggested. Vertical anisotropy of inhomogeneities and ray path distortion due to macroscopic spherical anisotrropy of atmosphere are taken into account. Some numerical results are discussed.

Citation Download Citation

Dmitri A. Marakassov and Andrey N. Shesternin "Modeling of radiation intensity fluctuations during stellar occultations by Earth's atmosphere", Proc. SPIE 5026, Ninth Joint International Symposium on Atmospheric and Ocean Optics/Atmospheric Physics. Part I: Radiation Propagation in the Atmosphere and Ocean, (27 March 2003); https://doi.org/10.1117/12.497201

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