Share Email Print
cover

Proceedings Paper

Modeling of radiation intensity fluctuations during stellar occultations by Earth's atmosphere
Author(s): Dmitri A. Marakassov; Andrey N. Shesternin
Format Member Price Non-Member Price
PDF $14.40 $18.00

Paper 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.

Paper Details

Date Published: 27 March 2003
PDF: 6 pages
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); doi: 10.1117/12.497201
Show Author Affiliations
Dmitri A. Marakassov, Institute of Atmospheric Optics (Russia)
Andrey N. Shesternin, Institute of Atmospheric Optics (Russia)


Published in SPIE Proceedings Vol. 5026:
Ninth Joint International Symposium on Atmospheric and Ocean Optics/Atmospheric Physics. Part I: Radiation Propagation in the Atmosphere and Ocean
Gennadii G. Matvienko; Vladimir P. Lukin, Editor(s)

© SPIE. Terms of Use
Back to Top