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

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

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spie.5026..177m&link_type=abstract

Ninth Joint International Symposium on Atmospheric and Ocean Optics/Atmospheric Physics. Part I: Radiation Propagation in the At

Physics

Optics

Scientific paper

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.

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