Inverse theory for occultation measurements. I - Spectral inversion

Mathematics – Probability

Scientific paper

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Atmospheric Composition, Atmospheric Models, Environmental Monitoring, Occultation, Remote Sensing, Ozone, Probability Distribution Functions, Trace Contaminants

Scientific paper

Methods of solving the inverse problem for optical occultation measurements from a planet-orbiting satellite are examined. The possibilities of mapping the structure of the earth's stratosphere using the self-calibrating occultation principle are examined. The determination of contributions due to different atmospheric constituents in the occultation signal is investigated. The basic concepts of the occultation measurements are discussed and the principles of signal simulation are given. The theory of inversion problems is discussed, the inversion methods used are described, and results are compared. Inversion results for different star types and magnitudes are presented. The stellar occultation technique is a promising method of monitoring global vertical distributions of trace gases in the earth's atmosphere.

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