An inverse problem of the photometry of solar radiation reflected by an optically thick planetary atmosphere. III - Remote sensing of minor gaseous components and atmospheric aerosol

Details An inverse problem of the photometry of solar radiation reflected by an optically thick planetary atmosphere. III - Remote sensing of minor gaseous components and atmospheric aerosol An inverse problem of the photometry of solar radiation reflected by an optically thick planetary atmosphere. III - Remote sensing of minor gaseous components and atmospheric aerosol

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kosis..30..212u&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 30, no. 2, Mar.-Apr. 1992, p. 212-225. In Russian.

Physics

Optics

Aerosols, Atmospheric Composition, Atmospheric Optics, Optical Thickness, Planetary Atmospheres, Atmospheric Scattering, Remote Sensing, Solar Planetary Interactions, Solar Radiation, Weighting Functions

Scientific paper

Attention is given to the application of the inverse problem formulated by Ustinov (1991) to the remote sensing of minor gaseous components and aerosol in the planetary atmosphere on the basis of observational data on reflected solar radiation. The radiative transfer equation is considered in a two-component medium consisting of the background molecular atmosphere and the atmospheric component being sounded. General expressions that describe variations of the intensity of the outgoing radiation due to variations of the extinction coefficient and scattering phase function of the component sounded are obtained. These expressions are used to formulate the inverse problems of the retrieval of the minor gaseous component mixing ratio, volume extinction coefficient of scattering aerosol, and microphysical parameters of aerosol particles. Expressions for weighting functions of the appropriate linearized inverse problems are obtained.

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