The inverse thermal probe problem: to recover the vertical profile of the absorption coefficient of an optically active component of a planetary atmosphere from observing the emitted radiation.

Details The inverse thermal probe problem: to recover the vertical profile of the absorption coefficient of an optically active component of a planetary atmosphere from observing the emitted radiation. The inverse thermal probe problem: to recover the vertical profile of the absorption coefficient of an optically active component of a planetary atmosphere from observing the emitted radiation.

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990cosre..28..347u&link_type=abstract

Cosmic Res., Vol. 28, No. 3, p. 347 - 355

Computer Science

2

Planetary Atmospheres: Thermal Radiation, Planetary Atmospheres: Radiative Transfer

Scientific paper

The authors present a formulation of the inverse thermal problem of probing of a purely absorbing planetary atmosphere, allowing recovery of the vertical profile of the atmospheric component contributing to the thermal absorption of the atmosphere (and in this sense optically active component) in the observed spectral range. An expression for the kernel of the operator for the linearised inverse problem was obtained by two methods: by direct variation of the expression for the intensity of the emitted thermal radiation, and using the solutions of the direct and the conjugate problems of thermal radiation transfer. The results obtained can be applied to recover the vertical profile of the extinction coefficient of a purely absorbent aerosol and the ratio of the mixture of gas components.

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