Radiative transfer in the 4.3-micron CO2 band in the atmospheres of Venus and Mars under vibrational and rotational non-LTE conditions

Details Radiative transfer in the 4.3-micron CO2 band in the atmospheres of Venus and Mars under vibrational and rotational non-LTE conditions Radiative transfer in the 4.3-micron CO2 band in the atmospheres of Venus and Mars under vibrational and rotational non-LTE conditions

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kfnt....5...27o&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 5, July-Aug. 1989, p. 27-37. In Russian.

Computer Science

Atmospheric Models, Carbon Dioxide, Mars Atmosphere, Molecular Spectra, Radiative Transfer, Venus Atmosphere, Molecular Oscillations, Molecular Rotation, Nonequilibrium Thermodynamics, Spectral Bands, Thermodynamic Equilibrium

Scientific paper

A numerical solution to the problem of radiative transfer in the 4.3-micron CO2 band is obtained for the plane model atmospheres of Venus and Mars. The introduction of the individual source functions for certain rotational-vibrational transitions (the wideband approximation) is shown to increase the local maxima in the diurnal and nocturnal vertical profiles of the vibrational temperature of the 00(0)1 state as compared to those presented by Stepanova and Shved (1985).

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