Line-by-line radiative excitation model for the non-equilibrium atmosphere - Application to CO2 15-microns emission

Details Line-by-line radiative excitation model for the non-equilibrium atmosphere - Application to CO2 15-microns emission Line-by-line radiative excitation model for the non-equilibrium atmosphere - Application to CO2 15-microns emission

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jgr....9718083w&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 97, no. D16, p. 18,083-18,117.

Physics

60

Atmospheric Models, Carbon Dioxide, Infrared Radiation, Molecular Excitation, Radiative Transfer, Emission Spectra, Thermodynamic Equilibrium

Scientific paper

A new line-by-line algorithm for radiative excitation in infrared bands in a nonlocal thermodynamic equilibrium planetary atmosphere is described. A predictive model for the terrestrial CO2 15-microns emission that incorporates this generic algorithm is developed. The model is validated by comparing its results with emission spectra obtained in a limb-scanning rocket experiment.

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