CO2 infrared bands in the Martian atmosphere

Details CO2 infrared bands in the Martian atmosphere CO2 infrared bands in the Martian atmosphere

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.185...53r&link_type=abstract

In ESA The Planet Mars p 53-57 (SEE N83-19673 09-91)

Computer Science

Numerical Analysis

Carbon Dioxide, Infrared Spectra, Mars (Planet), Planetary Atmospheres, Isotropy, Numerical Analysis, Photons, Spectrum Analysis

Scientific paper

To obtain the intensities of the 4.3 and 15 micron CO2 fundamental bands in the Martian atmosphere, a first order approximation model was developed. The numerical method is based on the diffusion approximation, showing reasonable results at heights where the mean free path of photons was less than the scale height of the atmosphere. Situations not very far from equilibrium are then considered. The method allows a first study of the deviations of the isotropy in the radiation field. This approximation takes directly into account the thermal and non-thermal excitation processes of CO2 and therefore the physical behavior of the corresponding emissions can be easily analyzed.

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