Mariner 6: Origin of Mars Ionized Carbon Dioxide Ultraviolet Spectrum

Details Mariner 6: Origin of Mars Ionized Carbon Dioxide Ultraviolet Spectrum Mariner 6: Origin of Mars Ionized Carbon Dioxide Ultraviolet Spectrum

Mar 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970sci...167.1490d&link_type=abstract

Science, Volume 167, Issue 3924, pp. 1490-1491

Physics

7

Scientific paper

The predicted intensities of the ionized carbon dioxide (CO2{}+) emission feature at 2890 angstroms and the Fox-Duffendack-Barker bands are 5.2 and 19.9 kilorayleighs, respectively, for a vertical column. Direct photoionization of carbon dioxide by solar radiation contributes 3.5 and 4.1 kilorayleighs, respectively, and fluorescent scattering by CO2{}+, 1.6 and 15.3 kilorayleighs, respectively. Photoelectron impacts are less important.

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