The latitude variation of O2 dayglow and O3 abundance on Mars

Details The latitude variation of O2 dayglow and O3 abundance on Mars The latitude variation of O2 dayglow and O3 abundance on Mars

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...229..846t&link_type=abstract

Astrophysical Journal, Part 1, vol. 229, Apr. 15, 1979, p. 846-850.

Astronomy and Astrophysics

Astrophysics

17

Abundance, Dayglow, Latitude, Mars Atmosphere, Ozone, Atmospheric Models, Atmospheric Temperature, Emission Spectra, Mariner 9 Space Probe, Oxygen Spectra

Scientific paper

Spectroscopic observations of the Martian O2 dayglow near 1.27 microns directly show that the parent molecule, O3, has a strong latitude variation. These measurements give actual data on the equatorial concentrations, where Mariner gave only upper limits. The data also agree with a recent photochemical model, and the derived atmospheric temperature is in good agreement with this model.

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