First Detection of O2 Recombination Nightglow Emission at 1.27 µm in the Atmosphere of Mars with OMEGA/MEX and Comparison with Model

Details First Detection of O2 Recombination Nightglow Emission at 1.27 µm in the Atmosphere of Mars with OMEGA/MEX and Comparison with Model First Detection of O2 Recombination Nightglow Emission at 1.27 µm in the Atmosphere of Mars with OMEGA/MEX and Comparison with Model

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1884g&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1884

Computer Science

Scientific paper

OMEGA acquired night side limb profiles of the martian atmosphere. O2
emission at 1.27 µm is observed. These observations of O2 are
compared with LMD-GCM, showing that downward transport from the
thermosphere are occurring in the polar night.

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