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Vertical profiles of Mars 1.27 μm O 2 dayglow from MRO CRISM limb Spectra: Seasonal/global behaviors, comparisons to LMDGCM simulations, and a global definition for Mars water vapor profiles

R. Todd Clancy,Michael D. Smith,Franck Lefèvre,Timothy H. McConnochie,Brad J. Sandor,Michael J. Wolff,Steven W. Lee,Scott L. Murchie,Anthony D. Toigo,Hari Nair,Thomas Navarro

Icarus（2017）

Cited 42|Views85
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Abstract
•O2 dayglow emission profiles mapped for the first time in the Mars atmosphere.•Collisional de-excitation rate coefficient for Mars O2 emission found to be 3x lower.•Mars vertical profile of water vapor mapped in season and latitude for first time.•Mars cloud processes confine water more strongly to summer high latitudes.
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Key words
mars water vapor profiles,mro crism limb spectra,lmdgcm simulations
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