Analysis, Interpretation, and Modeling of Mars Dayglow Spectra

Details Analysis, Interpretation, and Modeling of Mars Dayglow Spectra Analysis, Interpretation, and Modeling of Mars Dayglow Spectra

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpico1447.9071h&link_type=abstract

Third International Workshop on The Mars Atmosphere: Modeling and Observations, held November 10-13, 2008 in Williamsburg, Virgi

Physics

Scientific paper

Simultaneous analysis of data from the Mars Express and Mariner 6, 7,
and 9 missions has better defined the altitude profiles of ultraviolet
dayglow emissions, providing more demanding challenges to models of the
Mars atmosphere from 80 to 200 km.

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