Potential of High Resolution Mid-Infrared Heterodyne Spectroscopy to Study the Martian Atmosphere

Details Potential of High Resolution Mid-Infrared Heterodyne Spectroscopy to Study the Martian Atmosphere Potential of High Resolution Mid-Infrared Heterodyne Spectroscopy to Study the Martian Atmosphere

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpico1447.9050s&link_type=abstract

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

Physics

Scientific paper

Infrared heterodyne spectroscopy at spectral resolutions of > 10^5
allows retrieval of many physical parameters from fully resolved
individual lines. The Cologne THIS and its specific application to the
atmosphere of Mars will be presented.

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