The O(1 S) 297.2-nm Dayglow Emission: A Tracer of CO2 Density Variations in the Martian Lower Thermosphere
Author:
Affiliation:
1. LPAP, STAR Institute; Université de Liège; Liege Belgium
2. Royal Observatory of Belgium; Brussels Belgium
3. LASP; University of Colorado Boulder; Boulder CO USA
Funder
Fonds De La Recherche Scientifique - FNRS
Federaal Wetenschapsbeleid
European Space Agency
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics
Link
http://onlinelibrary.wiley.com/wol1/doi/10.1029/2018JE005709/fullpdf
Reference56 articles.
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2. Room temperature photoabsorption cross section measurements of CO2 between 91,000 and 115,000 cm−1;Archer;Journal of Quantitative Spectroscopy and Radiative Transfer,2013
3. Mariner 6 and 7 ultraviolet spectrometer experiment: Upper atmosphere data;Barth;Journal of Geophysical Research,1971
4. Mariner 9 ultraviolet spectrometer experiment: Mars airglow spectroscopy and variations in Lyman alpha;Barth;Icarus,1972
5. Temperature dependence of the quenching of O(1S) by simple inorganic molecules;Capetanakis;The Journal of Chemical Physics,1993
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