Stochastic models of hot planetary and satellite coronas: Total water loss in the Martian atmosphere

Details Stochastic models of hot planetary and satellite coronas: Total water loss in the Martian atmosphere Stochastic models of hot planetary and satellite coronas: Total water loss in the Martian atmosphere

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sosyr..41..103s&link_type=abstract

Solar System Research, Volume 41, Issue 2, pp.103-108

Physics

2

96.12.Jt, 96.30.Gc, Atmospheres, Mars

Scientific paper

Estimates of the total thermal and nonthermal losses of hydrogen and the total nonthermal loss of oxygen from the atmosphere of Mars are discussed, and their ratio is analyzed. It is shown that an H to O ratio of 2:1 has not been achieved in any of the current models of various authors. The closest ratio, H:O = 4:1, has been obtained by Krestyanikova and Shematovich (2006) in the model of formation of a hot oxygen corona.

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