Physics
Scientific paper
Apr 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990angeo...8..251n&link_type=abstract
Annales Geophysicae (ISSN 0992-7689), vol. 8, April 1990, p. 251-256.
Physics
51
Hydrogen Atoms, Mars Atmosphere, Oxygen Atoms, Planetary Temperature, Upper Atmosphere, Venus Atmosphere, High Temperature Gases, Lyman Alpha Radiation, Mariner 5 Space Probe, Solar Wind, Ultraviolet Photometry, Planets, Hydrogen, Oxygen, Atmosphere, Venus, Mars, Optical Properties, Production Rate, Models, Solar Wind, Interactions, Coronas, Density, Spacecraft Observations, Photoionization, Magnetosheath, Mass Loading
Scientific paper
Optical observations of hot atoms in the atmospheres of Venus and Mars are briefly reviewed. A summary of hot hydrogen and oxygen production and loss processes is given. Results of some recent model calculations as well as a number of new results of the hot hydrogen and oxygen populations are presented and their implication in terms of solar wind interaction processes is discussed.
Cravens Thomas E.
Kim Jongsoo
Nagy Andrew F.
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