O/++/ in the Venusian ionosphere

Details O/++/ in the Venusian ionosphere O/++/ in the Venusian ionosphere

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981jgr....86.2438f&link_type=abstract

Journal of Geophysical Research, vol. 86, Apr. 1, 1981, p. 2438-2442.

Physics

21

Atmospheric Models, Oxygen Ions, Photoionization, Planetary Ionospheres, Venus Atmosphere, Airglow, Atmospheric Chemistry, Carbon Dioxide, Carbon Monoxide, Charge Transfer, Helium Ions, Ion Production Rates, Nitrogen Ions, Pioneer Venus Spacecraft, Venus, Ionosphere, Oxygen, Photochemistry, Ions, Airglow, Source Medium, Models, Data, Production Rates, Altitude, Carbon, Nitrogen, Density, Comparisons

Scientific paper

It is shown that the revised photochemical theory for O(2+) in the earth's ionosphere, where double photoionization of O is the dominant source, is consistent with recent O(2+) measurements on Venus. A rate coefficient of 1.5 x 10 to the -10th cu m/sec for O(2+) + O is obtained, and the possible importance of O(2+) chemistry on minor atomic ions and airglow emissions is explored.

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