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The O2+ vibrational distribution in the Venusian ionosphere
Authors:JL Fox
Institution:Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138. U.S.A.
Abstract:Calculations are presented of the vibrational distribution of O2+ in the Venusian ionosphere for a model atmosphere based on Pioneer Venus data. At 100 km, quenching precludes the survival of vibrationally excited O2+. At the exobase, near 200 km, more than half are vibrationally excited. The effects of vibrationally excited O2+ on the hot oxygen corona and the airglow are discussed.
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