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Collisional vibrational quenching of O2+(v) and other molecular ions in planetary atmospheres
Authors:H. Böhringer  M. Durup-Ferguson  E.E. Ferguson  D.W. Fahey
Affiliation:Aeronomy Laboratory, National Oceanic and Atmospheric Administration Boulder, Colorado 80303 USA
Abstract:New experimental techniques have yielded several thermal energy vibrational quenching rate constants for O2+(v). Rates for quenching of O2+(v = 1) by O2, N2, Ar, CO2, H2, and CH4 are 3(?10), 2(?12), 1(?12), 1(?10), 2.5(?12), and 6(?10) cm3s?1 at 300 K. The quenching is somewhat faster for O2+(v = 2). The triatomic ions CO2+, NO2+, N2O+, SO2+, and H2O+ are all vibrationally deexcited with an efficiency greater than 10?3 in Ar or Ne collisions. A theoretical rationalization of the experimental results leads to the prediction that vibrational quenching in planetary atmospheres will generally be efficient, k > 1(?12) cm3s?1 for almost all ion and neutral gas pairs.
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