Collisional vibrational quenching of O2+(v) and other molecular ions in planetary atmospheres |
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Authors: | H. Böhringer M. Durup-Ferguson E.E. Ferguson D.W. Fahey |
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Affiliation: | Aeronomy Laboratory, National Oceanic and Atmospheric Administration Boulder, Colorado 80303 USA |
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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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