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• W1985593751 abstract "The rate coefficient for the reaction O+ + N2 → NO+ + N is determined as a function of temperature from the photochemistry of NO+ for both day and night conditions by using a large sample (>5300) of simultaneous measurements of ion and neutral concentrations and temperatures made by the Atmosphere Explorer C satellite. The results cover the ion temperature range 500–1200°K and can be represented by 1.2 × 10−12(Ti/300)−0.8 cm³ s−1. Using recent flow drift tube results, we calculate the rate coefficient as a function of ion temperature and mean ion drift velocity for ionospheric conditions and find that the satellite and laboratory determinations are in good agreement. Using this temperature dependence, we then refine our earlier determination of the dissociative recombination coefficient of NO+ with electrons. We confirm that this rate coefficient is represented by 4.2 × 10−7(Te/300)−0.85 cm³ s−1." @default.
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• W1985593751 date "1977-08-01" @default.
• W1985593751 modified "2023-10-10" @default.
• W1985593751 title "The rate coefficient for the O⁺+ N₂reaction in the ionosphere" @default.
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• W1985593751 doi "https://doi.org/10.1029/ja082i022p03287" @default.
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