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- W2077887066 abstract "Abstract Vibrational temperatures of N2 which are significantly greater than the gas kinetic temperature can influence chemical reaction rates and energy exchange processes in the thermosphere. The continuity equation for the number density of vibrational quanta has been solved numerically using representative values for the source and loss terms for the cases of low and high solar activity. The interaction between N2 vibration and thermal electrons, which has been neglected in previous calculations, has been included and shown to be important. Late afternoon maximum vibrational temperatures range from about 1700–3000°K from low to high solar activity. Corresponding noon values range from about 1500–2800°K." @default.
- W2077887066 created "2016-06-24" @default.
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- W2077887066 date "1972-11-01" @default.
- W2077887066 modified "2023-09-23" @default.
- W2077887066 title "Enhanced N2 vibrational temperatures in the thermosphere" @default.
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- W2077887066 doi "https://doi.org/10.1016/0032-0633(72)90119-5" @default.
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