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Nitrogen oxides and the airglow
Journal of Atmospheric and Terrestrial Physics, 1955Abstract The chemospheric processes lead to various possibilities for description of the contribution of nitrogen oxides in the airglow. An excitation of the Vegard-Kaplan system is indicated when nitric oxide is formed by a three-body collision process involving molecular nitrogen.
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Planetary and Space Science, 1992
Abstract Airglow OH emissions originate from the mesopause and provide optical signatures of various physical and chemical processes occurring in this region of the upper atmosphere. Emissions from different vibrational levels of the mesopause OH (in the ground electronic state) may peak at different heights. roughly between 80 and 90 km.
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Abstract Airglow OH emissions originate from the mesopause and provide optical signatures of various physical and chemical processes occurring in this region of the upper atmosphere. Emissions from different vibrational levels of the mesopause OH (in the ground electronic state) may peak at different heights. roughly between 80 and 90 km.
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The spectrum of the airglow and the aurora
Reports on Progress in Physics, 1951The spectrum of the night glow has been investigated from 3000 A. to 14 μ. While the majority of the emissions have been identified, numerous unidentified bands remain. The molecules O2, N2 and OH contribute emissions between 3000 A. and 4·5 μ. The enhancement of the N2+ bands and the [OI] and Na D-lines during twilight is generally attributed to ...
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Three‐dimensional modeling of equatorial spread F airglow enhancements
Geophysical Research Letters, 2009Joseph Huba, Jonathan Krall
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