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- W2056534717 abstract "A technique developed to deduce exospheric temperatures from the 7320- to 7330-A emission measured by the visible airglow experiment on board the AE-E satellite is considered. An excess emission in the measured 7320- to 7330-A brightness is noticed as a result of the interaction between the spacecraft and the atmosphere. The observed brightnesses are corrected for this effect. The galactic background emission is also carefully subtracted. The deduced temperatures exhibit a positive correlation with solar activity. It varies from approximately 700 K in late 1976 to approximately 1700 K at the peak of this solar cycle. The presence of a nonthermal oxygen corona is considered inconclusive." @default.
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- W2056534717 date "1982-01-01" @default.
- W2056534717 modified "2023-10-18" @default.
- W2056534717 title "Exospheric temperatures deduced from 7320- to 7330-Å (O+(²P) - O+(²D)) twilight observations" @default.
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- W2056534717 doi "https://doi.org/10.1029/ja087ia02p00913" @default.
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