Abstract
A sounding rocket measurement of the ultraviolet, atomic oxygen dayglow reveals an excess of emission compared to standard thermospheric model calculations at exospheric altitudes. We explore two explanations for this discrepancy: a breakdown of the radiative transfer model due to nonlocal thermal equilibrium (non‐LTE) conditions above the exobase and a hot atomic oxygen geocorona. In particular, the effects of non‐LTE on the ³P2,1,0 sublevel populations are modeled, and a hot O component in the upper thermosphere and lower exosphere is added to investigate the effects on the modeled emissions. For both cases, the data are reanalyzed and compared with the results using a standard LTE model. A hot O geocorona having a peak density of 106 cm−3 at 550 km and a temperature of 4000 K is consistent with the data and appears to be the most reasonable explanation of the high‐altitude enhanced emissions observed in the data.
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