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- W1659241446 abstract "The Wind Imaging Interferometer (WINDII) provides an unprecedented database of the O(1D) airglow emission rate measured during 1991-1995. Results from the database show a strong correlation between the daytime O(1D) emission rate and the solar irradiation, in which the emission rate for a given day increases with increasing cosl/eχ almost linearly, where χ is the solar zenith angle. The daytime aurora therefore can be separated from the background airglow. The daytime cusp (or cleft) aurora is clearly identified in both hemispheres at geomagnetic latitudes 70°-80° even during geomagnetic quiet times. The emission rate in the cusp region is enhanced by 20-120%, i.e. an increase of electron energy deposition by several hundred to 3000 Rayleighs." @default.
- W1659241446 created "2016-06-24" @default.
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- W1659241446 date "2005-01-01" @default.
- W1659241446 modified "2023-09-24" @default.
- W1659241446 title "THE DAYTIME CUSP AURORA IN THE O(1D) EMISSION OBSERVED BY WINDII ON UARS" @default.
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- W1659241446 doi "https://doi.org/10.1016/b978-044451881-1/50030-7" @default.
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