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Longitudinal Variation in the Thermospheric Superrotation: CHAMP Observation and TIE‐GCM Simulation

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Wang,  Hui
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Lühr,  B.
2.3 Geomagnetism, 2.0 Geophysics, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;

Zhang,  K. D.
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Zitation

Wang, H., Lühr, B., Zhang, K. D. (2021): Longitudinal Variation in the Thermospheric Superrotation: CHAMP Observation and TIE‐GCM Simulation. - Geophysical Research Letters, 48, 18, e2021GL095439.
https://doi.org/10.1029/2021GL095439


Zitierlink: https://gfzpublic.gfz-potsdam.de/pubman/item/item_5009041
Zusammenfassung
By means of 4 years of Challenging Minisatellite Payload (CHAMP) zonal wind observations and a Thermosphere-Ionosphere Electrodynamics General Circulation Model simulation, longitudinal and seasonal variations of thermospheric superrotation at magnetic equator are investigated first. The superrotation shows four- and three-peaked longitudinal patterns in March and September equinoxes, and a two-peaked variation during solstices. The superrotation is stronger in December than in June solstice, and stronger in March than in September equinox. The mean correlation between the zonal variation of superrotation and nighttime eastward wind is about 0.8, while it is 0.6 with daytime westward zonal wind. The interaction between the neutral wind and geomagnetic field plays a more important role in the superrotation, rather than the F-region electron density. The lower atmospheric tides tend to suppress the superrotation, but contribute to the longitudinal patterns of the superrotation. The viscous force is also important for the longitudinal modulation of the superrotation.