101. Solar wind, F 10.7 , and geomagnetic activity relationship to the equatorial plasma mass density at geosynchronous orbit
- Author
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R. E. Denton, Robert S. Weigel, and V. Veibell
- Subjects
Physics ,Geomagnetic storm ,Atmospheric Science ,010504 meteorology & atmospheric sciences ,Event (relativity) ,Geosynchronous orbit ,Plasmasphere ,010502 geochemistry & geophysics ,Atmospheric sciences ,01 natural sciences ,Solar wind ,Amplitude ,Earth's magnetic field ,Interplanetary magnetic field ,0105 earth and related environmental sciences - Abstract
We consider two types of events, identified by decreases in Dst below a threshold value and increases in the equatorial mass density at geosynchronous altitudes, ρeq, above a threshold value using the Takahashi et al. [2010] dataset. From the Dst events and 1-day averages, we find that there is a statistically weak and small-amplitude difference between ρeq on the day of the event and the days before and after. When hourly averages are considered, a significant peak is found to occur six hours after event onset, and the primary factor that determines the post-onset peak amplitude in ρeq is elevated F10.7. In addition, for hourly averages, ρeq following the onset of a Dst event depends on the north-south component of the interplanetary magnetic field, Bz after the time of onset, with higher average Bz four hours after the event onset corresponding to larger ρeq value 7-11 hours after onset. From the ρeq events, we find a weak dependence on Bz after the onset of an event, with higher average Bz four hours after the event onset corresponding to larger ρeq values 24-36 hours after onset.
- Published
- 2016
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