Physics
Scientific paper
Apr 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008georl..3517s14w&link_type=abstract
Geophysical Research Letters, Volume 35, Issue 17, CiteID L17S14
Physics
4
Magnetospheric Physics: Plasma Sheet, Magnetospheric Physics: Ring Current, Magnetospheric Physics: Plasma Convection (2463), Magnetospheric Physics: Magnetic Storms And Substorms (7954), Magnetospheric Physics: Magnetosphere: Inner
Scientific paper
Observations from the THEMIS spacecraft during a weak magnetic storm clearly show that the inner edge of the ion plasma sheet near dusk moved from r ~ 6 R E during the pre-storm quiet time to r ~ 3.5 R E during the main phase, and then moved outward during the recovery phase. The plasma sheet particles from the tail reached the inner magnetosphere during the main phase through open drift paths, which extended earthward with increasing convection, and were energized to ring current energies, resulting in an increase in ring current population. During the recovery phase, the plasma sheet region retreated to outside the inner magnetosphere as the region of open drift paths moved outward with decreasing convection, leaving the ring current particles within the expended closed drift path region. With no new particles from the plasma sheet, ring current population gradually decreased due to losses as the recovery phase proceeded.
Angelopoulos Vassilis
Auster Hans-Ulrich
Frey Sabine
Larson Davin
Lyons Larry R.
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