Physics
Scientific paper
Oct 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002georl..29t..15c&link_type=abstract
Geophysical Research Letters, Volume 29, Issue 20, pp. 15-1, CiteID 1954, DOI 10.1029/2002GL015160
Physics
44
Magnetospheric Physics: Magnetosphere-Inner, Magnetospheric Physics: Ring Current, Magnetospheric Physics: Storms And Substorms, Magnetospheric Physics: Magnetospheric Configuration And Dynamics, Magnetospheric Physics: Magnetosphere/Ionosphere Interactions
Scientific paper
The local time distribution of the ring current in the 27-119 keV range during several geomagnetic storm main phases have been investigated. The data was obtained by the high energy neutral atom (HENA) imager onboard IMAGE. Global proton distributions are derived from the observed energetic neutral atom (ENA) images using a linear inversion technique. During storms with low IMF By the peak of the proton distribution is around 01 MLT. For storms with high IMF By the peak can rotate to dawn. The rotation angle depends on solar wind velocity and interplanetary magnetic field (IMF) By, but less on IMF Bz. We discuss how this morphology implies the existence of strong and skewed equatorial electric fields in the inner magnetosphere. Our results are consistent with in-situ ring current measurements, radar observations and with kinetic models that self-consistently calculate the electric field produced by the closure of the partial ring current.
C:son Brandt Pontus
DeMajistre Robert
Fok Mei Ching
Mitchell Donald G.
Ohtani Shin
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