Physics
Scientific paper
Dec 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsm21a0326d&link_type=abstract
American Geophysical Union, Fall Meeting 2007, abstract #SM21A-0326
Physics
2716 Energetic Particles: Precipitating, 2730 Magnetosphere: Inner, 2736 Magnetosphere/Ionosphere Interactions (2431), 2788 Magnetic Storms And Substorms (7954), 7954 Magnetic Storms (2788)
Scientific paper
A variety of phenomena which occur during large geomagnetic storms (DST<-75 nT) are not yet fully understood. One such phenomenon, which affects ionospheric conditions and may be useful as a diagnostic for processes occurring at ~3-6 Re, is the occurrence of low latitude (ILat<65) broadband accelerated electron events observable at altitudes of ~2000-4000 km by the FAST satellite. Results of an initial study of 3+ years of FAST data indicate that such electrons are observed in ~6% of the low latitude, nightside (21- 03 MLT) FAST data during large storms versus <~1% during non-storm times. Individual storms have observed occurrence probabilities as high as 24%. Although properties of the events, and thus likely causes, vary, many events are accompanied by particle distributions and wave signatures that are similar to those observed during Alfvén-wave accelerated electron events on the plasma sheet boundary layer (PSBL). Alfvén- wave acceleration of electrons on the PSBL has been and continues to be well studied. Results of a recent study of PSBL Alfvén-wave events observed with Polar that may provide additional insight will also be discussed. That study compares altitude dependencies of wave properties at ~3-9 Re and differences in these dependencies between major storm and non-storm events.
Cattell Cynthia
Dombeck J.
Keiling Andreas
McFadden Johnjoe
Strangeway Robert
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