Physics
Scientific paper
Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsm13c..08t&link_type=abstract
American Geophysical Union, Fall Meeting 2010, abstract #SM13C-08
Physics
[2764] Magnetospheric Physics / Plasma Sheet, [2772] Magnetospheric Physics / Plasma Waves And Instabilities
Scientific paper
Equatorial magnetosonic waves have recently been suggested as a possible means for accelerating radiation-belt electrons. The theoretical criterion for growth of such waves is the presence of a positive slope in the hot-proton distribution function near the Alven speed in the direction perpendicular to the magnetic field. Recent analyses of the storm-time ring-current ion distributions predicted by the RAM model show that the energy-dependent drifts and losses of injected ions can produce free energy suitable to drive the magnetosonic instability. Moreover, a recent case study of ion observations at geosynchronous orbit likewise reveals conditions appropriate for magnetosonic wave growth. We have now conducted a survey of the occurrence frequency of regions of positive slope in the perpendicular hot-ion (1-45 keV) distribution observed at geosynchronous orbit by the LANL MPA instrument. The survey covers more than a full solar cycle and thus includes a wide range of magnetospheric activity levels. We present statistical results from this survey that characterize the locations and conditions for which free energy exists in the hot-ion population at geosynchronous orbit that could potentially give rise to magnetosonic waves.
Chen Leon L.
Denton Michael H.
Jordanova Vania K.
Mansergh Thorne Richard
Thomsen Michelle F.
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