Free Energy to Drive the Magnetosonic Instability at Geosynchronous Orbit

Physics

Scientific paper

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[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.

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