Study of Electromagnetic Ion Cyclotron Instability in Dipole Geometry

Details Study of Electromagnetic Ion Cyclotron Instability in Dipole Geometry Study of Electromagnetic Ion Cyclotron Instability in Dipole Geometry

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsm21a0310h&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SM21A-0310

Physics

2700 Magnetospheric Physics (6939), 6939 Magnetospheric Physics (2700)

Scientific paper

The Electromagnetic Ion Cyclotron (EMIC) wave is commonly observed in the Earth's magnetosphere. It is believed to be excited when a large number of particles are injected into the dusk side of the magnetosphere during substorms. Theoretical works have suggested that EMIC waves may contribute significantly to Relativistic Electron Precipitation (REP) by pitch-angle scattering. REP events are one of the important aspect of the radiation belt dynamics. We will be using a hybrid code simulation to study EMIC waves in dipole geometry, including instability, wave propagation, and wave-particle interaction. Up to date results will be shown in this poster.

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