Simulations of Pitch-angle Scattering of Relativistic Electrons With MLT-Dependent Diffusion Coefficients

Details Simulations of Pitch-angle Scattering of Relativistic Electrons With MLT-Dependent Diffusion Coefficients Simulations of Pitch-angle Scattering of Relativistic Electrons With MLT-Dependent Diffusion Coefficients

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsm21a1654s&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #SM21A-1654

Physics

2716 Energetic Particles: Precipitating, 2720 Energetic Particles: Trapped, 2774 Radiation Belts

Scientific paper

We present MLT-dependent simulations of pitch-angle scattering of relativistic (~MeV) electrons by chorus and EMIC waves. Numerical simulations indicate that in the case of scattering by chorus waves, pitch-angle distribution is relatively independent of MLT. In the case of scattering by EMIC and chorus waves, the modeled pitch-angle distribution shows significant variations with MLT. MLT-averaged simulations tend to overestimate net loss during a storm, but can accurately predict equilibrium loss rates and the overall shape of the pitch-angle distribution. Numerical simulations show that EMIC waves not only scatter electrons into the loss cone, but also create gradients in the pitch-angle distribution, assisting chorus waves in scattering of relativistic electrons into the loss cone. We also show that changes in the spectral properties of waves can significantly change loss rates. Loss rates reach a maximum level for EMIC waves with amplitudes above approximately 1 nT, present over a few percent of the drift orbit and then become relatively independent of the amplitudes of EMIC waves.

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