Storm-time Simulations with the 3D High Energy Electron Radiation Belt Code.

Details Storm-time Simulations with the 3D High Energy Electron Radiation Belt Code. Storm-time Simulations with the 3D High Energy Electron Radiation Belt Code.

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsm33a0343s&link_type=abstract

American Geophysical Union, Fall Meeting 2006, abstract #SM33A-0343

Physics

2716 Energetic Particles: Precipitating, 2720 Energetic Particles: Trapped, 2730 Magnetosphere: Inner, 2774 Radiation Belts, 2788 Magnetic Storms And Substorms (7954)

Scientific paper

Radiation belt electrons gain energy by radially diffusing inwards and through local heating. Losses of radiation belt electrons are provided by the resonant pitch-angle scattering by chorus and EMIC waves, and by outward radial diffusion, when the phase space density has a negative radial gradient. We present simulations of the stormtime dynamics of the radiation belts using the 3D code, obtained by solving the bounce and drift averaged Fokker-Planck equation. Numerical simulations show the relative contribution of various acceleration and loss mechanisms and feedback processes between them.

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