Test Particle Simulations of Relativistic Electrons Interacting with Whistler-mode Wave in the Radiation Belt

Physics

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2774 Radiation Belts, 7807 Charged Particle Motion And Acceleration, 7845 Particle Acceleration

Scientific paper

We performed test particle simulations where we assumed the dipole geomagnetic field (L=4) and a coherent whistler-mode wave. We found a very efficient acceleration process due to the resonant trapping by a coherent whistler-mode wave propagating away from the equator, which we call relativistic resonant acceleration (RRA). Weakly relativistic electrons of a few hundred keV can be accelerated to the range of a few MeV through a single resonant interaction, if the wave packet is continuously generated near the equator. In reality, however, as is the case with chorus emissions, a whistler-mode wave packet has a finite length. In our simulation, we assumed several wave packets with finite lengths are generated successively and propagate away from the equator. We varied frequency of whistler-mode wave packets to simulate chorus emissions. We also varied wave amplitude which is an important factor for controlling the resonant trapping. We found that electrons are gradually accelerated to a few MeV by interacting with several wave packets. We demonstrate that the RRA plays an important role in the formation of relativistic electron flux in the outer radiation belt.

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