Using Driven Particle-In-Cell Simulations to Examine Electron Diffusion by Whistler-Mode Waves
Abstract
Electron diffusion in energy and pitch angle space due to wave-particle interactions with whistler-mode waves is an important component of radiation belt modelling. Whistler-mode waves manifest in a number of different forms, each with different spectral forms and wave amplitudes: chorus, hiss, transmitter and lightning-generated whistler. Electron diffusion coefficients are typically derived for each of these forms using quasilinear theory, and then implemented into numerical diffusion codes. It is expected that the quasilinear approach will have limited success in particular circumstances, and this ultimately motivates our investigation. We report on novel numerical experiments that are somewhat analogous to an active experiment in space, and offer the chance to critically examine the efficacy of predictions by quasilinear theory for a given wave mode and ambient background plasma condition. The approach is to utilize quasi-static boundary-value-problem kinetic numerical experiments, for which whistler-mode waves are excited by using perturbative methods. For different background plasma conditions and wave excitations, diffusion coefficients and other characteristics are directly extracted from particles within the domain, and compared to predictions using quasilinear theory.
- Publication:
-
AGU Fall Meeting Abstracts
- Pub Date:
- December 2019
- Bibcode:
- 2019AGUFMSM21D3208A
- Keywords:
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- 2774 Radiation belts;
- MAGNETOSPHERIC PHYSICS;
- 7803 Active perturbation experiments;
- SPACE PLASMA PHYSICS;
- 7867 Wave/particle interactions;
- SPACE PLASMA PHYSICS;
- 7868 Wave/wave interactions;
- SPACE PLASMA PHYSICS