Gyrokinetic Particle Simulation of Kinetic Alfvén Wave Turbulence
Abstract
The previous studies of spectral cascade in Alfvénic turbulence clearly show signs of plasma heating, and there are several highly-debated explanations to this phenomenon. We have developed a nonlinear gyrokinetic particle simulation to study the perpendicular spectral cascade caused by Landau damping of kinetic Alfvén wave, which is one of those possible heating mechanisms. The current nonlinear gyrokinetic code includes scalar potential and vector potential. We will propose a new formulation that implements compressional magnetic perturbation into the existent code to form a complete, self-consistent nonlinear simulation.
- Publication:
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AGU Fall Meeting Abstracts
- Pub Date:
- December 2012
- Bibcode:
- 2012AGUFMSH51B2220L
- Keywords:
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- 2159 INTERPLANETARY PHYSICS / Plasma waves and turbulence;
- 2164 INTERPLANETARY PHYSICS / Solar wind plasma;
- 7839 SPACE PLASMA PHYSICS / Nonlinear phenomena;
- 7863 SPACE PLASMA PHYSICS / Turbulence