Two-dimensional full particle simulation of a perpendicular collisionless shock with a shock-rest-frame model
arXiv:0806.0199 · doi:10.1086/590408
Abstract
A two-dimensional (2D) shock-rest-frame model for particle simulations is developed. Then full kinetic dynamics of a perpendicular collisionless shock is examined by means of a 2D full particle simulation. We found that in the 2D simulation there are fewer nonthermal electrons due to surfing acceleration which was seen in the previous 1D simulations of a high Mach number perpendicular shock in a low-beta and weakly magnetized plasma. This is because the particle motion along the ambient magnetic field disturbs the formation of coherent electrostatic solitary structures which is necessary for electron surfing acceleration.
4 pages, 4 figures, ApJL in press. The paper with full resolution images is http://theo.phys.sci.hiroshima-u.ac.jp/~ryo/papers/shock_rest_2D.pdf
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- Relativistic Electron Shock Drift Acceleration in Low Mach Number Galaxy Cluster Shocks
- PIC Simulation Methods for Cosmic Radiation and Plasma Instabilities
- Electron Pre-Acceleration at Nonrelativistic High-Mach-Number Perpendicular Shocks
- Electron acceleration at a low-Mach-number perpendicular collisionless shock
- Non-relativistic perpendicular shocks modeling young supernova remnants: nonstationary dynamics and particle acceleration at forward and reverse shocks
- Mach Number Dependence of Electron Heating in High Mach Number Quasiperpendicular Shocks
- Microinstabilities at perpendicular collisionless shocks: A comparison of full particle simulations with different ion to electron mass ratio
- Dynamics and microinstabilities at perpendicular collisionless shock: A comparison of large-scale two-dimensional full particle simulations with different ion to electron mass ratio
- Global explicit particle-in-cell simulations of the nonstationary bow shock and magnetosphere
- Cross-scale coupling at a perpendicular collisionless shock
- Particle simulation study of electron heating by counterstreaming ion beams ahead of supernova remnant shocks
- Mach number and plasma beta dependence of the ion temperature perpendicular to the external magnetic field in the transition region of perpendicular collisionless shocks