Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1772332 | High Energy Density Physics | 2015 | 8 Pages |
Abstract
The role of electron dynamics in the process of a collisionless shock formation is analyzed with particle-in-cell simulations, the test-particles method, and quasilinear theory. The model of electron stochastic heating in turbulent electromagnetic fields corresponding to the nonlinear stage of two-stream and Weibel instabilities is developed. The analysis of electron and field heating rates shows that the ion motion provides the energy supply for a significant continuous heating of electrons. Such a heating thus plays a role of a friction force for ions, leading to their deceleration and a shock formation.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
S.G. Bochkarev, E. d'Humières, Ph. Korneev, V.Yu. Bychenkov, V. Tikhonchuk,