Nonlinear Development of Streaming Instabilities In Strongly Magnetized Plasmas
Space Physics
2015-05-13 v2 Solar and Stellar Astrophysics
Plasma Physics
Abstract
The nonlinear development of streaming instabilities in the current layers formed during magnetic reconnection with a guide field is explored. Theory and 3-D particle-in-cell simulations reveal two distinct phases. First, the parallel Buneman instability grows and traps low velocity electrons. The remaining electrons then drive two forms of turbulence: the parallel electron-electron two-stream instability and the nearly-perpendicular lower hybrid instability. The high velocity electrons resonate with the turbulence and transfer momentum to the ions and low velocity electrons.
Keywords
Cite
@article{arxiv.0903.1311,
title = {Nonlinear Development of Streaming Instabilities In Strongly Magnetized Plasmas},
author = {H. Che and J. F. Drake and M. Swisdak and P. H. Yoon},
journal= {arXiv preprint arXiv:0903.1311},
year = {2015}
}
Comments
Accepted by PRL