English

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

R2 v1 2026-06-21T12:19:20.683Z