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Suppression of collisionless magnetic reconnection in asymmetric current sheets

Plasma Physics 2016-07-27 v1 Earth and Planetary Astrophysics Solar and Stellar Astrophysics Space Physics

Abstract

Using fully kinetic simulations, we study the suppression of asymmetric reconnection in the limit where the diamagnetic drift speed >> Alfven speed and the magnetic shear angle is moderate. We demonstrate that the slippage between electrons and the magnetic flux facilitates reconnection, and can even result in fast reconnection that lacks one of the outflow jets. Through comparing a case where the diamagnetic drift is supported by the temperature gradient with a companion case that has a density gradient instead, we identify a robust suppression mechanism. The drift of the x-line is slowed down locally by the asymmetric nature of the current sheet and the resulting tearing modes, then the x-line is run over and swallowed by the faster-moving following flux.

Keywords

Cite

@article{arxiv.1602.05118,
  title  = {Suppression of collisionless magnetic reconnection in asymmetric current sheets},
  author = {Yi-Hsin Liu and Michael Hesse},
  journal= {arXiv preprint arXiv:1602.05118},
  year   = {2016}
}

Comments

5 pages, 4 figures