Drift and suppression of x-lines in asymmetric magnetic reconnection

POSTER

Abstract

The x-line of reconnection drifts in the outflow direction when the current sheet is asymmetric and has a guide field. In particular, reconnection can be choked off if the x-line drifts too fast. The energy conversion from the magnetic field to particles is hence significantly reduced. A suppression was suggested when the relative diamagnetic drift speed between electrons and ions exceeds the Alfv\'en speed based on the reconnecting magnetic field.\footnote{M. Swisdak et al., J. Geophys. Res., {\bf 108}, 1218, 2003} In this work, we re-visit this problem using Particle-in-Cell simulations. We break down the pressure gradient to a combination of density and temperature gradients, and find that the suppression effect from the temperature gradient is much weaker compared to that with a density gradient, consistent with a recent work using gyrokinetic simulations.\footnote{S. Kobayahsi et al., Phys. Plasmas, {\bf 21}, 04074, 2014} In addition, a wide range of parameters are explored to benchmark the theory, and the flux-breaking mechanism in these drifting x-lines is analyzed. This work has potential application at Earth's magnetopause and in Tokamak devices.\footnote{M. T. Beidler and P. Cassak, Phys. Rev. Let., {\bf 107}, 255002, 2011}

Authors

  • Yi-Hsin Liu

    • NASA/GSFC
    • NASA Goddard Space Flight Center
  • Michael Hesse

    • NASA/GSFC
  • William Daughton

    • LANL
  • Paul Cassak

    • WVU