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Development of Turbulent Magnetic Reconnection in a Magnetic Island

  • Can Huang
  • , Quanming Lu
  • , Rongsheng Wang
  • , Fan Guo
  • , Mingyu Wu
  • , San Lu
  • , Shui Wang
  • University of Science and Technology of China
  • Collaborative Innovation Center of Astronautical Science and Technology
  • Los Alamos National Laboratory Theoretical Division

Research output: Contribution to journalArticlepeer-review

Abstract

In this paper, with two-dimensional particle-in-cell simulations, we report that the electron Kelvin-Helmholtz instability is unstable in the current layer associated with a large-scale magnetic island, which is formed in multiple X-line guide field reconnections. The current sheet is fragmented into many small current sheets with widths down to the order of the electron inertial length. Secondary magnetic reconnection then occurs in these fragmented current sheets, which leads to a turbulent state. The electrons are highly energized in such a process.

Original languageEnglish
Article number245
JournalAstrophysical Journal
Volume835
Issue number2
DOIs
StatePublished - 1 Feb 2017
Externally publishedYes

Keywords

  • Sun: flares
  • acceleration of particles
  • magnetic reconnection

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