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Switch-off slow shock/rotational discontinuity structures in collisionless magnetic reconnection: What to look for in satellite observations

  • M. E. Innocenti
  • , E. Cazzola
  • , R. Mistry
  • , J. P. Eastwood
  • , M. V. Goldman
  • , D. L. Newman
  • , S. Markidis
  • , G. Lapenta
  • Centre for Mathematical Plasma Astrophysics
  • KU Leuven
  • University of Surrey
  • Imperial College London
  • Department of Physics
  • University of Colorado Boulder
  • Department of Computational Science and Technologies
  • KTH Royal Institute of Technology

Research output: Contribution to journal › Article › peer-review

8 Citations (Scopus)

Abstract

In Innocenti et al. (2015) we have observed and characterized for the first time Petschek-like switch-off slow shock/rotational discontinuity (SO-SS/RD) compound structures in a 2-D fully kinetic simulation of collisionless magnetic reconnection. Observing these structures in the solar wind or in the magnetotail would corroborate the possibility that Petschek exhausts develop in collisionless media as a result of single X point collisionless reconnection. Here we highlight their signatures in simulations with the aim of easing their identification in observations. The most notable signatures include a four-peaked ion current profile in the out-of-plane direction, associated ion distribution functions, increased electron and ion anisotropy downstream the SS, and increased electron agyrotropy downstream the RDs.

Original languageEnglish
Pages (from-to)3447-3455
Number of pages9
JournalGeophysical Research Letters
Volume44
Issue number8
DOIs
Publication statusPublished - 28 Apr 2017
Externally publishedYes

Keywords

  • Hall reconnection
  • Petschek exhaust
  • anisotropy and agyrotropy
  • ion distribution functions
  • magnetic reconnection
  • slow shock/rotational discontinuity

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