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Quadrupolar pattern of the asymmetric guide-field reconnection

  • F. Z. Peng
  • , H. S. Fu*
  • , J. B. Cao
  • , D. B. Graham
  • , Z. Z. Chen
  • , D. Cao
  • , Y. Xu
  • , S. Y. Huang
  • , T. Y. Wang
  • , Y. V. Khotyaintsev
  • , M. Andre
  • , C. T. Russell
  • , B. Giles
  • , P. A. Lindqvist
  • , R. B. Torbert
  • , R. E. Ergun
  • , J. L. Burch
  • *此作品的通讯作者
  • Beihang University
  • Box 537
  • Wuhan University
  • University of California at Los Angeles
  • NASA Goddard Space Flight Center
  • KTH Royal Institute of Technology
  • University of New Hampshire
  • University of Colorado Boulder
  • Southwest Research Institute

科研成果: 期刊稿件文章同行评审

摘要

With high-resolution data of the recently launched Magnetospheric Multiscale mission, we report a magnetic reconnection event at the dayside magnetopause. This reconnection event, having a density asymmetry Nhigh/Nlow ≈ 2 on the two sides of the reconnecting current sheet and a guide field Bg ≈ 0.4B0 in the “out-of-plane” direction, exhibit all the two-fluid features: Alfvenic plasma jets in the outflow region, bipolar Hall electric fields toward the current sheet center, quadrupolar Hall magnetic fields in the “out-of-plane” direction, and the corresponding Hall currents. Obviously, the density asymmetry Nhigh/Nlow ≈ 2 and the guide field Bg ≈ 0.4B0 are not sufficient to dismiss the quadrupolar pattern of Hall reconnection. This is different from previous simulations, where the bipolar pattern of Hall reconnection was suggested.

源语言英语
页(从-至)6349-6356
页数8
期刊Journal of Geophysical Research: Space Physics
122
6
DOI
出版状态已出版 - 1 6月 2017

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