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In situ spacecraft observations of a structured electron diffusion region during magnetopause reconnection

  • Giulia Cozzani*
  • , A. Retinò
  • , F. Califano
  • , A. Alexandrova
  • , O. Le Contel
  • , Y. Khotyaintsev
  • , A. Vaivads
  • , H. S. Fu
  • , F. Catapano
  • , H. Breuillard
  • , N. Ahmadi
  • , P. A. Lindqvist
  • , R. E. Ergun
  • , R. B. Torbert
  • , B. L. Giles
  • , C. T. Russell
  • , R. Nakamura
  • , S. Fuselier
  • , B. H. Mauk
  • , T. Moore
  • J. L. Burch
*此作品的通讯作者
  • Sorbonne Université
  • University of Pisa
  • Box 537
  • University of Calabria
  • Université d'Orléans
  • University of Colorado Boulder
  • KTH Royal Institute of Technology
  • University of New Hampshire
  • NASA Goddard Space Flight Center
  • University of California at Los Angeles
  • Austrian Academy of Sciences
  • Southwest Research Institute
  • University of Texas at San Antonio
  • Johns Hopkins University Applied Physics Laboratory

科研成果: 期刊稿件文章同行评审

摘要

The electron diffusion region (EDR) is the region where magnetic reconnection is initiated and electrons are energized. Because of experimental difficulties, the structure of the EDR is still poorly understood. A key question is whether the EDR has a homogeneous or patchy structure. Here we report Magnetospheric Multiscale (MMS) spacecraft observations providing evidence of inhomogeneous current densities and energy conversion over a few electron inertial lengths within an EDR at the terrestrial magnetopause, suggesting that the EDR can be rather structured. These inhomogenenities are revealed through multipoint measurements because the spacecraft separation is comparable to a few electron inertial lengths, allowing the entire MMS tetrahedron to be within the EDR most of the time. These observations are consistent with recent high-resolution and low-noise kinetic simulations.

源语言英语
文章编号043204
期刊Physical Review E
99
4
DOI
出版状态已出版 - 9 4月 2019

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