Skip to main navigation Skip to search Skip to main content

Drift waves, intense parallel electric fields, and turbulence associated with asymmetric magnetic reconnection at the magnetopause

  • R. E. Ergun
  • , L. J. Chen
  • , F. D. Wilder
  • , N. Ahmadi
  • , S. Eriksson
  • , M. E. Usanova
  • , K. A. Goodrich
  • , J. C. Holmes
  • , A. P. Sturner
  • , D. M. Malaspina
  • , D. L. Newman
  • , R. B. Torbert
  • , M. R. Argall
  • , P. A. Lindqvist
  • , J. L. Burch
  • , J. M. Webster
  • , J. F. Drake
  • , L. Price
  • , P. A. Cassak
  • , M. Swisdak
  • M. A. Shay, D. B. Graham, R. J. Strangeway, C. T. Russell, B. L. Giles, J. C. Dorelli, D. Gershman, L. Avanov, M. Hesse, B. Lavraud, O. Le Contel, A. Retino, T. D. Phan, M. V. Goldman, J. E. Stawarz, S. J. Schwartz, J. P. Eastwood, K. J. Hwang, R. Nakamura, S. Wang
  • University of Colorado Boulder
  • NASA Goddard Space Flight Center
  • University of Maryland, College Park
  • University of New Hampshire Durham
  • Southwest Research Institute
  • KTH Royal Institute of Technology
  • West Virginia University
  • University of Delaware
  • Swedish Institute of Space Physics
  • University of California, Los Angeles
  • IRAP/CNRS
  • Centre national de la recherche scientifique
  • LPP
  • University of California, Space Sciences Laboratory
  • Imperial College London
  • Space Research Institute

Research output: Contribution to journalArticlepeer-review

Abstract

Observations of magnetic reconnection at Earth's magnetopause often display asymmetric structures that are accompanied by strong magnetic field (B) fluctuations and large-amplitude parallel electric fields (E||). The B turbulence is most intense at frequencies above the ion cyclotron frequency and below the lower hybrid frequency. The B fluctuations are consistent with a thin, oscillating current sheet that is corrugated along the electron flow direction (along the X line), which is a type of electromagnetic drift wave. Near the X line, electron flow is primarily due to a Hall electric field, which diverts ion flow in asymmetric reconnection and accompanies the instability. Importantly, the drift waves appear to drive strong parallel currents which, in turn, generate large-amplitude (~100 mV/m) E|| in the form of nonlinear waves and structures. These observations suggest that turbulence may be common in asymmetric reconnection, penetrate into the electron diffusion region, and possibly influence the magnetic reconnection process.

Original languageEnglish
Pages (from-to)2978-2986
Number of pages9
JournalGeophysical Research Letters
Volume44
Issue number7
DOIs
Publication statusPublished - 16 Apr 2017
Externally publishedYes

Keywords

  • asymmetric magnetic reconnection
  • drift waves
  • parallel electric fields
  • turbulence

Fingerprint

Dive into the research topics of 'Drift waves, intense parallel electric fields, and turbulence associated with asymmetric magnetic reconnection at the magnetopause'. Together they form a unique fingerprint.

Cite this