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Magnetospheric Multiscale observations of large-amplitude, parallel, electrostatic waves associated with magnetic reconnection at the magnetopause

  • R. E. Ergun
  • , J. C. Holmes
  • , K. A. Goodrich
  • , F. D. Wilder
  • , J. E. Stawarz
  • , S. Eriksson
  • , D. L. Newman
  • , S. J. Schwartz
  • , M. V. Goldman
  • , A. P. Sturner
  • , D. M. Malaspina
  • , M. E. Usanova
  • , R. B. Torbert
  • , M. Argall
  • , P. A. Lindqvist
  • , Y. Khotyaintsev
  • , J. L. Burch
  • , R. J. Strangeway
  • , C. T. Russell
  • , C. J. Pollock
  • B. L. Giles, J. J.C. Dorelli, L. Avanov, M. Hesse, L. J. Chen, B. Lavraud, O. Le Contel, A. Retino, T. D. Phan, J. P. Eastwood, M. Oieroset, J. Drake, M. A. Shay, P. A. Cassak, R. Nakamura, M. Zhou, M. Ashour-Abdalla, M. André
  • University of Colorado Boulder
  • Imperial College London
  • University of New Hampshire
  • Southwest Research Institute
  • KTH Royal Institute of Technology
  • Swedish Institute of Space Physics
  • Institute of Geophysics and Planetary Physics, University of California
  • NASA Goddard Space Flight Center
  • University of Maryland
  • IRAP/CNRS
  • CNRS
  • LPP
  • University of California, Space Sciences Laboratory
  • The Bartol Research Institute
  • West Virginia University
  • Space Research Institute
  • University of California, Los Angeles

Résultats de recherche: Contribution à un journalLettreRevue par des pairs

Résumé

We report observations from the Magnetospheric Multiscale satellites of large-amplitude, parallel, electrostatic waves associated with magnetic reconnection at the Earth's magnetopause. The observed waves have parallel electric fields (E||) with amplitudes on the order of 100 mV/m and display nonlinear characteristics that suggest a possible net E||. These waves are observed within the ion diffusion region and adjacent to (within several electron skin depths) the electron diffusion region. They are in or near the magnetosphere side current layer. Simulation results support that the strong electrostatic linear and nonlinear wave activities appear to be driven by a two stream instability, which is a consequence of mixing cold (<10 eV) plasma in the magnetosphere with warm (~100 eV) plasma from the magnetosheath on a freshly reconnected magnetic field line. The frequent observation of these waves suggests that cold plasma is often present near the magnetopause.

langue originaleAnglais
Pages (de - à)5626-5634
Nombre de pages9
journalGeophysical Research Letters
Volume43
Numéro de publication11
Les DOIs
étatPublié - 16 juin 2016
Modification externeOui

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