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Electron Heating by Debye-Scale Turbulence in Guide-Field Reconnection

  • Yu V. Khotyaintsev
  • , D. B. Graham
  • , K. Steinvall
  • , L. Alm
  • , A. Vaivads
  • , A. Johlander
  • , C. Norgren
  • , W. Li
  • , A. Divin
  • , H. S. Fu
  • , K. J. Hwang
  • , J. L. Burch
  • , N. Ahmadi
  • , O. Le Contel
  • , D. J. Gershman
  • , C. T. Russell
  • , R. B. Torbert
  • Swedish Institute of Space Physics
  • KTH Royal Institute of Technology
  • University of Helsinki
  • University of Bergen
  • National Space Science Center
  • Saint Petersburg State University
  • Beihang University
  • Southwest Research Institute
  • University of Colorado Boulder
  • NASA Goddard Space Flight Center
  • University of California, Los Angeles
  • University of New Hampshire Durham

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

We report electrostatic Debye-scale turbulence developing within the diffusion region of asymmetric magnetopause reconnection with a moderate guide field using observations by the Magnetospheric Multiscale mission. We show that Buneman waves and beam modes cause efficient and fast thermalization of the reconnection electron jet by irreversible phase mixing, during which the jet kinetic energy is transferred into thermal energy. Our results show that the reconnection diffusion region in the presence of a moderate guide field is highly turbulent, and that electrostatic turbulence plays an important role in electron heating.

langue originaleAnglais
Numéro d'article045101
journalPhysical Review Letters
Volume124
Numéro de publication4
Les DOIs
étatPublié - 30 janv. 2020

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