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Observational Evidence for Stochastic Shock Drift Acceleration of Electrons at the Earth's Bow Shock

  • T. Amano
  • , T. Katou
  • , N. Kitamura
  • , M. Oka
  • , Y. Matsumoto
  • , M. Hoshino
  • , Y. Saito
  • , S. Yokota
  • , B. L. Giles
  • , W. R. Paterson
  • , C. T. Russell
  • , O. Le Contel
  • , R. E. Ergun
  • , P. A. Lindqvist
  • , D. L. Turner
  • , J. F. Fennell
  • , J. B. Blake
  • University of Tokyo
  • University of California, Space Sciences Laboratory
  • Chiba University
  • ISAS/JAXA
  • Osaka University
  • NASA Goddard Space Flight Center
  • Institute of Geophysics and Planetary Physics, University of California
  • Université Paris-Saclay
  • University of Colorado Boulder
  • KTH Royal Institute of Technology
  • The Aerospace Corporation

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

The first-order Fermi acceleration of electrons requires an injection of electrons into a mildly relativistic energy range. However, the mechanism of injection has remained a puzzle both in theory and observation. We present direct evidence for a novel stochastic shock drift acceleration theory for the injection obtained with Magnetospheric Multiscale observations at the Earth's bow shock. The theoretical model can explain electron acceleration to mildly relativistic energies at high-speed astrophysical shocks, which may provide a solution to the long-standing issue of electron injection.

langue originaleAnglais
Numéro d'article065101
journalPhysical Review Letters
Volume124
Numéro de publication6
Les DOIs
étatPublié - 14 févr. 2020
Modification externeOui

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