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Multiple overshoot and rebound of a bursty bulk flow

  • E. V. Panov
  • , R. Nakamura
  • , W. Baumjohann
  • , V. Angelopoulos
  • , A. A. Petrukovich
  • , A. Retinò
  • , M. Volwerk
  • , T. Takada
  • , K. H. Glassmeier
  • , J. P. McFadden
  • , D. Larson On Leave From
  • Space Research Institute
  • Space Research Institute (IKI)
  • Institute of Geophysics and Planetary Physics, University of California
  • ISAS/JAXA
  • Technical University Braunschweig
  • Max-Planck-Institut für Sonnensystemforschung
  • University of California, Space Sciences Laboratory

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

162 Citations (Scopus)

Résumé

Chen and Wolf (1999) used a thin-filament theory to construct a 2D model of a bursty bulk flow (BBF) motion inside the plasma sheet. The modeling revealed that the low-entropy filament overshoots its equilibrium position and executes a heavily damped oscillation about that position. In this letter we demonstrate, for the first time, the multiple overshoot and rebound of a BBF observed by the five THEMIS probes on 17 March 2008 just after 10:22 UT. We found that the BBF oscillatory braking was accompanied by interlaced enhancements and depletions of radial pressure gradients. The earthward and tailward flow bursts caused formation of vortices with opposite sense of rotation.

langue originaleAnglais
Numéro d'articleL08103
journalGeophysical Research Letters
Volume37
Numéro de publication8
Les DOIs
étatPublié - 1 avr. 2010
Modification externeOui

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