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Cluster Observations of a Dispersive Flapping Event of Magnetotail Current Sheet

  • Z. J. Rong*
  • , Y. H. Cai
  • , J. W. Gao
  • , A. T.Y. Lui
  • , C. Shen
  • , A. A. Petrukovich
  • , Y. Wei
  • , W. X. Wan
  • *Corresponding author for this work
  • Chinese Academy of Sciences
  • University of Chinese Academy of Sciences
  • Johns Hopkins University Applied Physics Laboratory
  • Harbin Institute of Technology Shenzhen
  • Space Research Institute of the Russian Academy of Sciences

Research output: Contribution to journalArticlepeer-review

Abstract

A kink-like flapping event of Earth magnetotail current sheet, which consists of two frequency bands successively, is studied by the multipoint observations of Cluster. The multipoint analysis of Cluster observations demonstrates that the higher frequency band (period is about 10 min) has faster propagation velocity (about 30 km/s), shorter wavelength (about 3 RE), and smaller amplitude (1–1.5 RE). In contrast, the lower frequency band (period is about 22 min) shows slower propagation velocity (about 21 km/s), longer wavelength (about 4.4 RE), and larger amplitude (2–3 RE). Comparison with the flapping models demonstrates that the dispersion of theoretical models does not show consistency with the results of this event, which suggests that new or more advanced kink-like flapping theories or models in the future have to consider the constraints of the dispersive properties demonstrated by this event.

Original languageEnglish
Pages (from-to)5571-5579
Number of pages9
JournalJournal of Geophysical Research: Space Physics
Volume123
Issue number7
DOIs
StatePublished - Jul 2018
Externally publishedYes

Keywords

  • current sheet
  • dispersive properties
  • flapping waves
  • magnetotail
  • neutral sheet
  • plasma sheet

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