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Statistical Characteristics in the Spectrum of Whistler Waves Near the Diffusion Region of Dayside Magnetopause Reconnection

  • Y. Ren
  • , L. Dai
  • , C. Wang
  • , W. Li
  • , X. Tao
  • , B. Lavraud
  • , O. Le Contel
  • State Key Laboratory of Space Weather
  • National Space Science Center
  • University of Chinese Academy of Sciences
  • Boston University
  • Department of Geophysics and Planetary Science
  • CAS Key Laboratory of Geospace Environment
  • IRAP/CNRS

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

24 Citations (Scopus)

Résumé

Using Magnetospheric Multiscale (MMS) data, we present a statistical analysis revealing characteristics in the frequency spectrum of whistler waves in the vicinity of the diffusion region of magnetopause reconnection. On the magnetosphere side of reconnection, whistler waves are highly centered around the 1/2 electron cyclotron frequency (Ωe). On the magnetosheath side of reconnection, whistler waves are mainly below 1/2 Ωe and peaked around 0.2 Ωe. The electron temperature anisotropy associated with the waves is evaluated. The occurrence rate of the whistler waves is large in the presence of perpendicular electron temperature anisotropy (Te⊥/Te‖ > 1). However, a large part of the whistler waves events occurs in association with parallel electron temperature anisotropy (Te⊥/Te‖ < 1) on the magnetosheath side of reconnection, reflecting a large number of the total observations with this electron condition. These results shed new lights on the whistler-related electron kinetic processes near the reconnection diffusion region.

langue originaleAnglais
Numéro d'articlee2020GL090816
journalGeophysical Research Letters
Volume48
Numéro de publication1
Les DOIs
étatPublié - 16 janv. 2021

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