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Global view of dayside magnetic reconnection with the dusk-dawn IMF orientation: A statistical study for Double Star and Cluster data

  • Z. Y. Pu*
  • , X. G. Zhang
  • , X. G. Wang
  • , Jue Wang
  • , X. Z. Zhou
  • , M. W. Dunlop
  • , Lun Xie
  • , C. J. Xiao
  • , Qiu Gang Zhong
  • , Sui Yan Fu
  • , Z. X. Liu
  • , C. M. Carr
  • , Z. Wei Ma
  • , C. Shen
  • , E. Lucek
  • , Henri Rème
  • , Philippe Escoubet
  • *Corresponding author for this work
  • Peking University
  • CAS - National Space Science Center
  • University of Massachusetts Lowell
  • Rutherford Appleton Laboratory
  • CAS - National Astronomical Observatories
  • Imperial College London
  • Zhejiang University
  • CNRS
  • ESA/ESTEC

Research output: Contribution to journalArticlepeer-review

Abstract

Double Star/TC-1 and Cluster data show that both component reconnection and anti-parallel reconnection occur at the magnetopause when the interplanetary magnetic field (IMF) is predominantly dawnward. The occurrence of these different features under these very similar IMF conditions are further confirmed by a statistical study of 290 fast flows measured in both the low and high latitude magnetopause boundary layers. The directions of these fast flows suggest a possible S-shaped configuration of the reconnection X-line under such a dawnward dominated IMF orientation.

Original languageEnglish
Article numberL20101
JournalGeophysical Research Letters
Volume34
Issue number20
DOIs
StatePublished - 28 Oct 2007
Externally publishedYes

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