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Double Star TC-1 observations of component reconnection at the dayside magnetopause: A preliminary study

  • Z. Y. Pu*
  • , C. J. Xiao
  • , X. G. Zhang
  • , Z. Y. Huang
  • , S. Y. Fu
  • , Z. X. Liu
  • , M. W. Dunlop
  • , Q. G. Zong
  • , C. M. Carr
  • , H. Rème
  • , I. Dandouras
  • , A. Fazakerley
  • , T. Phan
  • , T. L. Zhang
  • , H. Zhang
  • , X. G. Wang
  • *Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

In spring 2004 Double Star TC-1 measured a number of reconnection signatures at the dayside low-latitude magnetopause (MP) when there was a notable By component in the magnetosheath. In a number of events we can show that reconnection was operating nearby TC-1 in the subsolar MP region. In this paper we describe three representative events: (a) event on 21 March 2004 in which the reconnection site can be remotely monitored, the space-craft was passing by the X-line; (b) event on 12 March 2004 in which TC-1 observed the magnetospheric part of the quadrupolar field, together with a consistent flow reversal; (c) event on 26 March 2004 which occurred for northward IMF, TC-1 observed a reversal of vy across the equatorial MP. In these events the shear angles across the MP were considerably smaller than 180°; a noticeable guide field was present. These observations are consistent with near equatorial component merging, suggesting that component reconnection preferably occurs at the dayside low-latitude MP. There is evidence that when a pronounced magnetic shear across the MP exists in the By component, reconnection may operate at the dayside low-latitude MP for northward IMF Bz.

Original languageEnglish
Pages (from-to)2889-2895
Number of pages7
JournalAnnales Geophysicae
Volume23
Issue number8
DOIs
StatePublished - 8 Nov 2005
Externally publishedYes

Keywords

  • Magnetospheric physics (Magnetopause, cusp, arid boundary layers; Solar wind-magnetosphere interactions)
  • Space plasma physics (Magnetic reconnection)

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