Intrinsic time scale for reconnection on the dayside magnetopause

C. T. Russell, G. Le, H. Kawano, S. M. Petrinec, T. L. Zhang

Research output: Contribution to journalArticlepeer-review

13 Citations (Scopus)


Recently much attention has been focused on the transient behavior of the magnetopause in response to pressure pulses and southward fluctuations of the interplanetary magnetic field. We examine the motion of the magnetopause behind the foreshock and conclude that this motion is affected by foreshock pressure variations but not by fluctuations in the direction of the magnetic field. Neither magnetopause erosion nor flux transfer event occurrence is controlled by the foreshock. On the contrary, flux transfer events occur at times of steady IMF and their quasi-periodic behavior is controlled by the magnetopause or the magnetosphere and is not driven by the external boundary conditions. Since flux transfer events are clearly due to reconnection, this observation implies that the IMF must be southward some time perhaps as long as 7 minutes before flux transfer begins.

Original languageEnglish
Pages (from-to)1913-1917
Number of pages5
JournalAdvances in Space Research
Issue number12
Publication statusPublished - Jan 1 1997
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • Aerospace Engineering
  • Astronomy and Astrophysics
  • Geophysics
  • Atmospheric Science
  • Space and Planetary Science
  • Earth and Planetary Sciences(all)


Dive into the research topics of 'Intrinsic time scale for reconnection on the dayside magnetopause'. Together they form a unique fingerprint.

Cite this