Articles | Volume 33, issue 10
https://doi.org/10.5194/angeo-33-1301-2015
https://doi.org/10.5194/angeo-33-1301-2015
Regular paper
 | 
26 Oct 2015
Regular paper |  | 26 Oct 2015

A physical explanation for the magnetic decrease ahead of dipolarization fronts

Z. H. Yao, J. Liu, C. J. Owen, C. Forsyth, I. J. Rae, Z. Y. Pu, H. S. Fu, X.-Z. Zhou, Q. Q. Shi, A. M. Du, R. L. Guo, and X. N. Chu

Viewed

Total article views: 1,804 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,053 676 75 1,804 75 82
  • HTML: 1,053
  • PDF: 676
  • XML: 75
  • Total: 1,804
  • BibTeX: 75
  • EndNote: 82
Views and downloads (calculated since 26 Oct 2015)
Cumulative views and downloads (calculated since 26 Oct 2015)

Cited

Latest update: 23 Nov 2024
Download
Short summary
We use THEMIS large data set of dipolarization front events to build a 2-D pressure distribution in XZ plane, and thus derive the current system around the dipolarization front. Our results show that a banana current loop is formed around the dipolarization front. This current is also suggested to be the reason for the magnetic dip observed ahead of the dipolarization front. In addition, the current density is too small to contribute a substorm current wedge.