Articles | Volume 36, issue 4
https://doi.org/10.5194/angeo-36-1027-2018
https://doi.org/10.5194/angeo-36-1027-2018
Regular paper
 | 
27 Jul 2018
Regular paper |  | 27 Jul 2018

A possible source mechanism for magnetotail current sheet flapping

Liisa Juusola, Yann Pfau-Kempf, Urs Ganse, Markus Battarbee, Thiago Brito, Maxime Grandin, Lucile Turc, and Minna Palmroth

Viewed

Total article views: 3,389 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
2,350 951 88 3,389 125 149
  • HTML: 2,350
  • PDF: 951
  • XML: 88
  • Total: 3,389
  • BibTeX: 125
  • EndNote: 149
Views and downloads (calculated since 25 May 2018)
Cumulative views and downloads (calculated since 25 May 2018)

Viewed (geographical distribution)

Total article views: 3,389 (including HTML, PDF, and XML) Thereof 3,241 with geography defined and 148 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 19 Nov 2025
Download
Short summary
The Earth's magnetic field is shaped by the solar wind. On the dayside the field is compressed and on the nightside it is stretched as a long tail. The tail has been observed to occasionally undergo flapping motions, but the origin of these motions is not understood. We study the flapping using a numerical simulation of the near-Earth space. We present a possible explanation for how the flapping could be initiated by a passing disturbance and then maintained as a standing wave.
Share