Articles | Volume 43, issue 1
https://doi.org/10.5194/angeo-43-151-2025
https://doi.org/10.5194/angeo-43-151-2025
Regular paper
 | 
21 Feb 2025
Regular paper |  | 21 Feb 2025

Investigation of the occurrence of significant deviations in the magnetopause location: solar-wind and foreshock effects

Niklas Grimmich, Adrian Pöppelwerth, Martin Owain Archer, David Gary Sibeck, Ferdinand Plaschke, Wenli Mo, Vicki Toy-Edens, Drew Lawson Turner, Hyangpyo Kim, and Rumi Nakamura

Viewed

Total article views: 371 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
193 67 111 371 13 12
  • HTML: 193
  • PDF: 67
  • XML: 111
  • Total: 371
  • BibTeX: 13
  • EndNote: 12
Views and downloads (calculated since 08 Oct 2024)
Cumulative views and downloads (calculated since 08 Oct 2024)

Viewed (geographical distribution)

Total article views: 371 (including HTML, PDF, and XML) Thereof 363 with geography defined and 8 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 21 Feb 2025
Download
Short summary
The boundary of Earth's magnetic field, the magnetopause, deflects and reacts to the solar wind, the energetic particles emanating from the Sun. We find that certain types of solar wind favour the occurrence of deviations between the magnetopause locations observed by spacecraft and those predicted by models. In addition, the turbulent region in front of the magnetopause, the foreshock, has a large influence on the location of the magnetopause and thus on the accuracy of the model predictions.
Share