Articles | Volume 41, issue 2
https://doi.org/10.5194/angeo-41-327-2023
https://doi.org/10.5194/angeo-41-327-2023
Regular paper
 | 
21 Aug 2023
Regular paper |  | 21 Aug 2023

Velocity of magnetic holes in the solar wind from Cluster multipoint measurements

Henriette Trollvik, Tomas Karlsson, and Savvas Raptis

Viewed

Total article views: 1,102 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
767 254 81 1,102 53 56
  • HTML: 767
  • PDF: 254
  • XML: 81
  • Total: 1,102
  • BibTeX: 53
  • EndNote: 56
Views and downloads (calculated since 24 Feb 2023)
Cumulative views and downloads (calculated since 24 Feb 2023)

Viewed (geographical distribution)

Total article views: 1,102 (including HTML, PDF, and XML) Thereof 1,115 with geography defined and -13 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 20 Nov 2024
Download
Short summary
The solar wind is in a plasma state and can exhibit a range of phenomena like waves and instabilities. One observed phenomenon in the solar wind is magnetic holes (MHs). They are localized depressions in the magnetic field. We studied the motion of MHs using the multispacecraft ESA Cluster mission. We derived their velocities in the solar wind frame and found that both linear and rotational MHs are convected with the solar wind.