Articles | Volume 38, issue 1
https://doi.org/10.5194/angeo-38-51-2020
https://doi.org/10.5194/angeo-38-51-2020
Regular paper
 | 
15 Jan 2020
Regular paper |  | 15 Jan 2020

On the magnetic characteristics of magnetic holes in the solar wind between Mercury and Venus

Martin Volwerk, Charlotte Goetz, Ferdinand Plaschke, Tomas Karlsson, Daniel Heyner, and Brian Anderson

Viewed

Total article views: 1,721 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,137 551 33 1,721 62 38
  • HTML: 1,137
  • PDF: 551
  • XML: 33
  • Total: 1,721
  • BibTeX: 62
  • EndNote: 38
Views and downloads (calculated since 02 Sep 2019)
Cumulative views and downloads (calculated since 02 Sep 2019)

Viewed (geographical distribution)

Total article views: 1,721 (including HTML, PDF, and XML) Thereof 1,549 with geography defined and 172 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 25 Apr 2024
Download
Short summary
The magnetic field that is carried by the solar wind slowly decreases in strength as it moves further from the Sun. However, there are sometimes localized decreases in the magnetic field strength, called magnetic holes. These are small structures where the magnetic field strength decreases to less than 50 % of the surroundings and the plasma density increases. This paper presents a statistical study of the behaviour of these holes between Mercury and Venus using MESSENGER data.