Articles | Volume 37, issue 3
https://doi.org/10.5194/angeo-37-299-2019
https://doi.org/10.5194/angeo-37-299-2019
Review paper
 | 
08 May 2019
Review paper |  | 08 May 2019

Kinematic models of the interplanetary magnetic field

Christoph Lhotka and Yasuhito Narita

Viewed

Total article views: 2,989 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
2,124 789 76 2,989 85 75
  • HTML: 2,124
  • PDF: 789
  • XML: 76
  • Total: 2,989
  • BibTeX: 85
  • EndNote: 75
Views and downloads (calculated since 06 Dec 2018)
Cumulative views and downloads (calculated since 06 Dec 2018)

Viewed (geographical distribution)

Total article views: 2,989 (including HTML, PDF, and XML) Thereof 2,613 with geography defined and 376 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 07 Oct 2024
Download
Short summary
The interplanetary magnetic field is a consequence of the solar magnetic field and the solar wind. Different magnetic field models exist in literature that allow us to better understand how the solar field extends throughout the solar system. We highlight different aspects of these different interplanetary magnetic field models and discuss possible applications. Verification of these models will become possible using data from the Parker Solar Probe and BepiColombo space mission.