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: 3,095 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
2,183 829 83 3,095 91 80
  • HTML: 2,183
  • PDF: 829
  • XML: 83
  • Total: 3,095
  • BibTeX: 91
  • EndNote: 80
Views and downloads (calculated since 06 Dec 2018)
Cumulative views and downloads (calculated since 06 Dec 2018)

Viewed (geographical distribution)

Total article views: 3,095 (including HTML, PDF, and XML) Thereof 2,715 with geography defined and 380 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 14 Jan 2025
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.