Annales Geophysicae
Annales Geophysicae
ANGEO
Articles | Volume 35, issue 4
Articles | Volume 35, issue 4
https://doi.org/10.5194/angeo-35-965-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-35-965-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
Articles | Volume 35, issue 4
Regular paper
 | Highlight paper
 | 
21 Aug 2017
Regular paper | Highlight paper |  | 21 Aug 2017

The electric current approach in the solar–terrestrial relationship

Syun-Ichi Akasofu

Viewed

Total article views: 2,322 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,607 636 79 2,322 58 64
  • HTML: 1,607
  • PDF: 636
  • XML: 79
  • Total: 2,322
  • BibTeX: 58
  • EndNote: 64
Views and downloads (calculated since 21 Aug 2017)
Cumulative views and downloads (calculated since 21 Aug 2017)

Cited

Latest update: 23 Apr 2024
Download
Short summary
The sequence of phenomena consisting of solar flares, coronal mass ejections (CMEs), auroral substorm, and geomagnetic storms is mostly a manifestation of electromagnetic energy dissipation. Thus, first of all, it is natural to consider each of them in terms of a sequence of power supply (dynamo), power transmission (electric currents/circuits), and dissipation (mostly observed phenomena), i.e., as an input–output process and the electric current line approach.
Read more