Annales Geophysicae
Annales Geophysicae
ANGEO
Articles | Volume 44, issue 1
Articles | Volume 44, issue 1
https://doi.org/10.5194/angeo-44-47-2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/angeo-44-47-2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Articles | Volume 44, issue 1
Regular paper
 | 
30 Jan 2026
Regular paper |  | 30 Jan 2026

Solar wind driving of the auroral outflow during the 23–26 September 1998 storm

Kai Zhao, Lynn M. Kistler, Eric J. Lund, Niloufar Nowrouzi, Christopher G. Mouikis, and Naritoshi Kitamura

Viewed

Total article views: 3,413 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
2,771 528 114 3,413 141 207
  • HTML: 2,771
  • PDF: 528
  • XML: 114
  • Total: 3,413
  • BibTeX: 141
  • EndNote: 207
Views and downloads (calculated since 25 Feb 2025)
Cumulative views and downloads (calculated since 25 Feb 2025)

Viewed (geographical distribution)

Total article views: 3,413 (including HTML, PDF, and XML) Thereof 3,413 with geography defined and 0 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 06 Jun 2026
Download
Short summary
This study utilizes data from the FAST spacecraft orbiting over the auroral regions to investigate the temporal progression of energy inputs resulting from a Coronal Mass Ejection (CME) and how that energy increases the outflow of ionospheric plasma. We found that the various forms of energy are all enhanced during the initial phase of a storm, and the energy inputs are strongly correlated with the solar wind-magnetosphere coupling functions, especially in the dayside cusp region.
Read more
Share