Articles | Volume 42, issue 2
https://doi.org/10.5194/angeo-42-355-2024
https://doi.org/10.5194/angeo-42-355-2024
Regular paper
 | 
06 Sep 2024
Regular paper |  | 06 Sep 2024

Statistical comparison of electron precipitation during auroral breakups occurring either near the open–closed field line boundary or in the central part of the auroral oval

Maxime Grandin, Noora Partamies, and Ilkka I. Virtanen

Viewed

Total article views: 538 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
352 109 77 538 17 15
  • HTML: 352
  • PDF: 109
  • XML: 77
  • Total: 538
  • BibTeX: 17
  • EndNote: 15
Views and downloads (calculated since 20 Feb 2024)
Cumulative views and downloads (calculated since 20 Feb 2024)

Viewed (geographical distribution)

Total article views: 538 (including HTML, PDF, and XML) Thereof 523 with geography defined and 15 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 06 Oct 2024
Download
Short summary
Auroral displays typically take place at high latitudes, but the exact latitude where the auroral breakup occurs can vary. In this study, we compare the characteristics of the fluxes of precipitating electrons from space during auroral breakups occurring above Tromsø (central part of the auroral zone) and above Svalbard (poleward boundary of the auroral zone). We find that electrons responsible for the aurora above Tromsø carry more energy than those precipitating above Svalbard.