Articles | Volume 39, issue 2
https://doi.org/10.5194/angeo-39-277-2021
https://doi.org/10.5194/angeo-39-277-2021
Regular paper
 | Highlight paper
 | 
04 Mar 2021
Regular paper | Highlight paper |  | 04 Mar 2021

Characteristics of fragmented aurora-like emissions (FAEs) observed on Svalbard

Joshua Dreyer, Noora Partamies, Daniel Whiter, Pål G. Ellingsen, Lisa Baddeley, and Stephan C. Buchert

Viewed

Total article views: 8,121 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
6,253 1,752 116 8,121 154 207
  • HTML: 6,253
  • PDF: 1,752
  • XML: 116
  • Total: 8,121
  • BibTeX: 154
  • EndNote: 207
Views and downloads (calculated since 05 Aug 2020)
Cumulative views and downloads (calculated since 05 Aug 2020)

Viewed (geographical distribution)

Total article views: 8,121 (including HTML, PDF, and XML) Thereof 7,854 with geography defined and 267 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 09 Feb 2026
Download
Short summary
Small-scale auroral features are still being discovered and are not well understood. Where aurorae are caused by particle precipitation, the newly reported fragmented aurora-like emissions (FAEs) seem to be locally generated in the ionosphere (hence, aurora-like). We analyse data from multiple instruments located near Longyearbyen to derive their main characteristics. They seem to occur as two types in a narrow altitude region (individually or in regularly spaced groups).
Share