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: 9,412 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
7,118 2,160 134 9,412 189 241
  • HTML: 7,118
  • PDF: 2,160
  • XML: 134
  • Total: 9,412
  • BibTeX: 189
  • EndNote: 241
Views and downloads (calculated since 05 Aug 2020)
Cumulative views and downloads (calculated since 05 Aug 2020)

Viewed (geographical distribution)

Total article views: 9,412 (including HTML, PDF, and XML) Thereof 9,062 with geography defined and 350 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Saved (final revised paper)

Discussed (final revised paper)

Latest update: 18 Aug 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