Articles | Volume 40, issue 1
https://doi.org/10.5194/angeo-40-1-2022
https://doi.org/10.5194/angeo-40-1-2022
Regular paper
 | 
04 Jan 2022
Regular paper |  | 04 Jan 2022

Types of pulsating aurora: comparison of model and EISCAT electron density observations

Fasil Tesema, Noora Partamies, Daniel K. Whiter, and Yasunobu Ogawa

Viewed

Total article views: 2,771 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
2,032 636 103 2,771 95 78
  • HTML: 2,032
  • PDF: 636
  • XML: 103
  • Total: 2,771
  • BibTeX: 95
  • EndNote: 78
Views and downloads (calculated since 29 Mar 2021)
Cumulative views and downloads (calculated since 29 Mar 2021)

Viewed (geographical distribution)

Total article views: 2,771 (including HTML, PDF, and XML) Thereof 2,665 with geography defined and 106 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Discussed (final revised paper)

Latest update: 13 Dec 2024
Download
Short summary
In this study, we present the comparison between an auroral model and EISCAT radar electron densities during pulsating aurorae. We test whether an overpassing satellite measurement of the average energy spectrum is a reasonable estimate for pulsating aurora electron precipitation. When patchy pulsating aurora is dominant in the morning sector, the overpass-averaged spectrum is found to be a reasonable estimate – but not when there is a mix of pulsating aurora types in the post-midnight sector.