Articles | Volume 39, issue 1
https://doi.org/10.5194/angeo-39-69-2021
https://doi.org/10.5194/angeo-39-69-2021
Regular paper
 | 
22 Jan 2021
Regular paper |  | 22 Jan 2021

Electron precipitation characteristics during isolated, compound, and multi-night substorm events

Noora Partamies, Fasil Tesema, Emma Bland, Erkka Heino, Hilde Nesse Tyssøy, and Erlend Kallelid

Viewed

Total article views: 2,026 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,466 483 77 2,026 70 64
  • HTML: 1,466
  • PDF: 483
  • XML: 77
  • Total: 2,026
  • BibTeX: 70
  • EndNote: 64
Views and downloads (calculated since 24 Aug 2020)
Cumulative views and downloads (calculated since 24 Aug 2020)

Viewed (geographical distribution)

Total article views: 2,026 (including HTML, PDF, and XML) Thereof 1,852 with geography defined and 174 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 01 Nov 2024
Download
Short summary
About 200 nights of substorm activity have been analysed for their magnetic disturbance magnitude and the level of cosmic radio noise absorption. We show that substorms with a single expansion phase have limited lifetimes and spatial extents. Starting from magnetically quiet conditions, the strongest absorption occurs after 1 to 2 nights of substorm activity. This prolonged activity is thus required to accelerate particles to energies, which may affect the atmospheric chemistry.