Articles | Volume 38, issue 4
https://doi.org/10.5194/angeo-38-931-2020
https://doi.org/10.5194/angeo-38-931-2020
Regular paper
 | 
28 Aug 2020
Regular paper |  | 28 Aug 2020

Outer Van Allen belt trapped and precipitating electron flux responses to two interplanetary magnetic clouds of opposite polarity

Harriet George, Emilia Kilpua, Adnane Osmane, Timo Asikainen, Milla M. H. Kalliokoski, Craig J. Rodger, Stepan Dubyagin, and Minna Palmroth

Viewed

Total article views: 2,621 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
2,021 534 66 2,621 67 54
  • HTML: 2,021
  • PDF: 534
  • XML: 66
  • Total: 2,621
  • BibTeX: 67
  • EndNote: 54
Views and downloads (calculated since 15 Apr 2020)
Cumulative views and downloads (calculated since 15 Apr 2020)

Viewed (geographical distribution)

Total article views: 2,621 (including HTML, PDF, and XML) Thereof 2,040 with geography defined and 581 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 20 Nov 2024
Download
Short summary
We compared trapped outer radiation belt electron fluxes to high-latitude precipitating electron fluxes during two interplanetary coronal mass ejections (ICMEs) with opposite magnetic cloud rotation. The electron response had many similarities and differences between the two events, indicating that different acceleration mechanisms acted. Van Allen Probe data were used for trapped electron flux measurements, and Polar Operational Environmental Satellites were used for precipitating flux data.