Articles | Volume 41, issue 2
https://doi.org/10.5194/angeo-41-429-2023
https://doi.org/10.5194/angeo-41-429-2023
Regular paper
 | 
02 Nov 2023
Regular paper |  | 02 Nov 2023

Relativistic kinematic effects in the interaction time of whistler-mode chorus waves and electrons in the outer radiation belt

Livia R. Alves, Márcio E. S. Alves, Ligia A. da Silva, Vinicius Deggeroni, Paulo R. Jauer, and David G. Sibeck

Viewed

Total article views: 1,079 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
749 264 66 1,079 42 51
  • HTML: 749
  • PDF: 264
  • XML: 66
  • Total: 1,079
  • BibTeX: 42
  • EndNote: 51
Views and downloads (calculated since 28 Feb 2023)
Cumulative views and downloads (calculated since 28 Feb 2023)

Viewed (geographical distribution)

Total article views: 1,079 (including HTML, PDF, and XML) Thereof 1,076 with geography defined and 3 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 01 Nov 2024
Download
Short summary
We derive the wave–particle interaction time (IT) equation considering the effects of special relativity theory for whistler-mode chorus waves and relativistic electrons in Earth's radiation belt. Results show that IT has a non-linear dependence on the wave group velocity, electrons' energy, and initial pitch angle. Our results show that the interaction time is generally longer when applying the complete relativistic approach compared to a non-relativistic calculation.