Articles | Volume 40, issue 3
https://doi.org/10.5194/angeo-40-315-2022
https://doi.org/10.5194/angeo-40-315-2022
Regular paper
 | 
31 May 2022
Regular paper |  | 31 May 2022

Fine structure and motion of the bow shock and particle energisation mechanisms inferred from Magnetospheric Multiscale (MMS) observations

Krzysztof Stasiewicz and Zbigniew Kłos

Viewed

Total article views: 2,234 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,649 504 81 2,234 51 45
  • HTML: 1,649
  • PDF: 504
  • XML: 81
  • Total: 2,234
  • BibTeX: 51
  • EndNote: 45
Views and downloads (calculated since 21 Jan 2022)
Cumulative views and downloads (calculated since 21 Jan 2022)

Viewed (geographical distribution)

Total article views: 2,234 (including HTML, PDF, and XML) Thereof 2,130 with geography defined and 104 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 21 Nov 2024
Download
Short summary
The acceleration, or energisation, of particles is a common and fundamental process throughout the universe. This study presents new observations of the acceleration of protons by waves at the bow shock upstream of the Earth, where the solar wind first encounters Earth’s magnetic field. The results are important, because they provide insight into acceleration processes that can create high-energy particles both near the Earth and at other astrophysical systems.