Articles | Volume 36, issue 5
https://doi.org/10.5194/angeo-36-1171-2018
https://doi.org/10.5194/angeo-36-1171-2018
Regular paper
 | 
07 Sep 2018
Regular paper |  | 07 Sep 2018

Magnetosheath jet properties and evolution as determined by a global hybrid-Vlasov simulation

Minna Palmroth, Heli Hietala, Ferdinand Plaschke, Martin Archer, Tomas Karlsson, Xóchitl Blanco-Cano, David Sibeck, Primož Kajdič, Urs Ganse, Yann Pfau-Kempf, Markus Battarbee, and Lucile Turc

Viewed

Total article views: 2,923 (including HTML, PDF, and XML)
HTML PDF XML Total Supplement BibTeX EndNote
2,072 782 69 2,923 297 88 73
  • HTML: 2,072
  • PDF: 782
  • XML: 69
  • Total: 2,923
  • Supplement: 297
  • BibTeX: 88
  • EndNote: 73
Views and downloads (calculated since 08 Mar 2018)
Cumulative views and downloads (calculated since 08 Mar 2018)

Viewed (geographical distribution)

Total article views: 2,923 (including HTML, PDF, and XML) Thereof 2,755 with geography defined and 168 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 20 Nov 2024
Download
Short summary
Magnetosheath jets are high-velocity plasma structures that are commonly observed within the Earth's magnetosheath. Previously, they have mainly been investigated with spacecraft observations, which do not allow us to infer their spatial sizes, temporal evolution, or origin. This paper shows for the first time their dimensions, evolution, and origins within a simulation whose dimensions are directly comparable to the Earth's magnetosphere. The results are compared to previous observations.