Articles | Volume 41, issue 2
https://doi.org/10.5194/angeo-41-551-2023
https://doi.org/10.5194/angeo-41-551-2023
Regular paper
 | 
07 Dec 2023
Regular paper |  | 07 Dec 2023

Local bow shock environment during magnetosheath jet formation: results from a hybrid-Vlasov simulation

Jonas Suni, Minna Palmroth, Lucile Turc, Markus Battarbee, Giulia Cozzani, Maxime Dubart, Urs Ganse, Harriet George, Evgeny Gordeev, Konstantinos Papadakis, Yann Pfau-Kempf, Vertti Tarvus, Fasil Tesema, and Hongyang Zhou

Viewed

Total article views: 894 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
624 203 67 894 54 51
  • HTML: 624
  • PDF: 203
  • XML: 67
  • Total: 894
  • BibTeX: 54
  • EndNote: 51
Views and downloads (calculated since 11 May 2023)
Cumulative views and downloads (calculated since 11 May 2023)

Viewed (geographical distribution)

Total article views: 894 (including HTML, PDF, and XML) Thereof 925 with geography defined and -31 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 12 May 2024
Download
Short summary
Magnetosheath jets are structures of enhanced plasma density and/or velocity in a region of near-Earth space known as the magnetosheath. When they propagate towards the Earth, these jets can disturb the Earth's magnetic field and cause hazards for satellites. In this study, we use a simulation called Vlasiator to model near-Earth space and investigate jets using case studies and statistical analysis. We find that jets that propagate towards the Earth are different from jets that do not.