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

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Latest update: 20 Nov 2024
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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.