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

Data sets

Vlasov methods in space physics and astrophysics M. Palmroth, U. Ganse, Y. Pfau-Kempf, M. Battarbee, L. Turc, T. Brito, M. Grandin, S. Hoilijoki, A. Sandroos, and S. von Alfthan https://doi.org/10.1007/s41115-018-0003-2

Vlasiator M. Palmroth http://helsinki.fi/vlasiator/

Model code and software

VLSV: file format and tools A. Sandroos https://github.com/fmihpc/vlsv/

Analysator: python analysis toolkit O. Hannuksela and the Vlasiator team https://github.com/fmihpc/analysator/

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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.