Magnetosheath jets at Mars.


Journal

Science advances
ISSN: 2375-2548
Titre abrégé: Sci Adv
Pays: United States
ID NLM: 101653440

Informations de publication

Date de publication:
02 Jun 2023
Historique:
medline: 2 6 2023
pubmed: 2 6 2023
entrez: 2 6 2023
Statut: ppublish

Résumé

Plasma entities, known as magnetosheath jets, with higher dynamic pressure than the surrounding plasma, are often seen at Earth. They generate waves and contribute to energy transfer in the magnetosheath. Affecting the magnetopause, they cause surface waves and transfer energy into the magnetosphere, causing throat auroras and magnetic signatures detectable on the ground. We show that jets exist also beyond Earth's environment in the magnetosheath of Mars, using data obtained by the MAVEN spacecraft. Thus, jets can be created also at Mars, which differs from Earth by its smaller bow shock, and they are associated with an increased level of magnetic field fluctuations. Jets couple large and small scales in magnetosheaths in the solar system and can play a similar part in astrophysical plasmas.

Identifiants

pubmed: 37267367
doi: 10.1126/sciadv.adg5703
pmc: PMC10413640
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

eadg5703

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Auteurs

Herbert Gunell (H)

Department of Physics, Umeå University, 901 87 Umeå, Sweden.

Maria Hamrin (M)

Department of Physics, Umeå University, 901 87 Umeå, Sweden.

Sara Nesbit-Östman (S)

Department of Physics, Umeå University, 901 87 Umeå, Sweden.

Eva Krämer (E)

Department of Physics, Umeå University, 901 87 Umeå, Sweden.

Hans Nilsson (H)

Swedish Institute of Space Physics, Box 812, 981 28 Kiruna, Sweden.

Classifications MeSH