Quenching of zonal winds in Jupiter's interior.
Jupiter
interior dynamics
magnetohydrodynamics
Journal
Proceedings of the National Academy of Sciences of the United States of America
ISSN: 1091-6490
Titre abrégé: Proc Natl Acad Sci U S A
Pays: United States
ID NLM: 7505876
Informations de publication
Date de publication:
18 Jun 2024
18 Jun 2024
Historique:
medline:
10
6
2024
pubmed:
10
6
2024
entrez:
10
6
2024
Statut:
ppublish
Résumé
Gravity and magnetic field data obtained by the Juno mission show that Jupiter's strong zonal winds extend a few thousand kilometers into the interior, but are quenched above the level where the electrical conductivity becomes significant. Here, we extend a simple linearized model [Christensen et al.,
Identifiants
pubmed: 38857406
doi: 10.1073/pnas.2402859121
doi:
Types de publication
Journal Article
Langues
eng
Sous-ensembles de citation
IM
Pagination
e2402859121Subventions
Organisme : EPSRC
ID : EP/R014604/1
Déclaration de conflit d'intérêts
Competing interests statement:The authors declare no competing interest.