The Structure of the Large-Scale Heliosphere as Seen by Current Models.
Analytical
Heliosphere
Modeling
Numerical
Journal
Space science reviews
ISSN: 0038-6308
Titre abrégé: Space Sci Rev
Pays: Netherlands
ID NLM: 100971458
Informations de publication
Date de publication:
2022
2022
Historique:
received:
02
02
2022
accepted:
06
05
2022
entrez:
6
6
2022
pubmed:
7
6
2022
medline:
7
6
2022
Statut:
ppublish
Résumé
This review summarizes the current state of research aiming at a description of the global heliosphere using both analytical and numerical modeling efforts, particularly in view of the overall plasma/neutral flow and magnetic field structure, and its relation to energetic neutral atoms. Being part of a larger volume on current heliospheric research, it also lays out a number of key concepts and describes several classic, though still relevant early works on the topic. Regarding numerical simulations, emphasis is put on magnetohydrodynamic (MHD), multi-fluid, kinetic-MHD, and hybrid modeling frameworks. Finally, open issues relating to the physical relevance of so-called "croissant" models of the heliosphere, as well as the general (dis)agreement of model predictions with observations are highlighted and critically discussed.
Identifiants
pubmed: 35664863
doi: 10.1007/s11214-022-00902-6
pii: 902
pmc: PMC9156516
doi:
Types de publication
Journal Article
Review
Langues
eng
Pagination
36Informations de copyright
© The Author(s) 2022.
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