Dynamics of Large-Scale Solar Flows

The Sun’s axisymmetric large-scale flows, differential rotation and meridional circulation, are thought to be maintained by the influence of rotation on the thermal-convective motions in the solar convection zone. These large-scale flows are crucial for maintaining the Sun’s global magnetic field. O...

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Detalles Bibliográficos
Autores principales: Hotta, Hideyuki, Bekki, Yuto, Gizon, Laurent, Noraz, Quentin, Rast, Mark
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Netherlands 2023
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10656343/
https://www.ncbi.nlm.nih.gov/pubmed/38023293
http://dx.doi.org/10.1007/s11214-023-01021-6

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10656343/
https://www.ncbi.nlm.nih.gov/pubmed/38023293
http://dx.doi.org/10.1007/s11214-023-01021-6

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