A low upper limit on the subsurface rise speed of solar active regions

Magnetic field emerges at the surface of the Sun as sunspots and active regions. This process generates a poloidal magnetic field from a rising toroidal flux tube; it is a crucial but poorly understood aspect of the solar dynamo. The emergence of magnetic field is also important because it is a key...

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Detalles Bibliográficos
Autores principales: Birch, Aaron C., Schunker, Hannah, Braun, Douglas C., Cameron, Robert, Gizon, Laurent, Löptien, Björn, Rempel, Matthias
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Association for the Advancement of Science 2016
Materias:
Research Articles
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4956390/
https://www.ncbi.nlm.nih.gov/pubmed/27453947
http://dx.doi.org/10.1126/sciadv.1600557

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4956390/
https://www.ncbi.nlm.nih.gov/pubmed/27453947
http://dx.doi.org/10.1126/sciadv.1600557

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