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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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| Publicat a: | Sci Adv |
|---|---|
| Autors principals: | , , , , , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
American Association for the Advancement of Science
2016
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| Matèries: | |
| Accés en línia: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4956390/ https://ncbi.nlm.nih.gov/pubmed/27453947 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1126/sciadv.1600557 |
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