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Cyclic Evolution of Coronal Fields from a Coupled Dynamo Potential-Field Source-Surface Model
The structure of the Sun’s corona varies with the solar-cycle phase, from a near spherical symmetry at solar maximum to an axial dipole at solar minimum. It is widely accepted that the large-scale coronal structure is governed by magnetic fields that are most likely generated by dynamo action in the...
| Autores principales: | , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Springer Netherlands
2015
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4938017/ https://www.ncbi.nlm.nih.gov/pubmed/27445420 http://dx.doi.org/10.1007/s11207-015-0831-8 |