Impact of a Realistic Density Stratification on a Simple Solar Dynamo Calculation
In our Sun, the magnetic cycle is driven by the dynamo action occurring inside the convection zone, beneath the surface. Rotation couples with plasma turbulent motions to produce organized magnetic fields that erupt at the surface and undergo relatively regular cycles of polarity reversal. Among oth...
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| Formato: | article |
| Idioma: | eng |
| Publicado em: |
2013
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| Texto completo: | http://hdl.handle.net/10174/7418 |
| País: | Portugal |
| Oai: | oai:dspace.uevora.pt:10174/7418 |