A Low-Order Solar Dynamo Model: Inferred Meridional Circulation Variations Since 1750
In this work we present the possible variations that the meridional circulation of the Sun might have undergone during the last 250 years. In order to do this, we reduce an α-Ω dynamo to a low-order system that focuses on the time evolution of one of the solar magnetic field components. Afterward we...
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| Formato: | article |
| Idioma: | eng |
| Publicado em: |
2012
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| Texto completo: | http://hdl.handle.net/10174/5686 |
| País: | Portugal |
| Oai: | oai:dspace.uevora.pt:10174/5686 |