Solar Variability Induced in a Dynamo Code by Realistic Meridional Circulation Variations
In this work we use an already-published method to infer a variation profile for the solar meridional circulation over the last 250 years. We feed this variation profile into a numerical dynamo code, and we reconstruct a sunspot time series that acts as a proxy for solar cycle activity. We perform t...
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| Formato: | article |
| Idioma: | eng |
| Publicado em: |
2012
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| Texto completo: | http://hdl.handle.net/10174/5688 |
| País: | Portugal |
| Oai: | oai:dspace.uevora.pt:10174/5688 |