Comparison of Stellar Oscillations and Activity Data to Infer Internal Rotation
Recently it has beeen suggested that the latitude distribution of the main surface features of solar activity is intimately related to the angular velocity profile inside the Sun through the working of a MHD dynamo in the boundary layer between the convective and the radiative zones (Belvedere et al...
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| Veröffentlicht in: | International Astronomical Union Colloquium 1993, Vol.137, p.675-678 |
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| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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