Non-linear alpha-omega-dynamos driven by magnetic buoyancy
An alpha-omega-dynamo with an alpha-effect based on magnetic buoyancy instabilities is described. This alpha-effect has one main advantage over previous descriptions, namely, that it is derived from a numerical model of the physical processes that are thought to occur at the base of the convection z...
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| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2000-06, Vol.315 (1), p.165-183 |
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| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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