Limits on the magnetic field strength at the base of the solar convection zone
โ Scribed by Sydney D'Silva; Robert F. Howard
- Publisher
- Springer
- Year
- 1993
- Tongue
- English
- Weight
- 439 KB
- Volume
- 148
- Category
- Article
- ISSN
- 0038-0938
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๐ SIMILAR VOLUMES
Magnetic buoyancy is thought to play an important role in the dynamical behavior of the Sun's magnetic field in the convection zone. Magnetic buoyancy is commonly thought to cause inescapable rapid loss of toroidal flux from much of the convection zone, thereby suppressing effective operation of a s
Observations demonstrate a nearly 22-year periodic zonal flow superimposed on general solar differential rotation (LaBonte and Howard, 1982) and some meridional motions (e.g., Tuominen, Tuominen, and Kyrol~inen, 1983). Such flows can be excited by the magnetic wave generated by the dynamo in the sol