The decay of torque free toroidal magnetic fields confined beneath the solar convection zone
β Scribed by David Moss
- Publisher
- Springer Netherlands
- Year
- 1984
- Tongue
- English
- Weight
- 218 KB
- Volume
- 104
- Category
- Article
- ISSN
- 0004-640X
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π 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
Doing numerical calculations of axially symmetric force-flee fields, have noticed that there seem to be no solutions if the toroidal component of the field exceeds a certain limit. In the present paper this problem is reexamined in the approximation of a plane stellar surface using a very simple an