Thin-Shell Magnetohydrodynamic Equations for the Solar Tachocline
β Scribed by Mark S. Miesch; Peter A. Gilman
- Book ID
- 111611950
- Publisher
- Springer
- Year
- 2004
- Tongue
- English
- Weight
- 141 KB
- Volume
- 220
- Category
- Article
- ISSN
- 0038-0938
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π SIMILAR VOLUMES
The generation of magnetic field on the Sun is caused by a dynamo mechanism, and is related with the differential rotation of the solar interior. Helioseismologic observations show that strong velocity gradients concentrate in a thin layer located at the base of the convective region, known as the t
Variational equations are derived for thin elastic shells of arbitrary geometry from their related non-linear modal equations, The advantages of this procedure compared to methods commonly used in engineering applications are discussed. Numerical calculations are carried out for a simply supported c