The problem of the interaction between magnetic fields and differential rotation in the radiative zone of the Sun is investigated. It is demonstrated that effects of magnetic buoyancy can be neglected in the analysis of this interaction. It is shown that hydromagnetic torsional waves propagating fro
โฆ LIBER โฆ
Differential rotation and magnetic torques in the interior of the Sun
โ Scribed by Rosner, R.; Weiss, N. O.
- Book ID
- 109741667
- Publisher
- Nature Publishing Group
- Year
- 1985
- Tongue
- English
- Weight
- 371 KB
- Volume
- 317
- Category
- Article
- ISSN
- 0028-0836
- DOI
- 10.1038/317790a0
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It is presumed that a north-southern asymmetry of a solid-body rotation of large spots, depending on even and odd solar activity cycles (Gigolashvili and Khutsishvilil 1989, 1990) may possibly be explained by the asymmetry of the appearance of large structures with strong magnetic fields in the corr