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
Propagation of a dynamo field in the radiative interior of the Sun
โ Scribed by P. Garaud
- Publisher
- John Wiley and Sons
- Year
- 1999
- Tongue
- English
- Weight
- 211 KB
- Volume
- 304
- Category
- Article
- ISSN
- 0035-8711
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