The magnetic field pattern associated with large scale convective motions, which are much larger than the supergranules and have been conceived as a source of maintenance of the solar differential rotation, is calculated in the framework Of a slowly and differentially rotating thin spherical shell,
Thickness of the dry convection and large-scale subsidence above deserts
β Scribed by M. Gamo
- Publisher
- Springer
- Year
- 1996
- Tongue
- English
- Weight
- 934 KB
- Volume
- 79
- Category
- Article
- ISSN
- 0006-8314
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