## Abstract The motivation for considering distributed large scale dynamos in the solar context is reviewed in connection with the magnetic helicity constraint. Preliminary accounts of 3βdimensional direct numerical simulations (in spherical shell segments) and simulations of 2βdimensional mean fie
Cellular dynamo in a rotating spherical shell
β Scribed by A. V. Getling; R. D. Simitev; F. H. Busse
- Publisher
- John Wiley and Sons
- Year
- 2005
- Tongue
- English
- Weight
- 261 KB
- Volume
- 326
- Category
- Article
- ISSN
- 0004-6337
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