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
β¦ LIBER β¦
Erratum: Towards a model for the solar dynamo
β Scribed by David Moss; John Brooke
- Publisher
- John Wiley and Sons
- Year
- 2001
- Tongue
- English
- Weight
- 25 KB
- Volume
- 322
- Category
- Article
- ISSN
- 0035-8711
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