Role of differential rotation in the solar dynamo
Journal Article
·
· Sov. Astron. AJ (Engl. Transl.); (United States)
OSTI ID:5057469
On the example of the model developed in the authors' previous reports it is shown that compatibility of the theory of the solar magnetic dynamo with observations requires that 1) the angular velocity of the convective shell have a radial gradient and 2) this gradient be negative.
- Research Organization:
- Institute of Applied Mathematics, USSR Academy of Sciences
- OSTI ID:
- 5057469
- Journal Information:
- Sov. Astron. AJ (Engl. Transl.); (United States), Vol. 24:1
- Country of Publication:
- United States
- Language:
- English
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