The tachocline and the solar dynamo
β Scribed by P. A. Gilman
- Publisher
- John Wiley and Sons
- Year
- 2005
- Tongue
- English
- Weight
- 694 KB
- Volume
- 326
- Category
- Article
- ISSN
- 0004-6337
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
## Abstract Most probably the sunspot cycle period is ruled by a meridional flow located near the base of the convection zone (Hathaway et al. 2003). On the other hand, if the eddy diffusivity is low enough, dramatic modification of the standard __Ξ±__ ^2^__Ξ©__ βdynamo by the meridional flow are exp
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