Toward a dynamo model for the solar tachocline
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...
Guardado en:
| Autores principales: | Lillo, R., Mininni, P.D., Gómez, D.O. |
|---|---|
| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_03784371_v349_n3-4_p667_Lillo |
| Aporte de: |
Ejemplares similares
-
Toward a dynamo model for the solar tachocline
por: Lillo, Rolando Raúl, et al.
Publicado: (2005) -
Large-scale model of the axisymmetric kinematic dynamo
Publicado: (2016) -
Large-scale model of the axisymmetric kinematic dynamo
por: Sraibman, L., et al. -
A new technique for comparing solar dynamo models and observations
por: Mininni, P.D., et al.
Publicado: (2004) -
A new technique for comparing solar dynamo models and observations
por: Mininni, P.D., et al.