Solar neutrinos, sunspot number and the magnetic field in the convective zone
โ Scribed by G. Fiorentini; G. Mezzorani
- Book ID
- 113359936
- Publisher
- Elsevier Science
- Year
- 1991
- Tongue
- English
- Weight
- 270 KB
- Volume
- 253
- Category
- Article
- ISSN
- 0370-2693
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
Magnetic buoyancy is thought to play an important role in the dynamical behavior of the Sun's magnetic field in the convection zone. Magnetic buoyancy is commonly thought to cause inescapable rapid loss of toroidal flux from much of the convection zone, thereby suppressing effective operation of a s
Observations demonstrate a nearly 22-year periodic zonal flow superimposed on general solar differential rotation (LaBonte and Howard, 1982) and some meridional motions (e.g., Tuominen, Tuominen, and Kyrol~inen, 1983). Such flows can be excited by the magnetic wave generated by the dynamo in the sol