Commentary on a putative magnetic field variation in the solar convection zone
โ Scribed by Gough, D. O.
- Book ID
- 126819074
- Publisher
- John Wiley and Sons
- Year
- 2013
- Tongue
- English
- Weight
- 401 KB
- Volume
- 435
- Category
- Article
- ISSN
- 0035-8711
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