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The magnetic field transfer in the solar convective zone

โœ Scribed by A. A. Ruzmaikin; S. I. Vainshtein

Publisher
Springer Netherlands
Year
1978
Tongue
English
Weight
352 KB
Volume
57
Category
Article
ISSN
0004-640X

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๐Ÿ“œ SIMILAR VOLUMES

Dynamical behavior of strong magnetic fi
Dynamical behavior of strong magnetic fields in the solar convection zone
โœ S. Vainshtein; E. H. Levy ๐Ÿ“‚ Article ๐Ÿ“… 1991 ๐Ÿ› Springer ๐ŸŒ English โš– 644 KB

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

Large-scale flows excited by magnetic fi
Large-scale flows excited by magnetic fields in the solar convective zone
โœ N. I. Kleeorin; A. A. Ruzmaikin ๐Ÿ“‚ Article ๐Ÿ“… 1991 ๐Ÿ› Springer ๐ŸŒ English โš– 941 KB

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