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Generation of a magnetic field by the convective zones of hot stars

โœ Scribed by E. M. Drobyshevskii


Publisher
Springer
Year
1970
Tongue
English
Weight
556 KB
Volume
4
Category
Article
ISSN
0571-7256

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Dynamical behavior of strong magnetic fi
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