Dynamical behavior of strong magnetic fi
β
S. Vainshtein; E. H. Levy
π
Article
π
1991
π
Springer
π
English
β 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