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Study of surface convective zone behavior of solar pond in laboratory

โœ Scribed by Renyuan Zhang; C.E. Nielsen


Publisher
Elsevier Science
Year
1994
Tongue
English
Weight
297 KB
Volume
4
Category
Article
ISSN
0960-1481

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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