𝔖 Bobbio Scriptorium
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Solar magnetic fields and convection

✍ Scribed by J. H. Piddington


Publisher
Springer Netherlands
Year
1975
Tongue
English
Weight
635 KB
Volume
38
Category
Article
ISSN
0004-640X

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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