Magnetic field transfer by two-dimensional convection and solar 'semi- dynamo'

DOI10.1007/BF00643752zbMath0355.76076MaRDI QIDQ1237422

E. M. Drobyshevski

Publication date: 1977

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Diffusion and convection (76R99)

Related Items (5)

New form of dynamo equation for convective regions of rotating stars ⋮ Magnetic-flux transport by a convecting layer – topological, geometrical and compressible phenomena ⋮ The macroscopic magnetohydrodynamics of inhomogeneously turbulent cosmic plasmas ⋮ Topological semi-dynamos ⋮ The rate of magnetic field penetration through a Bénard convection layer

Cites Work

• Topological pumping of magnetic flux by three-dimensional convection

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