Topological semi-dynamos
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Publication:3336971
DOI10.1080/03091928308221743zbMath0546.76136OpenAlexW2039400242WikidataQ114640575 ScholiaQ114640575MaRDI QIDQ3336971
E. N. Kolesnikova, E. M. Drobyshevski, V. S. Yuferev
Publication date: 1983
Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1080/03091928308221743
continuous mediumazimuthal Coriolisfield generationquasi-steady magnetic field of the Sunthree-dimensional Bénard convection layertopological pumping effectwithout self-excitation
Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)
Cites Work
- Unnamed Item
- Magnetic field transfer by two-dimensional convection and solar 'semi- dynamo'
- The amplification of a weak applied magnetic field by turbulence in fluids of moderate conductivity
- The rate of magnetic field penetration through a Bénard convection layer
- Generation of Magnetic Fields by Fluid Motion
- Topological pumping of magnetic flux by three-dimensional convection
- On the spontaneous magnetic field in a conducting liquid in turbulent motion
- Entstehung von Magnetfeldern in bewegten Plasmen
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