New form of dynamo equation for convective regions of rotating stars

DOI10.1007/BF00642961zbMath0850.76835OpenAlexW2080405697MaRDI QIDQ1186755

Gennady S. Bisnovatyi-Kogan

Publication date: 28 June 1992

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

Full work available at URL: https://doi.org/10.1007/bf00642961

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Cites Work

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

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