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Transactions of the International Astronomical Union, 1988
Traditionally the theory of the solar dynamo has been divided into two parts. The first, more difficult part, is the derivation of equations governing the mean magnetic field; the second, easier, is the solution of this equation, and the interpretation of the result in terms of observed solar magnetism. This report follows the traditional division.
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Traditionally the theory of the solar dynamo has been divided into two parts. The first, more difficult part, is the derivation of equations governing the mean magnetic field; the second, easier, is the solution of this equation, and the interpretation of the result in terms of observed solar magnetism. This report follows the traditional division.
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1997
The solar dynamo problem is reviewed in the light of recent developments in dynamo theory. We distinguish between the generation of magnetic fields on scales smaller than the velocity correlation length-small scale dynamo, and larger than the velocity correlation length-large scale dynamo.
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The solar dynamo problem is reviewed in the light of recent developments in dynamo theory. We distinguish between the generation of magnetic fields on scales smaller than the velocity correlation length-small scale dynamo, and larger than the velocity correlation length-large scale dynamo.
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Observationally Guided Models for the Solar Dynamo and the Role of the Surface Field
Space Science Reviews, 2023Robert H Cameron, Manfred Schuessler
exaly
Evolution of Solar and Stellar Dynamo Theory
Space Science Reviews, 2023Paul Charbonneau, Dmitry Sokolov
exaly
Starspots, stellar cycles and stellar flares: Lessons from solar dynamo models
Science China: Physics, Mechanics and Astronomy, 2016Arnab Rai Choudhuri
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