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Mean-Field Magnetohydrodynamics of the Solar Convection Zone

Published online by Cambridge University Press:  14 August 2015

F. Krause
F. Krause*
Affiliation:
Zentralinstitut für Astrophysik, Potsdam, G.D.R.

Extract

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Observations of the solar surface show that some of the physical quantities, especially the velocity field and the magnetic field, show random character.

Type
Part 3: Dynamo Theory and Magnetic Dissipation
Information
Symposium - International Astronomical Union , Volume 71: Basic Mechanisms of Solar Activity , 1976 , pp. 305 - 321
Copyright
Copyright © Reidel 1976 

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