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A Dynamo Model for the Large Scale Fields
Published online by Cambridge University Press: 14 August 2015
Abstract
The expansion of the magnetic field in a series of force-free constituents for the internal field and that of ‘semi’ force-free constituents for the external field results in the skew symmetry of the coupling tensor of a magnetohydrodynamic dynamo. The periodic solution which exists in this case is deduced by the method of eigenvalues. Based on the numerical results a dynamo model is proposed to draw up the characteristic features of the magnetographic observations carried along the central meridian and at the polar areas.
- Type
- Part VIII: Theories of Large Scale Fields and the Activity Cycle
- Information
- Symposium - International Astronomical Union , Volume 43: Solar Magnetic Fields , 1971 , pp. 780 - 782
- Copyright
- Copyright © Reidel 1971