MAGNETOHYDRODYNAMIC DYNAMOS IN THE PRESENCE OF FOSSIL MAGNETIC FIELDS.
A fossil magnetic field embedded in the radiative core of the Sun has been thought possible for some time now. However, such a fossil magnetic field has, a priori, not been considered a visible phenomenon due to the effects of turbulence in the solar convection zone. Since a well developed theory (r...
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| Language: | en |
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The University of Arizona.
1982
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| Online Access: | http://hdl.handle.net/10150/185249 |