On the non-symmetric solar dynamo

Details On the non-symmetric solar dynamo On the non-symmetric solar dynamo

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...74..103c&link_type=abstract

(ESA and European Physical Society, ESLAB Symposium on Physics of Solar Variations, 14th, Scheveningen, Netherlands, Sept. 16-19

Physics

1

Dynamo Theory, Magnetohydrodynamics, Solar Magnetic Field, Solar Physics, Solar Corona, Solar Oscillations, Spherical Harmonics, Tensor Analysis

Scientific paper

The external field of the solar magnetohydrodynamic dynamo is expressed in terms of spherical harmonics and in powers of 1/r. The non-symmetric dynamo is stabilized by a phi-dependent rotational oscillation which interacts with the magnetic field, thus compensating for Ohmic loss. As a consequence, the axis of a dipole wave is found to move on a great circle, with revolution time equal to the magnetic cycle.

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