On the non-symmetric solar dynamo

descriptionPublicationkeyboard_double_arrow_right Article , Part of book or chapter of book 01 Jan 1981 English Publisher:Springer Science and Business Media LLCJournal:Solar Physics, volume 74, pages 103-105 (issn: 0038-0938, eissn: 1573-093X,

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Authors: I. K. Csada;

doi: 10.1007/bf00151278 , 10.1007/978-94-010-9633-1_12

On the non-symmetric solar dynamo

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Abstract

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 φ -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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Konkoly Thege Miklós Astronomical Institute
Hungary

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