Torsional Oscillations and Solar Magnetic Fields

Details Torsional Oscillations and Solar Magnetic Fields Torsional Oscillations and Solar Magnetic Fields

Dec 1955

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1955rspsa.233..302l&link_type=abstract

Proceedings of the Royal Society of London. Series A, Mathematical and Physical Sciences, Volume 233, Issue 1194, pp. 302-310

Physics

7

Scientific paper

Torsional magneto-mechanical oscillations of finite amplitude in an idealized non-uniformly rotating star that possesses a poloidal magnetic field are governed, in a first approximation, by a pair of linear wave equations. The approximation is valid if the rotational energy and the magnetic energy are small compared with the gravitational energy. Making various assumptions about the form of the poloidal field, we derive numerical estimates for the period of the fundamental mode (table 1), and discuss the results as they relate to the problem of solar variability.

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