A new model of the solar cycle

Details A new model of the solar cycle A new model of the solar cycle

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.278..294k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 278, Issue 1, pp. 294-302.

Astronomy and Astrophysics

Astronomy

47

Sun: Activity, Sun: Magnetic Fields, Sun: Rotation, Sunspots

Scientific paper

A new model of the solar magnetic activity cycle is proposed. The model is based on the symmetries of a rotating star, and describes the interaction between dipole and quadrupole fields in the weakly non-linear regime. The model describes not only pure dipole and quadrupole dynamos, but also the transitions with increasing dynamo number to mixed polarity states, and in appropriate regimes to aperiodic states which are highly suggestive of prolonged activity minima such as the Maunder minimum.

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