How far can minimal models explain the solar cycle?

Details How far can minimal models explain the solar cycle? How far can minimal models explain the solar cycle?

2012-01-30

arxiv.org/abs/1201.6227v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Accepted for publication in the Astrophysical Journal on 2012/01/30

Scientific paper

A physically consistent model of magnetic field generation by convection in a rotating spherical shell with a minimum of parameters is applied to the Sun. Despite its unrealistic features the model exhibits a number of properties resembling those observed on the Sun. The model suggests that the large scale solar dynamo is dominated by a non-axisymmetric $m=1$ component of the magnetic field.

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