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Possible explanations of the Maunder minimum from a flux transport dynamo model
Published 23 Jan 2011 in astro-ph.SR, astro-ph.EP, and astro-ph.HE | (1101.4342v1)
Abstract: We propose that at the beginning of the Maunder minimum the poloidal field or amplitude of meridional circulation or both fell abruptly to low values. With this proposition, a flux transport dynamo model is able to reproduce various important aspects of the historical records of the Maunder minimum remarkably well.
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