Zonal flows and grand minima in a solar dynamo model

Observations of differential rotation within the solar convection zone have revealed a cyclic pattern of zonal shear flows. Given that the 11-yr periodicity of this flow pattern is approximately half that of the 22-yr solar activity cycle, it is likely that these flows are magnetically driven. In th...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2006-09, Vol.371 (2), p.772-780
1. Verfasser:	Bushby, P. J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Earth, ocean, space Exact sciences and technology Magnetic fields MHD Sun: activity Sun: magnetic fields Sun: rotation Wind shear
Online-Zugang:	Volltext
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