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Observations of the Sun and solar-type stars continue to reveal phenomenawhose understanding is very likely to require a nonlinear framework. Here weshall concentrate on two such phenomena, namely the grand minima type behaviourobserved in the Sun and solar-type stars and the recent dynamical variations ofthe differential rotation in the solar convection zone, deduced from thehelioseismic observations, and discuss how their explanations have recentlymotivated the development/employment of novel ideas from nonlinear dynamics.

Aspects of the Dynamics Underlying Solar and Stellar Dynamo Models