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Chaotic behavior in stellar dynamos
Authors:N O Weiss
Institution:(1) Department of Applied Mathematics and Theoretical Physics, University of Cambridge, CB3 9EW, England
Abstract:Slowly rotating main-sequence stars with deep convective zones have activity cycles like the sun's. The solar cycle is aperiodic and modulated to give intervals of reduced activity. A simple sixth-order system, obtained by truncating the dynamo equations, has solutions that mimic this behavior. The transition to chaos is analyzed and the astrophysical significance of these results is discussed.
Keywords:Solar activity  magnetic cycles  dynamos  chaos
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