Chaotic behavior in stellar dynamos

Details Chaotic behavior in stellar dynamos Chaotic behavior in stellar dynamos

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985jsp....39..477w&link_type=abstract

Journal of Statistical Physics, Volume 39, Issue 5-6, pp. 477-491

Physics

9

Solar Activity, Magnetic Cycles, Dynamos, Chaos

Scientific paper

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.

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