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- W1976576670 abstract "We examine a pair of radially averaged, pseudo-Cartesian dynamo models, one with a dynamically variable α effect, and the other with a dynamically variable ω effect. Our models are kept deliberately minimal in order to permit extensive numerical analysis, including in particular direct solution of periodic orbits and continuation of unstable branches. Despite some differences in the formulations used, the bifurcation structure of the variable-ω model is found to resemble closely that computed by Jennings & Weiss, whereas that of the variable-α model matches the structure computed by Schmalz & Stix somewhat less well. Our two systems, however, resemble each other not at all, despite having the same linearized form. Quenching of the α and co effects is confirmed to have dramatically different effects, with ω-quenching perhaps producing better resemblance to the Sun. Also, we find the variable-α model to contain periodic solutions for positive dynamo number that do not show poleward propagation, contrary to conventional wisdom." @default.
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- W1976576670 date "1997-07-01" @default.
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- W1976576670 title "Simple solar dynamo models with variable and effects" @default.
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- W1976576670 doi "https://doi.org/10.1093/mnras/288.3.551" @default.
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