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arxiv: astro-ph/0609752 · v1 · submitted 2006-09-27 · 🌌 astro-ph

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Mean-field concept and direct numerical simulations of rotating magnetoconvection and the geodynamo

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classification 🌌 astro-ph
keywords directmean-fieldnumericalsimulationsgeodynamomagneticmagnetoconvectionmodels
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A comparison is made between mean-field models and direct numerical simulations of rotating magnetoconvection and the geodynamo. The mean-field coefficients are calculated with the fluid velocity taken from the direct numerical simulations. The magnetic fields resulting from mean-field models are then compared with the mean magnetic field from the direct numerical simulations.

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Cited by 1 Pith paper

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  1. Stochastic Resonance in a Thermally Driven Low-Dimensional Geodynamo Model

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    Slow periodic modulation of the alpha-effect in a low-dimensional thermally driven geodynamo model creates a multi-peaked distribution of magnetic polarity persistence times at integer multiples of the modulation timescale.