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Convective Plan Form Dynamos in a Layer

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Large-Scale Perturbations of Magnetohydrodynamic Regimes

Part of the book series: Lecture Notes in Physics ((LNP,volume 829))

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Abstract

We have explored in Chaps. 3 and 4 kinematic generation of the large-scale magnetic field by flows with a prescribed energy spectrum, that are synthesised from random-amplitude Fourier harmonics and model turbulent flows. In this chapter, following [1], we consider flows, which are, perhaps, more natural for a physicist and an experimenter—convective plan forms in an infinite horizontal plane layer of fluid. Such flows set in, when the difference of temperatures at the heated lower boundary and the upper boundary exceeds the critical value for the onset of thermal convection. We consider a finite-depth layer of fluid, and hence only horizontal slow variables can be introduced

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Notes

  1. 1.

    Evidently, this symmetry is distinct from axisymmetry.

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Correspondence to Vladislav Zheligovsky .

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© 2011 Springer-Verlag Berlin Heidelberg

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Zheligovsky, V. (2011). Convective Plan Form Dynamos in a Layer. In: Large-Scale Perturbations of Magnetohydrodynamic Regimes. Lecture Notes in Physics, vol 829. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-18170-2_5

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  • DOI: https://doi.org/10.1007/978-3-642-18170-2_5

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-18169-6

  • Online ISBN: 978-3-642-18170-2

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