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Scaling behaviour of small-scale dynamos driven by Rayleigh–Bénard convection
Published online by Cambridge University Press: 09 March 2021
Abstract
A numerical investigation of convection-driven dynamos is carried out in the plane layer geometry. Dynamos with different magnetic Prandtl numbers $Pm$ are simulated over a broad range of the Rayleigh number
$Ra$. The heat transport, as characterized by the Nusselt number
$Nu$, shows an initial departure from the heat transport scaling of non-magnetic Rayleigh–Bénard convection (RBC) as the magnetic field grows in magnitude; as
$Ra$ is increased further, the data suggest that
$Nu$ grows approximately as
$Ra^{2/7}$, but with a smaller prefactor in comparison with RBC. Viscous (
$\epsilon _u$) and ohmic (
$\epsilon _B$) dissipation contribute approximately equally to
$Nu$ at the highest
$Ra$ investigated; both ohmic and viscous dissipation approach a Reynolds-number-dependent scaling of the form
$Re^a$, where
$a \approx 2.8$. The ratio of magnetic to kinetic energy approaches a
$Pm$-dependent constant as
$Ra$ is increased, with the constant value increasing with
$Pm$. The ohmic dissipation length scale depends on
$Ra$ in such a way that it is always smaller, and decreases more rapidly with increasing
$Ra$, than the viscous dissipation length scale for all investigated values of
$Pm$.
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- © The Author(s), 2021. Published by Cambridge University Press
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