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Energy pathways in large- and small-scale convection-driven dynamos

Published 2 Dec 2022 in physics.flu-dyn, astro-ph.EP, astro-ph.SR, physics.geo-ph, and physics.plasm-ph | (2212.00969v2)

Abstract: We investigate the energy pathways between the velocity and the magnetic fields in a rotating plane layer dynamo driven by Rayleigh-B\'enard convection using direct numerical simulations. The kinetic and magnetic energies are divided into mean and turbulent components to study the production, transport, and dissipation associated with large and small-scale dynamos. This energy balance-based characterization reveals distinct mechanisms for large- and small-scale magnetic field generation in dynamos, depending on the nature of the velocity field and the conditions imposed at the boundaries.

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