Effect of electromagnetic boundary conditions on the onset of small-scale dynamos driven by convection
M. Fontana, P. D. Mininni, and P. Dmitruk
Phys. Rev. Fluids 8, L031801 (2023) - Published 1 March, 2023
The motion of conducting fluids in Earth’s convective core and in the solar convective region generate magnetic fields, but how strong must convection be to sustain a dynamo, and how do boundary conditions affect its onset? We examine this with a new method, treating different boundaries on equal footing, and show that changing the boundaries from conductors to vacuum greatly increases the energetic cost of sustaining magnetic fields against Ohmic losses. The threshold for magnetic field generation is shown to become independent of turbulence strength for strong enough convection. Our results impact the study of planetary and stellar dynamos and can guide experimental and numerical studies.































