Free-fall velocities and heat transport enhancement in liquid metal magneto-convection

In geo- and astrophysics, low Prandtl number convective flows often interact with magnetic fields. Although a static magnetic field acts as a stabilizing force on such flow fields, we find that self-organized convective flow structures reach an optimal state where the heat transport significantly increases and convective velocities reach the theoretical free-fall limit, i.e. the maximum possible velocity a fluid parcel can achieve when its potential buoyant energy is fully converted into kinetic energy. Our measurements show that the application of a static magnetic field leads to an anisotropic, highly ordered flow structure and a decrease of the turbulent fluctuations. When the magnetic field strength is increased beyond the optimum state, Hartmann braking becomes dominant and leads to a reduction of the heat and momentum transport. The results are relevant for the understanding of magneto-hydrodynamic convective flows in planetary cores and stellar interiors in regions with strong toroidal magnetic fields oriented perpendicular to temperature gradients.

Automated summary

In geo- and astrophysics, low Prandtl number convective flows interact with magnetic fields. Static magnetic fields can stabilize flow fields, but self-organized convective flow structures can reach an optimal state where heat transport significantly increases. An increase in magnetic field strength beyond this state can lead to a reduction in heat and momentum transport due to Hartmann braking.