Low inertia reversing geodynamos
Chris Jones, Yue-Kin Tsang

TL;DR
This paper investigates geodynamo models in the strong magnetic field regime, demonstrating that Earth-like magnetic reversals can occur under realistic parameter conditions with magnetic energy dominating kinetic energy.
Contribution
The study introduces a novel approach by increasing both Prandtl numbers to achieve strong field regimes in simulations, enabling Earth-like reversals with realistic energy hierarchies.
Findings
Earth-like reversals are possible at achievable parameters.
Magnetic energy exceeds kinetic energy except near reversals.
Simulations produce Earth-like magnetic fields away from reversals.
Abstract
Convection driven geodynamo models in rotating spherical geometry have regimes in which reversals occur. However, reversing dynamo models are usually found in regimes where the kinetic and magnetic energy is comparable, so that inertia is playing a significant role in the dynamics. In the Earth's core, the Rossby number is very small, and the magnetic energy is much larger than the kinetic energy. Here we investigate dynamo models in the strong field regime, where magnetic forces have a significant effect on convection. In the core, the strong field is achieved by having the magnetic Prandtl number Pm small, but the Ekman number E extremely small. In simulations, very small E is not possible, but the strong field regime can be reached by increasing Pm. However, if Pm is raised while the fluid Prandtl number is fixed at unity, the most common choice, the Peclet number number becomes…
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Taxonomy
TopicsGeomagnetism and Paleomagnetism Studies · Solar and Space Plasma Dynamics · Geophysics and Gravity Measurements
