Can Core Flows inferred from Geomagnetic Field Models explain the Earth's Dynamo?

TL;DR

This study investigates whether large-scale, geomagnetically inferred core flows can generate Earth's magnetic field through dynamo simulations, highlighting the importance of Lorentz force effects and flow complexity.

Contribution

The paper demonstrates that incorporating Lorentz force effects into large-scale flow models enables magnetic field generation, suggesting these flows are sufficient for Earth's dynamo without small-scale flows.

Findings

Magnetic field generated when Elsasser number > 0.25 and Reynolds number > 100.

Time periods from 120 to 50 years do not affect mean growth rate.

Inner-core footprint influences deep magnetic field generation.

Abstract

We test the ability of large scale velocity fields inferred from geomagnetic secular variation data to produce the global magnetic field of the Earth.Our kinematic dynamo calculations use quasi-geostrophic (QG) flows inverted from geomagnetic field models which, as such, incorporate flow structures that are Earth-like and may be important for the geodynamo.Furthermore, the QG hypothesis allows straightforward prolongation of the flow from the core surface to the bulk.As expected from previous studies, we check that a simple quasi-geostrophic flow is not able to sustain the magnetic field against ohmic decay.Additional complexity is then introduced in the flow, inspired by the action of the Lorentz force.Indeed, on centenial time-scales, the Lorentz force can balance the Coriolis force and strict quasi-geostrophy may not be the best ansatz.When the columnar flow is modified to account for the action of the Lorentz force, magnetic field is generated for Elsasser numbers larger than 0.25 and magnetic Reynolds numbers larger than 100.This suggests that our large scale flow captures the relevant features for the generation of the Earth's magnetic field and that the invisible small scale flow may not be directly involved in this process.Near the threshold, the resulting magnetic field is dominated by an axial dipole, with some reversed flux patches.Time-dependence is also considered, derived from principal component analysis applied to the inverted flows.We find that time periods from 120 to 50 years do not affect the mean growth rate of the kinematic dynamos.Finally we notice the footprint of the inner-core in the magnetic field generated deep in the bulk of the shell, although we did not include one in our computations.