Planetary gyre, time-dependent eddies, torsional waves, and equatorial jets at the Earth's core surface
N Gillet, D Jault, C. C. Finlay

TL;DR
This study models Earth's core surface flows over 70 years, revealing large-scale gyres, eddies, jets, and torsional waves, and assesses their impact on Earth's rotation and magnetic interactions.
Contribution
It provides a detailed, time-dependent quasi-geostrophic model of core flows, incorporating uncertainties and magnetic interactions, with new insights into torsional waves and angular momentum exchanges.
Findings
Identification of time-dependent large-scale eddies and jets at the core surface.
Retrieval of torsional waves explaining length-of-day variations.
Revised understanding of electromagnetic core-mantle coupling effects.
Abstract
We report a calculation of time-dependent quasi-geostrophic core flows for 1940-2010. Inverting recursively for an ensemble of solutions, we evaluate the main source of uncertainties, namely the model errors arising from interactions between unresolved core surface motions and magnetic fields. Temporal correlations of these uncertainties are accounted for. The covariance matrix for the flow coefficients is also obtained recursively from the dispersion of an ensemble of solutions. Maps of the flow at the core surface show, upon a planetary-scale gyre, time-dependent large-scale eddies at mid-latitudes and vigorous azimuthal jets in the equatorial belt. The stationary part of the flow predominates on all the spatial scales that we can resolve. We retrieve torsional waves that explain the length-of-day changes at 4 to 9.5 years periods. These waves may be triggered by the nonlinear…
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