A 3D numerical model of the earth's core with a viscosity two orders of magnitude lower than the state of the art suggests a link between the observed westward drift of the magnetic field and superrotation of the inner core. In our model, the axial electromagnetic torque has a dominant influence only at the surface and in the deepest reaches of the core, where it respectively drives a broad westward flow rising to an axisymmetric equatorial jet and imparts an eastward-directed torque on the solid inner core. Subtle changes in the structure of the internal magnetic field may alter not just the magnitude but the direction of these torques. This not only suggests that the quasi-oscillatory nature of inner-core superrotation [Tkal ci c H, Young M, Bodin T, Ngo S, Sambridge M (2013) The shuffling rotation of the earth's inner core revealed by earthquake doublets. Nat Geosci 6:497-502.] may be driven by decadal changes in the magnetic field, but further that historical periods in which the field exhibited eastward drift were contemporaneous with a westward inner-core rotation. The model further indicates a strong internal shear layer on the tangent cylinder that may be a source of torsional waves inside the core.geomagnetism | geodynamo T he slow westward drift of the geomagnetic field is one of the best-and longest-known features of the historical field, for which the most likely explanation is a latitudinally dependent westward flow in the outermost outer core (1, 2). Another westward-propagating and possibly related feature is equatorial waves (3), perhaps caused either by advection or instabilities on an equatorial westward jet. However, longer time series provide evidence of periods of eastward drift of the field over the past 3,000 y (4, 5). Although some geodynamo models have reproduced westward drift (6, 7), many rely on thermal winds whose structure is tied to the boundary conditions imposed by the lowermost mantle, which changes only on a timescale of 10-100 million years. A seemingly unrelated phenomenon is the superrotation (relative to the mantle) of the inner core, whose estimates vary from zero to several degrees per year (8). Links between core-surface flows and inner-core rotation are difficult to quantify because a coupling mechanism extending across the entire outer core has remained elusive. There is some evidence of such a coupling through thermal winds in polar regions (9); however, because their amplitude is linked to the mass and thermal flux at the inner-core boundary, unless the inner core is very young, the effect likely is small (10).The fluid outer core, bounded by the solid inner core and overlying mantle, likely is in a quasi-magnetostrophic balance, in which the forces of pressure, buoyancy, Coriolis, and Lorentz are almost in equilibrium (6). Two key nondimensional parameters in any model are the Ekman and Rossby numbers, measures of viscosity and inertia, respectively, believed to be ∼10 −15 and ∼10 −6in the core. However, because of the vast range of temporal and spatial scales in th...