In shearing dynamo simulations, shear-induced hemispheric small-scale magnetic helicity fluxes can overcompensate the scale transfer, making the mean-field amplitude nearly independent of magnetic Reynolds number.
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Magnetic helicity fluxes in dynamos from rotating inhomogeneous turbulence
In shearing dynamo simulations, shear-induced hemispheric small-scale magnetic helicity fluxes can overcompensate the scale transfer, making the mean-field amplitude nearly independent of magnetic Reynolds number.