Snapshots of the (yz)-correlations (normalised with ) for Ω = 10 and a magnetic field B = (0, 1, 10) (top) or B = (0, 1, −10) (bottom). From left to right: , and M_yz. In opposition to nonrotating turbulence (see Fig. 4), T_yz is now positive for both field geometries. As Käpylä et al. (2017) show with their numerical dynamo simulations, the numerical values of the two middle rows are rather robust against the variation of the magnetic Prandtl number; Pr = 0.1, Pm = 0.1, and θ = 45°.