Normalized local rotation profiles Ω/Ω_⊙ with for Runs H0, H0.1, H1, M1, M4, M10, M30 and the rms values of the radial r sin θ∂Ω/∂r (black line) and latitudinal shear sin θ∂Ω/∂θ (red) versus Coriolis number Co. The values have been calculated as a time average over the saturated state, and we have omitted the 5 closest grid points to the latitudinal boundary to remove boundary effects from the rms. The values of the HD runs (Set H) are shown with a solid line with plusses and the MHD runs (Set M) with dashed line with diamonds. The zero rotation run has been moved to Co = 10⁻⁴ to be visible in the lower panel. The transition from anti-solar to solar-like differential rotations occurs in between the vertical lines (left line: last anti-solar run, right line: first solar-like run) and is shown as solid (Set H) and dashed (Set M) lines.