Fig. 9.
Rotation laws in radius r and colatitude θ for fast rotation (Ω = 10) under the influence of the large-scale Lorentz force for B = (0, 0.1, 20) (left panel, blue lines) and B = (0, −0.1, 20) (right panel, blue lines). The differential rotation is due to the nonmagnetic Λ effect (red lines). The uppermost Ω-isolines belong to the equator, while the lowest curves belong to the poles.
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