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Fig. 6

image

Modulus of the absolute latitudinal differential rotation, , normalized by the solar rotation rate, as a function of rotation rate. The red lines result from fitting. The black dashed line indicates the break in the slope. Red and black circles stand for high- and low-resolution 2π runs, respectively, while blue triangles show the π∕2 wedges. We note that for the fit for moderate rotation, we do not take into account Run D with very low values. The dotted line indicates the transition from antisolar to solar-like latitudinal differential rotation.

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