Fig. 6
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Differential rotation proflies in the solar interior, following Markiel & Thomas (1999) parametrisation of the original data from Schou et al. (1998). The angle θ = 55° sets the change of the sign of the radial gradient, being Ωr > 0 nearer to the equator and Ωr < 0 closer to the poles. r = 0.715 R⊙ is the base of the solar convection zone and r = 0.665 R⊙ sets the bottom of the tachocline.
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