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Fig. 6.

image

Differential rotation between the inner equator and the outer sphere normalised to the outer value of the rotation rate Ω0 in the Eddington–Sweet regime, plotted as a function of Pr(N00)2Ro/E. The Rossby number Ro is varied to encompass the linear and non-linear regimes. The Ekman number is fixed to E = 10−6. The green curve corresponds to simulations with Pr(N00)2 = 10−1 (runs 1.4, 3.1, 4.1, 5.1, and 6.1 in Table 4) and the blue curve to simulations with Pr(N00)2 = 10−2 (runs 2.2, 3.2, 4.2, and 5.2 in the same table).

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