Fig. 3


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Solution run 1, a non-kinematic dynamo solution in the Pm > 1 regime. Its defining parameters are listed in the second line of Table 1. (A) Time series of normalized magnetic energy (black), integrated shear proxy (red), and equatorial parity (blue), starting from a seed magnetic field and Ω′ = 0 at t = 0. (B) Time-latitude diagram of the toroidal magnetic component extracted at r/R = 0.85, with a meridional plane snapshot at right. (C) Similar time-latitude diagram at r/R = 0.85 and meridional snapshot, but for the angular velocity perturbation normalized to the background angular velocity profile, i.e., Ω′(rθt)/Ω(rθ).

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