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Fig. 6.

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(a) Total magnetic energy as a function of time (in black) versus the radius of ⟨uϕϕmax in the equatorial plane (θ = π/2), in blue. The large radii correspond to a three-layer rotation, while low values denote anti-solar rotation (compare Figures 5c,d). (b) The magnitude of the zonal flow, Δuϕeq = |⟨uϕmax − ⟨uϕmin|, in the equatorial plane (in green). The rms of the magnetic Lorentz force is shown in red. (c) The two energy states of the flow – high and low – in the phase space of the total magnetic energy and the energy of the axisymmetric (zonal) flow, with the points colored by the rms of the Lorentz force, for Nρ = 6, Ra = 32 $ \widetilde{Ra} = 32 $.

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