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Fig. 4.

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Time evolution (in units of tturn) of vorticity and magnetic energy of runs with the shearing profile and different R (see Table A.3). If we use the shearing timescales, the magnetic instability is between 70 and 200 tshear with more similar growth rates (see Fig. 5). In both cases, R = 1.00 and R = 1.50 take the least amount of time to reach the instability. Dashed lines represent the exponential fits for Emag during dynamo growth (top panel), ωrms during vorticity growth, and ωrms during dynamo growth (bottom panel).

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