Fig. 7.
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Temporal evolution of the (a) toroidal and (b) poloidal magnetic energies for the azimuthal modes m = 0 to m = 6 in the unstratified run TU0. The dashed black lines show exponential fits to the energy evolution of the m = 1 mode within the time interval
. These fits are used to determine the instability growth rates σ discussed in the text.
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