Fig. 3
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Quadratic average of the large-scale magnetic field over the stellar surface (red; column 2 of Table C.1), polar strength of the dipolar component (green; column 5 of Table C.1), and average small-scale field over the rotation cycle (blue; column 4 of Table C.1) as a function of the observing epoch, for the 11 magnetic topologies of AU Mic derived with ZDI.
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