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Fig. A.1.

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Azimuthal and time-averaged distribution of the logarithm of the magnetisation, σ, for different spins (left to right) and for the SANE (top) and MAD (bottom) models. The dashed white line corresponds to the Bernoulli parameter, −hut = 1.02, and the black lines show log10(σ) = −1.0, 0.5, and 0 contours.

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