Fig. B.1.
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Upper panels: the measure of variability for the mass accretion rate s/⟨ṁ⟩, Lower panels: the measure of variability for the normalized magnetic flux accumulated on the black-hole horizon s/⟨ϕBH⟩, both for a time window of ±270 M (Event Horizon Telescope Collaboration 2022b) for all MAD models ideal and with different resistivity (see Table 1 for details.)
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