The impact of resistivity on the variability of black hole accretion flows

Open Access

Fig. A.1.

The mean normalized magnetic flux accumulated on the black-hole horizon (error bars indicate ±1s) for all MAD models in time windows 3000 − 5000 M (dashed error bars) and 3000 − 10000 M (solid error bars) respectively. The dashed horizontal line depicts the MAD saturation value $ϕ_{\max} \approx 50 / \sqrt{4 π} \approx 14$ $\phi_{\mathrm{max}}\approx 50/\sqrt{4\pi}\approx 14$ .

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