Dynamics of the accretion flow. The two panels show the ideal and resistive case for MAD models (left panels) and Multi-loop models (right panels). Upper panels: Mass accretion rate, Ṁ, through the black hole horizon. Middle panels: Magnetic flux accumulated on the black hole horizon, Φ_BH. Lower panels: Normalized magnetic flux accumulated on the black hole horizon, ϕ_BH (see Table 1 for model details).