Evolution of our GRMHD simulation over time. The top and middle panels show the logarithm of the density in the equatorial and a meridional plane, respectively, for three different times. The bottom panel shows the temporal evolution of the mass accretion rate (Ṁ) and the MAD parameter, $\mathrm{\Phi }={\varphi }_{\mathrm{BH}}/\sqrt{\dot{M}}$. The vertical dashed blue lines mark the time frames of the density plots.