Time dependence of the mass flux through the black hole horizon (top panel), the horizon integrated magnetic flux (middle panel), and the so-called MAD-ness parameter, ϕ_BH, given by Eq. (5), (bottom panel). Red lines denote the models with initial gas-to-magnetic pressure ratio β = 100, orchid lines present results for β = 50, and magenta lines denote β = 30. Black hole spin parameter in all models is a = 0.3. The disk inner radius is located at 6 and maximum pressure radius at 13 r_g (GRB-type models).