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Fig. 29
Mass accretion rate plot for an initially perturbed model with ϵρ = 0.2, but reverting to ϵρ = 0 upstream at time t = 300M. The black hole has spin a = 0.9 and the wind is in the equatorial plane. The solid line shows the final mass accretion rate from the equivalent flow with ϵρ = 0 throughout.
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