Fig. 4.

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Influence of αP on the super-SM JED parameter space: disk magnetization μ, deviation to Keplerian rotation δ, disk ejection efficiency ξ, thickness expansion hd = zid/h, accretion sonic Mach number ms, and laminar (jets) to turbulent (viscous) torque ratio Λ. Colored areas correspond to regions accessible by super-SM solutions. The curves represent the average solution for a given αP. See text for more details.
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