Schematic view (arbitrary scale) of our parabolic GRMHD jet with a moderately high spin (a ≥ 0.7). The system is organized by the highly magnetized funnel (parabolic jet) and the weakly magnetized coronal/wind above the RIAF body. Typical values of the ratio of magnetic to rest-mass energy: b²/ρ, the plasma-β, β_p, and the Bernoulli parameter, ﹩\mathrm{Be}\,(\approx -{u}_{t}-1)﹩, are specified. The limb-brightened (i.e., spine-sheath) structure is expressed as a context of the lateral stratification of the bulk Lorentz factor: Γ (dark-shaded area: Γ > 1; light-shaded area: Γ ≃ 1). The funnel edge (b²/ρ ≃ 1, β_p ≃ 1, Be ≈ 0, ﹩{u}^{r}\ne 0﹩) and the jet stagnation surface (Be ≈ 0, ﹩{u}^{r}=0﹩) are shown as the thick solid and dashed lines, respectively. Emerging blobs are illustrated near the funnel edge.