The relative importance of each angular momentum transport mechanism strongly depends on the latitude. We depict the polar angular dependence of the decomposed time-averaged angular momentum flux at r = 30r _g , normalized to the average angular momentum flux at r = 2r _g (Equation (10)). We break down the total radially outward angular momentum flux (﹩{T}_{\varphi }^{r}﹩, shown with the solid gray line, Equation (1)) into four components: (a) turbulent Maxwell stresses (−〈δ b ^r δ b _φ 〉; Equation (7)), (b) large-scale laminar Maxwell stresses (−〈b ^r 〉〈b _φ 〉; Equation (8)), (c) advective transport (〈wu ^r 〉〈u _φ 〉; Equation (6)), and (d) turbulent Reynolds stresses (〈δ wu ^r δ u _φ 〉; Equation (5)). The turbulent Maxwell stresses are the dominant mode of outward angular momentum transport within the disk, while the large-scale Maxwell and advective terms dominate in the winds.