Physical quantities of winds as a function of θ at r = 10³r_g from the 3D GRMHD simulation of black hole accretion in Y15. Top panels: density, temperature, and Mach number. Bottom panels: radial, meridional, and rotational velocities normalized by Keplerian velocity ﹩{v}_{k}({r}_{0})﹩. The value of the density is shown in code units. The density and temperature are time-averaged values, while all three velocity components are taken from one snapshot.