Disk-wind properties derived from the tomography along lines of constant V_Z. Red dashed curves show fits as a function of the poloidal velocity of the streamline V_p: the anchoring radius of the streamline r_0,con was fit by a third-order polynomial, the angle of the streamline with the flow axis θ by a power law and the product V_P × j by a constant value of 570 au km² s⁻². Blue dotted lines represent the extrapolation used to model the high-velocity component that could not be mapped by tomography due to its low S/N.