Visualization of the estimated compared to the PA_dust. Top panels show DL Tau (left) and CI Tau (right). Middle panels show DS Tau (left) and IP Tau (right). Bottom panel is IM Lup. The MUSE outflow/jet images are averaged from the different emission lines that are used to estimate the . We adopt the geometrical configuration visually demonstrated in Fig. 3 from Piétu et al. (2007) for the disks with positive and negative inclination. CI Tau has positive disk inclination, and the is measured from north to west. The rest of the sources have negative disk inclination and the is measured from north to east.