S CrA N at different scales. Right: Representation of the star–disk interaction region (not to scale), with the characteristic sizes derived in this work. The obliquity of the magnetosphere is simply illustrative as no consolidated value exists. Top-left: SPHERE polarized intensity image from Zhang et al. (2023), and the directions toward the HH objects associated to S CrA. We also reported the PA of the dusty disk measured from the K-band continuum and the orientation of photocenter shifts as yellow, red and blue cones, respectively. Dashed cones highlight the suggested outflow emission (see text). Bottom-left: ALMA ¹²CO(2–1) first moment map from Gupta et al. (2023). The cone is reported from the SPHERE observations, and the HH82 direction is indicated. Both images have been rotated to have the same orientation as the sketch, where the north and east directions are shown.