COR1 PAs (vertical axis) vs. EUVI PAs (horizontal axis) for jets observed at the north (left) and at the south polar coronal hole (right). The red dashed line represents the bisector of the plane and ideally should trace equal PAs between the EUVI and COR1 FOV (radial propagation); the green dashed line fits the data points. Events rooted significantly away from the poles in EUV tend to have an even larger deviation in COR1.