Sketch of the magnetic configuration of the CME flux ropes observed by Solar Orbiter/MAG and inserted in EUHFORIA. The left panel provides a top view (for an observer looking toward the negative Z direction), while the right panel provides a side view (for an observer looking toward the positive Y direction). CME1 is modeled as a low-inclination, right-handed (i.e., positive) chirality flux rope (clockwise rotation) characterized by a magnetic topology of SWN type. CME2 is modeled as a low-inclination, left-handed/negative chirality flux rope (counterclockwise rotation) characterized by a magnetic topology of SEN type.