Comparison between the FoVs of Metis (4.7–10.0 R_⊙) and SOHO/LASCO-C2 (2.2–6 R_⊙) on the right, and STEREO-A/COR2 (3–15 R_⊙) on the left on October 25. Despite the 34-degree angle between the two instruments PoS, the structure visible in the UV channel of Metis almost matches the bright central core of the CME visible from COR2, as shown in the picture on the left. The images are produced with the open-source software JHelioviewer (Müller et al. 2017).