Views of the flaring region from different imagers and at different times. The SDO/AIA 304 Å image from the impulsive phase of the event shows the prominence in eruption (a) while the SDO/AIA 171 Å image from the decay phase shows the flare loops (b). The filament eruption subsequently led to a CME detected by the SOHO/LASCO C2 coronagraph (c). Times are at Earth time. The Solar Orbiter EUI-FSI 304 Å image shows the pre-flare filament and the flare ribbons (d and e), and the 174 Å image shows the flare loops (f). Times are at the observation time (321s before Earth time). The AIA images have been processed using the multi-scale Gaussian normalisation (Morgan & Druckmüller 2014).