Paired HRI and AIA 171 images used for reconstructing the erupting filament and jet location, shown in (a1) and (a2). Accounting for light travel time differences, HRI_EUV images have been rotated to a certain angle to facilitate analysis and readability. Paired HRI_EUV and AIA 171 images used for reconstructing the post-flare loops, shown in (b1) and (b2). 3D reconstruction of the filament, the jet loction, and post-flare-loops from Solar Orbiter and SDO views, respectively, shown in (c1) and (c2). The points selected for reconstruction are specifically highlighted, with a colour bar indicating the height information of the filament and post-flare-loops.