SDO/AIA 171 Å observations corresponding to the eleven thin coronal jets associated with CBPs shown in Fig. 1. Cases 06 and 09 are those in which the spine of the jet, indicated by the gray arrows, can be easily distinguished in AIA. In the other cases, the jet base may be inferred, or the jet is completely absent. The intensity of the images is given in DN and times are in UT. The images display the same regions as observed by HRI_EUV but are not spatially co-aligned, as the goal is to provide contextual information. The AIA times have been selected to match the corresponding HRI_EUV observations, accounting for the light travel time delay due to Solar Orbiter’s position near the Sun. Individual movies for each dataset are available .