Series of images of 67P acquired in the visible range (616 nm) with the OSIRIS WAC on August 02, 2014. The panels show at the left the radially renormalised images and to the right the corresponding Laplace filtered image. The jet-like features clearly appear as very confined filaments of material varying in angular width. The FoV ranges from 17.2 × 17.2 to 13.9 × 13.9 km at the comet whereas the spatial resolution increases from 72 m/pix up to 52 m/pix. Date and time of image acquisition is on the frame, as well as the arrows indicating the angle convention for placing the detected jet-like features. The artifact to the right of each frame is due to the ghost resulting from overexposure of the nucleus. The look-up table is linear, white represents higher brightness intensity.