Solar jet and surge observed in the other AIA/EUV channels (131 Å, 193 Åand 94 Å). The first column shows the images overlaid with HMI longitudinal magnetic field contours (±300 Gauss) for positive and negative magnetic polarities with green and blue colours, respectively. Panel e shows a dome structure at the jet base highlighted by a white dashed contour. In panel g, the red box shows the field of view of the brightening at the jet base overlaid by the contours of the small bipole (710″, 220″) and the large bipole (695″, 230″).