Intensity and photospheric magnetic flux properties of an SSLS associated with a flux emergence. The top row shows the AIA 193 image and quasi-temporal HMI magnetogram for case 24 (see the online animation bp024.mov). The contours outline the ±25 and ±50 G magnetic flux concentrations. The evolution of the total magnetic flux is shown in the second row, and the maximum (peak) intensity and the total intensity flux evolution taken from the selected FOV are given in the third and fourth rows of Table 1. The two vertical thick lines together with the arrowed horizontal line (only shown in the top panel) indicate the SSLS lifetime.