Temporal evolution of the UV bursts identified here in four UV channels, namely the SDO/AIA 1600 Å channel (top row), SDO/AIA 1700 Å channel (second row), IRIS SJI Mg II 2796 Å channel (third row), and IRIS SJI Si IV 1400 Å channel (fourth row). The blue contours on the second row outline the co-spatial line-of-sight magnetic field at a value of −100 G as sampled by SO/PHI-HRT (first five columns) and SDO/HMI (sixth column). Multiple UV bursts are immediately evident in the IRIS SJI Si IV 1400 Å data through time. The bottom row plots the evolution of the intensity within this FOV through time for the IRIS SJI Si IV 1400 Å channel (solid line), the IRIS SJI Mg II 2796 Å channel (dashed line), the SDO/AIA 1600 Å channel (dotted line), and the SDO/AIA 1700 Å channel (dot-dashed line). A movie more clearly displaying the evolution of this region (combined with Fig. 3) is included with the online version of this article.