Multi-thermal space-time maps constructed along four different slits (see Fig. 1) using coordinated SST, IRIS, and SDO observations, illustrating the temporal and spatial evolution of plasma across different layers of the solar atmosphere. Top row (each example): SST Hα −0.8 Å (left) and Hα +0.8 Å (right) wing maps, sampling the lower chromosphere and revealing numerous upward-propagating jet-like structures. Second row: IRIS SJI 2796 Å (left) and SJI 1400 Å (right) maps, representing the upper chromosphere and transition region, respectively. Third row: corresponding coronal emission observed in the SDO/AIA 171 Å (left) and 131 Å (right) channels. Bottom row: composite maps formed by overlaying Hα −0.8 Å with AIA 171 Å (left) and Hα +0.8 Å with AIA 171 Å (right), highlighting the temporal and spatial correspondence between chromospheric jets and their coronal counterparts. The horizontal axis represents time, while the vertical axis shows the projected height along the slit.