Intensity maps obtained with SPICE for four different lines starting from the cool chromosphere and incrementally increasing up to the coronal temperatures. The first row shows three consecutive frames (14:02:59, 14:14:28, and 14:25:57) for the H I Lyβ line, the second row shows intensity maps for the C III line, and the two last rows show intensity maps for the Ne VIII and Mg IX lines, correspondingly.