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Fig. 8.
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EUV intensity along a coronal loop. Shown is the temporal evolution of the intensity in AIA filters at 171 Å (top panel), 193 Å (middle panel), and 304 Å (bottom panel) at all positions along the dotted blue line represented in Fig. 7. s = 0 corresponds to the footpoint of the coronal loop at the sunspot umbra.
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