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Fig. 5
Evolution of the AIA 94 Å emission after the GREGOR observations. The white arrow indicates the Fe xviii loops, whose footpoints lie in the ribbon. The ribbon itself is shown by the black contour in the top left image. This contour corresponds to the 80 DN s-1 px-1 value in the IRIS SJI 1400 Å observation at 12:00 UT.
This figure is made of several images, please see below:
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