Heating and cooling of coronal loops observed by SDO

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Fig. 6

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AIA/SDO extreme UV images and corresponding base-difference images. Panels (a)–c)) show the original images and panels (d)–f)) the respective difference images (d)–f)). The red contours in (d)–f)) indicate the Fe XVIII loops in Fig. 1a. Same FOV as in Fig. 1.

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