Fig. 7


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CME cavity observed in PROBA2/SWAP 174 Å binned down to SunCET required resolution of 30 (projected performance is 20). The cavity remains easily identifiable. SunCET’s SNR will be 9–30× higher off disk, making CME identification even easier. The 1.7 R FOV shown here, the largest of any solar EUV imager to date, is SWAP’s; SunCET’s extends to 4 R . Adapted from Byrne et al. (2014).

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