Fig. 7
Download original image
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).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.