Free Access
Fig. 3
Peak of X-ray irradiances vs. peak of EUV irradiances for 4502 flares in the interval 2014–2016 when Rosetta was at comet 67P. The X-ray irradiances are measured by GOES, and the EUV irradiances are estimated by the FISM v.1-model. Not all of these flares are directed toward Rosetta.
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.