Multipoint study of the rapid filament evolution during a confined C2 flare on 28 March 2022, leading to eruption

Solar Orbiter First Results (Nominal Mission Phase)

Open Access

Fig. 10.

Emergence of AR 12975 and the formation of the original filament as observed by SDO/HMI, selected SDO/AIA channels, and by KSO and GONG in Hα at six times (columns). HMI LOS magnetograms are scaled from −1500 G (red) to +1500 G (blue). The associated movie is available online.

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.