Impulsive coronal heating during the interaction of surface magnetic fields in the lower solar atmosphere

Open Access

Fig. B.6.

Open with DEXTER Download original image

Impulsive heating in the core of AR 12712. Panels a–i and f–g: are similar to Fig. 2. Panel j: IRIS SJI 1400 Å map in inverted grey scale. Animation of panels a–g 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.