Coronal hole boundaries at small scales - IV. SOT view. Magnetic field properties of small-scale transient brightenings in coronal holes

Free Access

Fig. 11

Open with DEXTER Download original image

As Fig. 8, lightcurves of a CH bright point that is marked as No. 2 event on November 12 in Fig. 1. The X-ray lightcurve is extracted from the FOV shown in Fig. 9 and the magnetic flux variations are extracted from the region outlined by dotted lines in Fig. 10.

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.