Diagnostic capabilities of spectropolarimetric observations for understanding solar phenomena - I. Zeeman-sensitive photospheric lines

Free Access

Fig. 7.

Spatial distribution of line core intensity signals for the lines of interest. The selected FOV corresponds to the highlighted area in Fig. 1 that is described in Fig. 6.

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.