Free Access

Fig. 6


Elemental abundances relative to solar photospheric values (Grevesse & Sauval 1998) as a function of the first ionisation potential (FIP) during quiescence (black) and flare (red). The top and bottom panels show abundance values obtained using a combination of MOS+RGS and PN+RGS, respectively. Dashed line at unity indicates the solar photospheric abundance.

This figure is made of several images, please see below:

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.