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.
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