Fig. 6
Top: active region synthetic spectrum for the Ti_poly filter using the photospheric abundances of Asplund et al. (2009). Bottom: flare synthetic spectrum for the Ti_poly filter using the coronal abundances of Feldman et al. (1992) and the “Flare 2” observation. The effective area is overplotted as a dashed line (scaled). The peak intensities of stronger lines are indicated.
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