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Fig. 9

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Emissivity ratio curves relative to the “foreground-subtracted” sunspot loop leg observed by Hinode EIS (Del Zanna 2009a), using the previous (Storey et al. 2002, above) and present (below) atomic data, and the new radiometric calibration (Del Zanna 2013). The intensities Iob are in phot cm-2 s-1 arcsec-2.

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