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Fig. C.1.

image

Top row: peak DN in a selection of SW lines, as a function of the position along the slit, for an average of 15 exposures of 60 s, with the 2″ slit on the quiet Sun, recorded on 2008-11-19 with the EIS study GDZ_QS1_NS_60x512. The dashed vertical line indicates the mid position of the 1024 slit. The bottom 512″ were observed by a raster starting at 11:38 UT, while the top 512″ were observed by a raster starting at 12:13 UT. Note the small temporal variation in the peaks of the lines. Middle row: line centroid positions; the dashed line indicates the estimated variation as available in the EIS software notes. Bottom row: FWHM in the lines, while the dashed line indicates the estimated variation as available in the EIS software notes.

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