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Fig. 10.


Time evolution of the IRIS NUV spectrum in the hot pockets. The observed spectra and best fits in the range around the k line corresponding to the pixels A and B marked in Fig. 7. Spectra are ordered by time stamp from the top to the bottom. The insets zoom into the region around the UV triplet blend. The brightness temperatures of the observed and synthetic 1.25 mm continua are indicated.

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