Fig. 4
Ca xvii 192 line profiles obtained with fil_rast_s2 on April 26, 2007 between 14:46 UT and 16:29 UT at two heights (20 000 km and 38 000 km). The downward arrows indicate the decrease in line emission from the corona to the prominence. Boxes 1, 5, 6, and 10 correspond to the corona, while the other ones are located on the prominence.
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