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Fig. 9
Emissivity ratio curves relative to the main Fe xii EUV transitions observed by Hinode EIS on 2007 Aug. 19, using the DM05 atomic model (above) and the present RM4+DW6 (below). The wavelengths and indices of the transitions are given, as well as the observed intensity Iob (see Del Zanna 2012, for details).
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