Fig. 3
EVE spectra during the flare on 2011 Mar. 03 after subtracting a pre-flare emission, (in W m-2 nm-1). Overplotted as dotted lines are the following iron lines: Fe xviii 93.93 Å, Fe xviii 103.97 Å, Fe xix 108.37 Å, Fe xxii 117.17 Å, Fe xx 118.88 Å, Fe xx 121.845 Å, Fe xxi 128.7 Å, Fe xxiii 132.8 Å, Fe xxii 135.755 Å. The AIA 94 (dashed-dotted) and 131 (dashed) Å channel responses are indicated on each graph.
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