Extreme-ultraviolet (EUV) observables of simulated plasmoid-mediated reconnection in the solar corona

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Fig. 12.

Spectral line profiles for the MUSE/SG Fe IX 171 Å, Solar-C/EUVST Fe X 174 Å, and Solar-C/EUVST Fe XII 195 Å lines, taken from case G6b. Layout is the same as for Fig. 11. A movie of the time evolution for t ∈ [18, 28] min is available online.

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