Fig. 10
Scaling of average X-ray and 171 Å emission as observed by AIA, ⟨LX⟩, and ⟨ L171⟩ with averagecoronal heating ⟨Htot⟩ for model runs listed in Table 1. The bars represent the standard deviation of LX and L171 in time. The red lines are power-law fits to the data. The blue line in panel a indicates what is expected from the RTV scaling laws. See Sects. 5 and 6.5.
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