Fig. 2.
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Atmospheric profiles for the clusters with high emission in the blue wing of the representative profiles. The columns are split into the two different simulations (left: simulation A, right: simulation B). Top row: Average spectra of the clusters. Bottom three rows: Average atmospheric quantities in the clusters. From the top, they are the gas temperature, line-of-sight velocity, and total dissipative heating (Qviscous + Qjoule). The dashed black lines show the averages for the entire simulations. The distribution in the bottom row is the column mass of the blue emission clusters where τν equals unity for the inner blue wing (−5.4 km s−1) of Ca II H.
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