Fig. 8
Solar coronal EMD (composed of ARs, COs, and FLs) that best matches spectral parameters of ɛ Eri. Blue line: AR contribution; green line: CO contribution; red line: FL contribution; gray line: total EMD of the chosen model. Each observation is represented by a different fraction of surface coverage with AR, CO, and FL selected as describedin Sect. 3.1. Red triangles: medians of the 1000 best-fit parameters of the selected synthetic spectra; black dots: best-fit parameters of the observations.
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