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Öğe Faculae Cancel out on the Surfaces of Active Suns (vol 934, L23, 2022)(Iop Publishing Ltd, 2022) Nemec, N. -E.; Shapiro, A. I.; Isik, E.; Sowmya, K.; Solanki, S. K.; Krivova, N. . A.; Cameron, R. H.In Figures 1 and 2(a) the values given on the x- and y-axes, as well as the values on the x-axis given in Figure 2(b), do not correspond to the disk area coverage in percent. The values must be multiplied by 10 in order to be in units of percent of the solar/stellar disk. These plots were solely for demonstration purposes of the change in the area coverages with increasing stellar activity and do not affect the following results and conclusions.











