Fig. 7From: A review of the SCOSTEP’s 5-year scientific program VarSITI—Variability of the Sun and Its Terrestrial ImpactSchematic representation of several modeled sunspot groups on the solar disk, with their corresponding modeled flaw energies computed with the Aulanier et al. (2013) simulation. A sunspot group consists of several pairs of sunspots. In each group, a pair of sunspots (surrounded by red curve) representing 30% of the sunspot group area is modeled in the simulation (taken from Schmieder 2018)Back to article page