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Fig. 7 | Progress in Earth and Planetary Science

Fig. 7

From: A review of the SCOSTEP’s 5-year scientific program VarSITI—Variability of the Sun and Its Terrestrial Impact

Fig. 7

Schematic 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)

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