Small-scale and large-scale dynamos in global convection simulations of solar-like stars

Open Access

Fig. 15.

Time-averaged mean magnetic energy of the mean fields ${\bar{B}}^{2} / 2$ ${\overline{\boldsymbol{B}}}^2/2$ (top row) and fluctuating fields $\bar{B^{' 2}}$ $\overline{{\boldsymbol{B}}^{\prime 2}}$ (bottom) for all M and S runs in units of 10⁵ J/m³ for all magnetic runs (M+S). We disregard 7° near the latitudinal boundaries for determining the minimum and maximum values of the color range.

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