Fig. A.1.
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Time evolution of the mean turbulent kinetic energy density EK in the convection zone for simulations with nominal (L = 3.21 × 107 L⊙, blue) and low (L = 3.21 × 104 L⊙, purple) stellar luminosities. The convective time scales are assumed to be τconv = 1 000 s for the nominal simulations (see Eq. 7) and τconv = 10 000 s for the low luminosity ones.
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