Stochastic excitation of waves in magnetic stars - I. Scaling laws for the mode amplitudes

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Fig. 4.

Scaling laws given by Stevenson for the change in (top) wavenumber $\tilde{K}$ $\tilde{K}$ and (bottom) in convective velocity $\tilde{U}$ $\tilde{U}$ . The grey zone in the bottom figure, between A = 1, 28 and A = 3, 43, shows the transition region, in which the low-A and the high-A prescription cannot be clearly distinguished.

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