Slices of the evolution of the n = 10 and n = 11 g modes of the reference model, as in Fig. 5, but now plotted with logarithmic amplitude. The left panel shows the n = 10 mode before its avoided crossing with the n = 11 mode, while the right panel shows the n = 11 mode after its avoided crossing with the n = 10 mode. This shows that the structure of the n = 10 mode before the crossing is similar to the n = 11 mode after the crossing, with the exception of an additional node near the core of the star.