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Fig. 3.


Eigenfunction Ψ(r) of several radial acoustic modes (black: n = 10 (ν0 = 1.580 mHz); red: n = 20 (ν0 = 2.912 mHz); blue: n = 30 (ν0 = 4.267 mHz)) as computed by our model (solid lines), and calculated using the ADIPLS code (dashed lines). The radial axis is zoomed to show only the outermost region. The eigenfunctions have been normalised so that their maximum over the entire solar interior equals 1.

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