Correspondence between the CESTAM profiles and their respective analogues in our model. (a) Comparison of extracted from a CESTAM solar model (in grey) and obtained from our model (in red). (b) Comparison of Y^CESTAM(t) extracted from the same model with . (c) Comparison of ψ^CESTAM(t) with . In the last two panels, the regions in which the curves are expected to correspond are shaded in red.