“…For other cratons (e.g., Australia, Greenland, Arabia) such consistency was not observed [e.g., Heintz and Kennett , 2005; Hansen et al , 2006; Ucisik et al , 2008]. Some of the discrepancy may be explained by a component of density‐driven flow in the asthenosphere (e.g., underneath Arabia [ Hansen et al , 2006]; see section 2.3), a modification of the asthenospheric flow field around keels [e.g., Fouch et al , 2000; Eaton et al , 2004; Heintz and Kennett , 2005; Gao et al , 2008], and a significant lithospheric contribution (e.g., Australia [e.g., Simons and van der Hilst , 2003; Heintz and Kennett , 2005] and east Antarctica [ Reading and Heintz , 2008]). Some other reported discrepancies between φ SKS and φ APM may have resulted from the large range of published φ APM [e.g., Heintz et al , 2003; Evans et al , 2006] or from the use of an inappropriate APM model (e.g., NNR in Antarctica [ Reading and Heintz , 2008], or HS2‐NUVEL1A in Africa [ Barruol and Ben Ismail , 2001]).…”