Fig. 7From: Towards more realistic core-mantle boundary heat flux patterns: a source of diversity in planetary dynamosNon-dimensional normalized CMB heat flux pattern inferred from probabilistic tomography. The same pattern was used for different q ∗ values (see Table 1), hence the absence of a color bar. Red/blue denotes positive/negative heat flux anomalies, respectively. From Amit et al. (in press)Back to article page