Fig. 16From: Towards more realistic core-mantle boundary heat flux patterns: a source of diversity in planetary dynamosNon-dimensional CMB heat flux resulting from an impactor of radius 800 km falling on the north pole (left) or the equator (right). 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 Monteux et al. (2015) Back to article page