Fig. 2From: Towards more realistic core-mantle boundary heat flux patterns: a source of diversity in planetary dynamosScatter plots of CMB heat flux anomalies vs. seismic shear velocity anomalies at the lowermost mantle based on mantle convection simulations. a Isochemical cases without (red) and with (green) post-perovskite. b Thermochemical cases with various density contrasts δ ρ m at the CMB. From Nakagawa and Tackley (2008) Back to article page