Skip to main content

Table 2 Summary of dynamo models imposed outer boundary heat flux patterns in AC09 (Amit and Choblet 2009), AC12 (Amit and Choblet 2012), ADC15 (Amit et al. in press), ODHZ13 (Olson et al. 2013), AO15 (Amit and Olson 2015), SJ12 (Sreenivasan and Jellinek 2012), and MACLT15 (Monteux et al. 2015). For each paper, the reference and alternative patterns are given. Tomographic always refers to present-day, HF1 is the time-dependent model of Zhang and Zhong (2011). For more details, see text

From: Towards more realistic core-mantle boundary heat flux patterns: a source of diversity in planetary dynamos

Paper

Reference

Alternative

AC09

Tomographic

Thermal + post-perovskite

AC12

\({Y_{2}^{2}}\)

\({Y_{2}^{2}}\) + ridges

ADC15

Tomographic

Probabilistic tomography

ODHZ13

Tomographic

HF1

AO15

Homogeneous

Rotated \({Y_{2}^{0}}\)

SJ12

Homogeneous

Plume-induced

KJRF14

Homogeneous

Impact-induced

MACLT15

Degree-1

Impact-induced