Skip to main content
Progress in Earth and Planetary Science
Fig. 3 | Progress in Earth and Planetary Science

Fig. 3

From: Effect of width, amplitude, and position of a core mantle boundary hot spot on core convection and dynamo action

Fig. 3

Influence of various model parameters on EAA contribution. Impact of a anomaly amplitude, b tilt angle, c shell geometry, and d vigour of convection on the EAA contribution for varying anomaly width Ψ. The coloured vertical lines denote the colatitude of the tangent cylinder. Reference parameters (unless specified otherwise): Ra=4×107, q ∗=1.0, τ=0, β=0.35

Back to article page