Fig. 4: Electrical conductivity for a BMO-driven dynamo and time evolution of the dynamo. | Nature Astronomy

Fig. 4: Electrical conductivity for a BMO-driven dynamo and time evolution of the dynamo.

From: Electrical conductivities of (Mg,Fe)O at extreme pressures and implications for planetary magma oceans

Fig. 4: Electrical conductivity for a BMO-driven dynamo and time evolution of the dynamo.

a, The solid lines represent the minimum electrical conductivity required for dynamo generation in BMOs in super-Earths. The x axis is the planetary mass Mp normalized by the Earth mass M. The black, grey and light grey lines correspond to CMFs of 0.20, 0.32 and 0.68. The dashed lines and dashed-dotted lines represent the electrical conductivity based on equation (2) using the P and T condition at the CMB and the average P and T in the BMO. b, Time evolution of the magnetic field strength at the planetary surface as a function of time for a 6 M planet. The orange lines represent the BMO-driven dynamo, and the grey lines represent the core-driven dynamo. Details of the best fit, MLT, CIA and MAC are discussed in the main text.

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