Conditions for Earth-like geodynamo models

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Rotating convective turbulence in Earth and planetary cores (2015, background): “The latter case produces a more uniform large-scale axial dipolar magnetic field, with fewer large-scale magnetic flux patches outside the tangent cylinder, dissimilar to geomagnetic observations (cf. Christensen et al., 2010).”
Turbulent geodynamo simulations: a leap towards Earth's core (2017, background): “…laws that excluded diffusion properties (viscosity, thermal and magnetic diffusivities), it was argued that the simulations had reached an asymptotic regime, which allowed extrapolation to the Earth (Christensen et al., 2010), planets (Christensen, 2010), and some stars (Christensen et al., 2009).”