Dynamo simulations show non-dipolar magnetic field strengths are comparable across dipolar and non-dipolar regimes when scaled by driving power, while the dipole component is an order of magnitude weaker in the non-dipolar regime.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
UNVERDICTED 2representative citing papers
Top-heavy thermochemical geodynamo simulations show heterogeneous outer boundary heat flux reproduces observed longitudinal inclination anomaly variations, while elevated chemical driving reduces longitudinal structures and promotes polar radial field minima.
citing papers explorer
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A New Scaling Law for Non-Dipolar Magnetic Fields in Rapidly Rotating Stars and Planets
Dynamo simulations show non-dipolar magnetic field strengths are comparable across dipolar and non-dipolar regimes when scaled by driving power, while the dipole component is an order of magnitude weaker in the non-dipolar regime.
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Paleomagnetic signatures of core-mantle interactions inferred from top-heavy thermochemical geodynamo simulations
Top-heavy thermochemical geodynamo simulations show heterogeneous outer boundary heat flux reproduces observed longitudinal inclination anomaly variations, while elevated chemical driving reduces longitudinal structures and promotes polar radial field minima.