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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Pith papers citing it
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astro-ph.EP 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
3D anelastic simulations find that both convective zone Busse columns and weather-layer PV homogenization produce Jupiter-like jets, with the weather layer causing deviations in thermal wind balance and long-term high-latitude jet migration.
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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Superrotation and Jet Migration in Simulations of Jupiter's Convective Zone and Weather Layer
3D anelastic simulations find that both convective zone Busse columns and weather-layer PV homogenization produce Jupiter-like jets, with the weather layer causing deviations in thermal wind balance and long-term high-latitude jet migration.