Dynamo-generated magnetic fields confine the tachocline against radiative spreading in global simulations, with stronger stable stratification producing longer cycles, deeper penetration via skin effect, and better confinement plus interior spin-down transmission.
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2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
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 Dynamo Confinement Scenario for the Solar Tachocline and its Implications for Spin-down in the Radiative Spreading Regime
Dynamo-generated magnetic fields confine the tachocline against radiative spreading in global simulations, with stronger stable stratification producing longer cycles, deeper penetration via skin effect, and better confinement plus interior spin-down transmission.
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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.