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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Review of helioseismic inversions shows the solar modelling problem remains unsolved with broad implications for stellar seismology and fields relying on precise stellar parameters.
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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Progress in global helioseismology: a new light on the solar modelling problem and its implications for solar-like stars
Review of helioseismic inversions shows the solar modelling problem remains unsolved with broad implications for stellar seismology and fields relying on precise stellar parameters.