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.
year = 2014, month = aug, volume =
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Active-region magnetic fields modulate deeper meridional flows in the Sun's near-surface shear layer, driving episodic poleward flux transport and hemispheric asymmetries in polar field evolution.
Synthetic spectra tests show Zeeman broadening recovers M dwarf magnetic field strengths more reliably with joint abundance fitting and WAIC selection than with free line strengths or BIC/AIC, which underestimate by 30-50% in active cases.
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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Active-region Modulation of Subsurface Meridional Flows and Magnetic Flux Transport on the Sun
Active-region magnetic fields modulate deeper meridional flows in the Sun's near-surface shear layer, driving episodic poleward flux transport and hemispheric asymmetries in polar field evolution.
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Testing the reliability of magnetic field strength measurements for M dwarfs
Synthetic spectra tests show Zeeman broadening recovers M dwarf magnetic field strengths more reliably with joint abundance fitting and WAIC selection than with free line strengths or BIC/AIC, which underestimate by 30-50% in active cases.