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astro-ph.SR2025
Dynamo Confinement of a Radiatively Spreading Solar Tachocline Revealed by Self-consistent Global Simulations
Loren I. Matilsky, Lydia Korre, Nicholas H. Brummell
The helioseismically observed solar tachocline is a thin internal boundary layer of shear that separates the rigidly-rotating solar radiative zone from the differentially-rotating…
astro-ph.SR2025
Towards a self-consistent hydrodynamical model of the solar tachocline
P. Garaud, D. O. Gough, L. I. Matilsky
The solar tachocline is an internal boundary layer in the Sun located between the differentially-rotating convection zone and the uniformly-rotating radiative interior beneath. Spi…