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A Dynamo Confinement Scenario for the Solar Tachocline and Its Implications for Spin-down in the Radiative Spreading Regime

  • Authors: Loren I. Matilsky, Lydia Korre, Nicholas H. Brummell

Loren I. Matilsky et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 12.

Scatter symbols: realized amplitude of ﹩{\left\langle | {{\boldsymbol{B}}}_{{\rm{pol}}}{| }^{2}\right\rangle }_{t}﹩ in the RZ summed over the largest scales m = (0, 1, 2) for Cases M3, M4, and M6. Solid curves: profile for ﹩{\left\langle | {{\boldsymbol{B}}}_{{\rm{pol}}}{| }^{2}\right\rangle }_{{\rm{sph}},t}﹩ predicted by the nonaxisymmetric quasicyclic skin effect Equation (51). Each profile is normalized by its value at ﹩{r}^{* }={r}_{{\rm{skin}}}^{* }=0.692{R}_{\odot }﹩.

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