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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 5.

(a) Differential rotation contrast in the RZ defined in Equation (32a), plotted with respect to case number. (b) Differential rotation contrast in the CZ defined in Equation (32b). (c) The confinement ratio f defined in Equation (34). Note that because of the chosen ordering, f monotonically decreases for the MHD cases within the radiative spreading regime. (d) The RZ’s shear-layer thickness defined in Equation (35).

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