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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 13.

Difference of the bulk rotation rate of the RZ from the background frame rate, Ωrz − 1/2, as a function of Bu for the MHD cases (see Equation (33)). The dotted line separates the radiative spreading cases on the left from the lone viscous spreading case on the right.

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