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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 9.

Equilibrated-state values of σdyn, denoted by σdyn(∞), for all of our cases, plotted with respect to case number. We approximate ﹩{\sigma }_{{\rm{dyn}}}(\infty )\approx {[{\left\langle {\tau }_{{\rm{v}}}\right\rangle }_{{\rm{drz}},t}/{\left\langle {\tau }_{{\rm{mc}}}\right\rangle }_{{\rm{drz}},t}]}^{1/2}﹩, where the temporal average is over the equilibrated state.

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