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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 2.

Location in parameter space (Bu and σ) of the different simulations and the Sun. Cases 1 and 2 have the same Bu and σ, but different Raf (see Table 1). The viscous and radiative spreading regimes are separated at σ = σc ≈ 10 for the simulations or σ = σc ≈ 35 for the present-day Sun (see Appendix F).

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