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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 8.

(a) σdyn(t) for Cases H3, H4, and H6 and (b) Cases M3, M4, and M6. (c) Angular momentum deficit of the RZ, ΔL(t), for Cases H0, H3, H4, and H6 and (d) Cases M0, M3, M4, and M6. Panels (e) and (f): shear-layer thickness Δ(t) for the same cases as panels (c) and (d), respectively. See Equations (24), (41), and (43). The vertical colored lines correspond to the values of t3/4 for each case.

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