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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 10.

Mollweide projections and power spectra in azimuthal wavenumber for the poloidal magnetic field Bpol in the upper RZ (﹩{r}^{\ast }﹩/R = 0.692) for (a)–(c) Case M3, (d)–(f) Case M4, and (g)–(i) Case M6. The power spectra ﹩| {{\boldsymbol{B}}}_{{\rm{pol}}}^{m}{| }^{2}﹩ (Equation (45)) have been horizontally and temporally averaged over the equilibrated state.

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