Image Details
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.
© 2026. The Author(s). Published by the American Astronomical Society.