﹩{\mathrm{log}}_{10}({{\rm{\nabla }}}_{{\rm{s}}})﹩ as a function of log₁₀ (ρ), comparing our 0.3 M_⊙, (a) 10 Myr or (b) 1 Gyr, α_MLT = 1.7 stellar model at ﹩{\rm{\Omega }}=20\,{{\rm{\Omega }}}_{\odot }﹩, B_v-max = 10⁴ G, and (a) δ = 0.03 or (b) δ = 0.06, to our α_MLT(r) model (plus markers). We include the rotating-only and magnetic-only cases for further comparison.