Radius inflation determined from Δs_ad via Equation (18) as a function of the outputted radius inflation from the MM14 models for 0.3 M_⊙, (a) 10 Myr or (b) 1 Gyr, α_MLT = 1.7 stellar models at all combinations of ﹩{B}_{{\rm{v}}-\max }={10}^{3}\mbox{--}{10}^{5}\,{\rm{G}}﹩ (﹩{\rm{\Delta }}1\,{\mathrm{log}}_{10}({\rm{G}})﹩) and (a) δ = 0.01–0.03 (Δ0.005) or (b) δ = 0.01–0.06 (Δ0.005). y = x (orange) is plotted for ease of comparison.