Notes. The estimated mean coronal temperature $T_0=\frac{1}{2}(T_{\mathrm{p}0}+T_{\mathrm{e}0})$ is shown on the third line. The associated coronal and at 1 au velocities (u₀, u_1 au), and densities (n₀, n_1 au), respectively, are shown in the four bottom lines. The initial parameters from Dakeyo et al. (2022) have been modified in order to fit the in situ measured temperatures and velocities of their five wind populations with the computed wind solutions including f(r) modeling. The 1 au density values are also calibrated to the five wind populations in order to have a direct comparison with Dakeyo et al. (2022) isopoly models. Bold values are features of primary interest.