Hα profiles as in Fig. 5, but now the density ρ₀ is varied to keep the mass loss rate at 0.1   Ṁ_acc, while the disk wind outer radius r_do changes from 30.0   R_∗ to 5.0   R_∗, and each line represents a different r_do and a different ρ₀. In a), r_do = 30.0   R_∗ and ρ₀ = 4.71 × 10^-12   gcm^-3 (dark grey thick solid line), r_do = 20.0   R_∗ and ρ₀ = 5.72 × 10^-12   gcm^-3 (black thin dashed line), r_do = 10.0   R_∗ and ρ₀ = 9.02 × 10^-12   gcm^-3 (black thin dotted line), r_do = 7.5   R_∗ and ρ₀ = 1.19 × 10^-11   gcm^-3 (dark grey thin dashed line), r_do = 5.0   R_∗ and ρ₀ = 2.13 × 10^-11   gcm^-3 (light grey thin solid line). In b), the lines have the same value of r_do, but their ρ₀ are 10 times higher than in a). The black thin line represents the line profile with only the magnetospheric component.