The left column shows the outflow temperature, pressure, velocity, and hydrogen number density profiles as a function of radius for ﹩\dot{M}=1{0}^{13}﹩ g s⁻¹, together with the excited-state population ratio n₃/n₂. The dotted black line shows n₃/n₂ under the LTE assumption, highlighting the NLTE departure in the extended atmosphere. The right column shows the outflow model synthetic spectrum for ﹩\dot{M}=1{0}^{13}﹩ g s⁻¹ (orange) compared with the observed line profile (black) and the emission contribution function as a function of wavelength and radius. The line core probes up to 1.8 R_p, while the double peaks probe ∼1.3 R_p.