Same plot as in Fig. 23 with the absorption calculated over the range −230 to −140 km s^-1 for HD 189733b (escape rate Ṁ = 2 × 10⁹ g s^-1; ionizing flux F_ion = 10  F_⊙, stellar wind with temperature T_wind = 3 × 10⁴ K, bulk velocity V_wind = 200 km s^-1, and density n_wind = 2 × 10⁴ cm^-3). The blue points correspond to the transit and post-transit observations divided into 751 s time exposures (see Bourrier et al. 2013). Only particles with observed velocities in the range −230 to −140 km s^-1 are represented.