Same as Fig. E.1, but for HD 192281 (O4.5V(n)((f)); vsin i = 276 km s^-1). Our ELODIE spectra of this star have a rather low S/N, rendering the fitting more uncertain. Some mismatches remain, in particular for He ii 5412 and the C iii 4153–4163 complex. Because wind parameters were not derived, wind-sensitive lines are not well reproduced: too much emission is seen in He ii 4686 and N iii 4634–4643 for the best-fit model.