“…The emission spectra obtained are shown in Figure 50, in the left part for the VUV region, in the right part for the UV, VIS, and NIR. CO(4+) system, C 2 Swan and CN Violet systems can be identified, as well as molecular lines for CO + and CO, and atomic lines for O and C. However, the conditions, in term of flow enthalpy and pressure, for which these spectra have been obtained, are not documented in [46].…”