“…, graphs3,5,6,8,9,11,12,14,15,18,18,20,21), there is the observed appearance of O 24 Σg − →4 Πu and H α 3 → 2[13]. In the ultraviolet region, a CO (B 3 Σ → B 3 Π) spectrum (graphs 7-21) is observed at 283.3 nm (unmarked), which could be counted as proof of intense production of CO.From the graphs, it can be seen that it reaches up to 3000 counts for BG 20/80 composition (graph 19).…”