[PDF][PDF] The CO Cameron bands in the Mars dayglow and aurora: consequences of revised cross sections
The spin-forbidden CO a 3Π-> X1σ Cameron bands (190-270 nm) are the dominant feature
of the middle ultraviolet spectrum of the Martian dayglow and aurora. Since their discovery in …
of the middle ultraviolet spectrum of the Martian dayglow and aurora. Since their discovery in …