Model calculation of the [OI] 630 nm dayglow and [OI] 557.7 nm dayglow limb intensity for two different solar zenith angles (30 and 70 degrees) at aphelion and perihelion, and their measurements by TGO/NOMAD
Description
This dataset contains vertical profile of [OI] 630 nm and [OI] 557.7 nm dayglow intensity simulated by a theoretical model and measured with TGO/NOMAD-UVIS.
These are presented as Figure 4 in Gérard, J. C., Aoki, S., Gkouvelis, L., Soret, L., Willame, Y., Thomas, I. R., et al. (2021). First observation of the oxygen 630 nm emission in the Martian dayglow. Geophysical Research Letters, 48(8), e2020GL092334. https://doi.org/10.1029/2020GL092334