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- W2186253265 abstract "The (0-0) transition of the Infrared Atmospheric band system (a∆gXΣg ) of O2 at 1.27 μm was first detected in the Mars dayglow by Noxon et al. [1976]. The typical intensity of this band is about 1-30 MR [Slanger et al., 2008]. Since 2003, the SPectroscopy for the Investigation of the Atmosphere of Mars (SPICAM) experiment on board Mars Express provides systematic measurements of the emission such that a global and temporal distribution of the emission has been produced [Fedorova et al., 2006a]. Recently, the Observatoire pour la Mineralogie, l’Eau, les Glaces et l’Activite (OMEGA) instrument, also on Mars Express, observed for the first time the O2 IR emission at nighttime [Gondet et al., 2010]. The feature was also measured by the Mars Climate Sounder (MCS) on the Mars Reconnaissance Orbiter (MRO) around the same period [McCleese and Kass, 2010]." @default.
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- W2186253265 date "2010-01-01" @default.
- W2186253265 modified "2023-09-27" @default.
- W2186253265 title "SIMULATIONS OF THE O2 IR ATMOSPHERIC EMISSIONS IN THE MAR" @default.
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