The Orbiting Carbon Observatory (OCO) mission

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Spaceborne observations of ocean glint reflectance and modeling of wave slope distributions (2006, background): “On the other hand, the intense sunglint contribution is needed for retrieving atmospheric column of various gases such as water vapor [Vespérini et al., 1999; Kleidman et al., 2000] or carbon dioxide [Crisp et al., 2004].”
The Orbiting Carbon Observatory (OCO-2): spectrometer performance evaluation using pre-launch direct sun measurements (2014, background): “See Crisp et al. (2004), Pollock et al. Atmos.”
The HITRAN 2008 molecular spectroscopic database (2005, methodology): “A notable effort is the set of extensive Fourier transform spectroscopy (FTS) experiments carried out by the Jet Propulsion Laboratory (JPL) [51–58] in order to support the OCO mission [8].”
Filling-in of near-infrared solar lines by terrestrial fluorescence and other geophysical effects: simulations and space-based observations from SCIAMACHY and GOSAT (2012, positive): “The upcoming launch of the Orbiting Carbon Observatory-2 (OCO-2) (Crisp et al., 2004) will facilitate the use of solar Fraunhofer lines for ﬂuorescence retrievals at wavelengths near the O 2 -”