OMEGA: Observatoire pour la Minéralogie, l'Eau, les Glaces et l'Activité

By J. Bibring, A. Soufflot, M. Berthe, Y. Langevin, B. Gondet, P. Drossart, M. Bouye, M. Combès, P. Puget, A. Semery and 33 more. 2004

315 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/d1b94c79699046f3ec811aa0888345337b6a60ea

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Citations in the corpus

Global investigation of olivine on Mars: Insights into crust and mantle compositions (2013, methodology): “[8] OMEGA consists of an infrared whisk-broom system coupled to a “visible” push-broom one, resulting in the measurement of surface radiance from 0.3 to 5.2mm [Bibring et al., 2004, 2005].”
CRISM multispectral summary products: Parameterizing mineral diversity on Mars from reflectance (2007, methodology): “…validity of the above approach using data from the Mars Express (MEX) Observatoire pour la Mineralogie, l’Eau, les Glaces, et l’Activité (OMEGA) instrument, a visible to near-infrared imaging spectrometer with spatial and spectral coverage similar to that of CRISM [Bibring et al., 2004b, 2005].”
Martian surface mineralogy from Observatoire pour la Minéralogie, l'Eau, les Glaces et l'Activité on board the Mars Express spacecraft (OMEGA/MEx): Global mineral maps (2007, background): “These investigations are presented in several other papers that reveal unique regional mineralogical units (e.g., phyllosilicates in Mawrth Vallis and olivine/phyllosilicate in Nili Fossae).”
Hydration state of the Martian surface as seen by Mars Express OMEGA: 2. H2O content of the surface (2007, methodology): “0148-0227/07/2006JE002853$09.00 E08S07 1 of 15 [3] The wavelength range of OMEGA (0.38–5.1 mm) [Bibring et al., 2004] includes the fundamental symmetric and asymmetric H2O stretches centered near 2.9 mm, the overtone of the H2O bend at 3.1 mm (fundamental bend at 6 mm), and additional overtone and…”
Quantifying absolute water content of minerals using near‐infrared reflectance spectroscopy (2005, methodology): “…Mars Express and NASA’s Mars Reconnaissance Orbiter (MRO), will utilize visible-near-infrared (VIS-NIR) spectrometers (OMEGA and CRISM, respectively) [Bibring et al., 2004; Murchie et al., 2003] to retrieve global coverage high spatial and spectral resolution reflectance data of the surface of…”
Observations of the south seasonal cap of Mars during recession in 2004–2006 by the OMEGA visible/near‐infrared imaging spectrometer on board Mars Express (2007, methodology): “Such analyses have already been performed on OMEGA data for the south perennial cap [Bibring et al., 2004a; Douté et al., 2007], the north perennial cap [Langevin et al., 2005], the north seasonal cap [Schmitt et al., 2005] and the ‘‘cryptic region’’ of the south seasonal cap [Langevin et al.,…”