0000000000208036

AUTHOR

Claude Camy-peyret

showing 3 related works from this author

Model, software and database for line-mixing effects in the ν3 and ν4 bands of CH4 and tests using laboratory and planetary measurements-I: N2(and ai…

2006

International audience; Absorption spectra of the infrared ν3 and ν4 bands of CH4 perturbed by N2 over large ranges of pressure and temperature have been measured in the laboratory. A theoretical approach accounting for line mixing is proposed to (successfully) model these experiments. It is similar to that of Pieroni et al. [J Chem Phys 1999;110:7717–32] and is based on state-to-state rotational cross-sections calculated with a semi-classical approach and a few empirical parameters. The latter, which enable switching from the state space to the line space, are deduced from a fit of a single room temperature spectrum of the ν3 band at 50 atm. The comparisons between numerous measured and ca…

methane infrared spectra atmotspheric absorptionRadiationMaterials science010504 meteorology & atmospheric sciencesDatabaseAbsorption spectroscopy[PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]computer.software_genre01 natural sciencesAtomic and Molecular Physics and OpticsSpectral line010309 opticssymbols.namesakeAtmosphere of EarthFourier transform13. Climate action0103 physical sciencesRadiative transfersymbolsEmission spectrumAbsorption (electromagnetic radiation)computerSpectroscopy0105 earth and related environmental sciencesLine (formation)
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The 1997 spectroscopic GEISA databank

1999

International audience; The current version GEISA-97 of the computer-accessible database system GEISA (Gestion et Etude des Informations Spectroscopiques Atmosphériques: Management and Study of Atmospheric Spectroscopic Information) is described. This catalogue contains 1,346,266 entries. These are spectroscopic parameters required to describe adequately the individual spectral lines belonging to 42 molecules (96 isotopic species) and located between 0 and 22,656 cm-1. The featured molecules are of interest in studies of the terrestrial as well as the other planetary atmospheres, especially those of the Giant Planets. GEISA-97 contains also a catalog of absorption cross-sections of molecule…

Physics[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Radiation010504 meteorology & atmospheric sciences0103 physical sciencesAstronomy010303 astronomy & astrophysics01 natural sciencesSpectroscopyAtomic and Molecular Physics and OpticsSpectral line0105 earth and related environmental sciencesWeb site
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Inter-comparison of stratospheric O<sub>3</sub> and NO<sub>2</sub> abundances retrieved from …

2006

Abstract. Stratospheric O3 and NO2 abundances measured by different remote sensing instruments are inter-compared: (1) Line-of-sight absorptions and vertical profiles inferred from solar spectra in the ultra-violet (UV), visible and infrared (IR) wavelength ranges measured by the LPMA/DOAS (Limb Profile Monitor of the Atmosphere/Differential Optical Absorption Spectroscopy) balloon payload during balloon ascent/descent and solar occultation are examined with respect to internal consistency. (2) The balloon borne stratospheric profiles of O3 and NO2 are compared to collocated space-borne skylight limb observations of the Envisat/SCIAMACHY satellite instrument. The trace gas profiles are retr…

Atmospheric Science010504 meteorology & atmospheric sciencesDifferential optical absorption spectroscopyBalloonAtmospheric sciences01 natural sciencesOccultationTrace gasSCIAMACHY010309 opticsAtmosphereAltitude13. Climate action0103 physical sciencesEnvironmental scienceSatellite0105 earth and related environmental sciencesRemote sensingAtmospheric Chemistry and Physics
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