0000000000930145

AUTHOR

J.-b. Brubach

showing 2 related works from this author

Self and N-2 collisional broadening of far-infrared methane lines measured at the SOLEIL synchrotron

2012

International audience; Following our recent study devoted to measurements of intensities of pure rotation lines of methane, room temperature far infrared spectra of methane diluted in nitrogen at five total pressures between 100 and 800 hPa have been recorded at the AILES beamline of the SOLEIL synchrotron. One hundred and five N-2 broadening coefficients of methane pure rotation lines have been measured in the 83-261 cm(-1) spectral range using multi-spectrum non-linear least squares fitting of Voigt profiles. Pressure-induced line shifts were not needed to fit the spectra to the noise level and line mixing effects were neglected. One hundred and seventy-six self broadening coefficients h…

Materials science010504 meteorology & atmospheric sciencesWIDTHSSynchrotron radiationchemistry.chemical_elementNU(4) BANDTRANSITIONS01 natural sciences7. Clean energySpectral lineMethanelaw.inventionsymbols.namesakechemistry.chemical_compoundFar infraredRETRIEVALSlaw0103 physical sciencesSPECTRAL REGION(CH4)-C-12010303 astronomy & astrophysicsTEMPERATURESpectroscopy0105 earth and related environmental sciences[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]RadiationDIODE-LASER SPECTROSCOPYCM(-1)NitrogenAtomic and Molecular Physics and OpticsSynchrotronBeamlinechemistry[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]13. Climate actionsymbolsSHIFT COEFFICIENTSAtomic physicsTitan (rocket family)
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The high-resolution far-infrared spectrum of methane at the SOLEIL synchrotron

2010

International audience; As a tetrahedral molecule, methane has no permanent dipole moment. Its spectrum, however, displays faint absorption lines in the THz region, due to centrifugal distorsion effects. This is important for planetary applications since this region is used to measure methane concentration in some planetary atmospheres, in particular on Titan. Up to now, all measurements relied either on some old low resolution infrared absorption spectra, or on high resolution Stark measurements for low J values only. Even if these results have been reexamined recently [E. H. Wishnow, G. S. Orton, I. Ozier and H. P. Gush, J. Quant. Spectrosc. Radiat. Transfer 103, 102-117 (2007)], it seeme…

010504 meteorology & atmospheric sciencesAbsorption spectroscopyAnalytical chemistrySynchrotron radiationFar infrared7. Clean energy01 natural sciencesSpectral linelaw.inventionOpticsFar infraredlaw0103 physical sciencesAbsorption (logic)010303 astronomy & astrophysicsSpectroscopy0105 earth and related environmental sciencesPhysicsRadiationSynchrotron radiationbusiness.industryResolution (electron density)BremsstrahlungAtomic and Molecular Physics and OpticsSynchrotron[CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistry13. Climate action[ CHIM.THEO ] Chemical Sciences/Theoretical and/or physical chemistrybusinessTitanMethaneLine intensities
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