0000000000022216

AUTHOR

Tony Gabard

showing 40 related works from this author

2nu3 band of 12CF4 and its simultaneous analysis with nu3

1995

Abstract A nearly Doppler-limited spectrum of the 2ν 3 band of the 12 CF 4 molecule between 2536.0 and 2599.8 cm −1 was recorded at T = 77 K using difference-frequency laser spectroscopy. The simultaneous analysis of the ground (G.S.), ν 3 = 1, and ν 3 = 2 states was performed using an isolated band model to sixth order in the tetrahedral formalism. Fourteen hundred seventy-five transitions were assigned through J = 35 to the F 2 and E vibrational components of the ν 3 = 2 level. A total of 1864 transition frequencies were fit simultaneously (1000 2ν 3 - G.S. newly assigned transitions together with 575 ν 3 - G.S. and 289 ν 3 - ν 3 transitions already reported in the literature). The ground…

Physics[PHYS]Physics [physics]010304 chemical physicsSixth orderOvertone band010402 general chemistry01 natural sciencesAtomic and Molecular Physics and Optics0104 chemical sciencesFormalism (philosophy of mathematics)0103 physical sciencesMoleculePhysical and Theoretical ChemistryAtomic physicsGround stateSpectroscopySpectroscopy
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Nitrogen broadening of SF6 transitions in the nu3 band

2001

Abstract Nitrogen induced pressure-broadened halfwidths of a number of ν3 transitions of SF6 are calculated using the complex Robert–Bonamy (CRB) formalism. The calculations are made at 200, 250, 296 and 350 K and the temperature dependence of the halfwidths are determined. The intermolecular potential is taken as a sum of the leading electrostatic and Lennard-Jones [6] , [7] , [8] , [9] , [10] , [11] , [12] atom–atom components. The dynamics of the collision process are correct to second order in time. The calculated halfwidths are used to simulate the ν3 spectrum, which is compared to a simulation made using the HITRAN96 halfwidths and measurements made at the Universite Pierre et Marie C…

010504 meteorology & atmospheric sciences[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Organic Chemistrychemistry.chemical_elementSulfur hexafluoride01 natural sciencesNitrogenAnalytical ChemistryMarie curieInorganic ChemistrySulfur hexafluoridechemistry.chemical_compoundFormalism (philosophy of mathematics)chemistry[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencesIntermolecular potentialTemperature dependence of the halfwidthHalfwidthsAtomic physicsLine broadening010306 general physicsSpectroscopy0105 earth and related environmental sciences
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Calculated helium-broadened line parameters in the nu4 band of 13CH4

1998

International audience; Helium line-broadening coefficients for transitions in the nu4 band of 13CH4 have been calculated using a semi-classical model. This model is analogous to the one that we have used in a previous study on argon line-broadening coefficients for transitions in the nu3 band of 12CH4. For the present study, over 270 room temperature measurements were considered. The J, symmetry and fine structure dependences of the data are satisfactorily reproduced, although deficiencies of the semi-classical model are evidenced.

RadiationArgonMaterials science010304 chemical physicschemistry.chemical_element01 natural sciencesTemperature measurementAtomic and Molecular Physics and OpticsSymmetry (physics)chemistry0103 physical sciencesAtomic physics010306 general physicsSpectroscopyHeliumLine (formation)
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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 methane Raman spectrum from 1200 to 5500 cm(-1): A first step toward temperature diagnostic using methane as a probe molecule in combustion syste…

2005

International audience; We present a study of the spontaneous Raman spectra of (CH4)-C-12 from 1200 to 5500 cm(-1) at various temperatures. This study is of interest from a fundamental as well as from a practical point of view with regards to the temperature diagnostic in hydrocarbon combustion. The present investigation shows that the spontaneous (CH4)-C-12 Raman spectra are very sensitive to temperature and that the complexity of methane spectra is not an obstacle to use methane as a probe molecule in laser-diagnostic techniques. Our study consists in determining the polarisability parameters of methane (CH4)-C-12, unknown at the present time, from spontaneous Raman spectra recorded at pr…

Materials scienceAnalytical chemistry02 engineering and technologyCombustion01 natural sciences7. Clean energyTemperature measurementMethaneSpectral linesymbols.namesakechemistry.chemical_compoundNuclear magnetic resonance(CH4)-C-12Coherent anti-Stokes Raman spectroscopyPhysical and Theoretical ChemistryRamanSpectroscopyPropellant[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]methane010401 analytical chemistrypolarisability021001 nanoscience & nanotechnologyAtomic and Molecular Physics and Optics0104 chemical scienceschemistry13. Climate actionsymbolsCombustion chamber0210 nano-technologyRaman spectroscopytensorial formalismtemperature measurement
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N2-, O2- and air-broadened half-widths and line shifts for transitions in the nu3 band of methane in the 2726- to 3200-cm-1 spectral region

2008

International audience; Complex Robert-Bonamy calculations of the pressure-broadened half-width and the pressure-induced line shift are made for some 4000 transitions in the [nu]3 band of methane with N2, O2, and air as the perturbing gases. This work focuses on A and F symmetry transitions in the spectral range 2726 to 3200 cm-1. More work is needed on the intermolecular potential before calculations can be made for the E-symmetry transitions. The calculations are made at 225 and 296 K in order to determine the temperature dependence of the half-width. The calculations are compared with measurements. These data are to support remote sensing of the Earth and Titan atmospheres.

Work (thermodynamics)Range (particle radiation)Materials science010504 meteorology & atmospheric sciences7. Clean energy01 natural sciencesAtomic and Molecular Physics and OpticsSpectral lineSymmetry (physics)Methane[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]010309 opticssymbols.namesakechemistry.chemical_compoundchemistry0103 physical sciencessymbols[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Physical and Theoretical ChemistryAtomic physicsTitan (rocket family)SpectroscopyEarth (classical element)0105 earth and related environmental sciencesLine (formation)
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Model, software and database for line-mixing effects in the nu3 and nu4 bands of CH4 and tests using laboratory and planetary measurements - II : H2 …

2006

International audience; The absorption shapes of the nu(2), nu(3) and nu(4) infrared bands of CH4 perturbed by H-2 in large ranges of pressure and temperature have been measured in the laboratory. In order to model these spectra, the theoretical approach accounting for line-mixing effects proposed for CH4-N-2 and CH4-air and successfully tested in the companion paper (1), is used. As before, state-to-state rotational rates are used together with some empirical parameters that are deduced from a fit of a single room temperature spectrum of the nu(3) band at about 50 atm. The comparisons between measured and calculated spectra in the nu(3) and nu(4) regions under a vast variety of conditions …

Spectral shape analysis010504 meteorology & atmospheric sciencesInfraredcomputer.software_genre01 natural sciences7. Clean energyJovianSpectral line0103 physical sciencesRadiative transferAbsorption (electromagnetic radiation)Spectroscopy0105 earth and related environmental sciencesLine (formation)Physics[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Radiation010304 chemical physicsSpectrometerDatabasemethane infrared spectraAtomic and Molecular Physics and Optics[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]13. Climate actionAstrophysics::Earth and Planetary Astrophysicscomputergiant planets emission
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Symmetry-adapted tensorial formalism to model rovibrational and rovibronic spectra of molecules pertaining to various point groups

2004

International audience; We present a short review on the tensorial formalism developed by the Dijon group to solve molecular spectroscopy problems. This approach, originally devoted to the rovibrational spectroscopy of highly symmetrical species (spherical tops) has been recently extended in several directions: quasi-spherical tops, some symmetric and asymmetric tops, and rovibronic spectroscopy of spherical tops in a degenerate electronic state. Despite its apparent complexity (heavy notations, quite complex mathematical tools), these group theoretical tensorial methods have a great advantage of flexibility: a systematic expansion of effective terms for any rovib- rational/rovibronic probl…

[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Rovibrational spectroscopyRovibronic spectroscopySymmetrizationTensorial formalism02 engineering and technologyMolecular spectroscopyPoint group01 natural sciencesSpectral lineTheoretical physics[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]Quantum mechanics0103 physical sciencesPhysics::Atomic and Molecular ClustersMoleculeLineshapesPhysical and Theoretical ChemistrySpectroscopySpectroscopyPhysics010304 chemical physicsDegenerate energy levelsRotational–vibrational spectroscopy021001 nanoscience & nanotechnologyAtomic and Molecular Physics and OpticsFormalism (philosophy of mathematics)Group theory0210 nano-technology
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Speed-dependent broadening and line mixing in CH4 perturbed by Ar and N2 from multispectrum fits

2000

International audience; Speed-dependent broadenings and shifts have been determined for the P and R branches of the nu3 band of CH4 perturbed by Ar and N2 using a multispectrum fitting analysis of high-resolution tunable difference-frequency laser spectra recorded at pressures 3, the tetrahedral fine structure components in each J manifold are collisionally coupled and exhibit significant interference. The coupled lines are treated using a speed-dependent first-order line-mixing profile and are compared to a speed-independent full relaxation matrix inversion procedure with off-diagonal coupling elements calculated from an atom-atom Lennard-Jones potential model.

RadiationMaterials science010504 meteorology & atmospheric sciences[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Laser01 natural sciencesAtomic and Molecular Physics and OpticsSpectral linelaw.invention[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]law0103 physical sciencesTetrahedronRelaxation matrixAtomic physics010306 general physicsSpectroscopy0105 earth and related environmental sciences
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Line broadening coefficient calculations for methane perturbed by nitrogen

2010

Abstract We report semiclassical line broadening calculations for methane perturbed by nitrogen at room temperature. For this, we have developed a symmetrized version of the Robert and Bonamy theory. The interaction potential was built from electrostatic (octopole and hexadecapole for methane, quadrupole for nitrogen) and atom–atom contributions. The relative (classical) trajectories of the molecules were computed in the frame of the usual parabolic model, through analytical formula. High orders of developments had to be used for the short range molecular interactions. As a consequence, a combination of symbolic computation and source code generation was employed to implement practical calc…

Line broadening coefficients010504 meteorology & atmospheric sciencesAbsorption spectroscopyNitrogenSemiclassical physics7. Clean energy01 natural sciencesSpectral lineMethanechemistry.chemical_compound0103 physical sciences[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Perturbation theoryPhysics::Chemical PhysicsSpectroscopy010303 astronomy & astrophysicsInfrared spectroscopySpectroscopy0105 earth and related environmental sciencesLine (formation)PhysicsRadiationAtomic and Molecular Physics and Optics[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]chemistryQuadrupoleAtomic physicsMethane
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Measurement of rotational relaxation in the ground state of methane perturbed by argon at low temperature

1999

International audience; Relaxation processes at low temperature in methane perturbed by argon have been investigated on the basis of new measurements. Diode laser absorption spectra of methane in the region of the dyad nu2/nu4 in supersonic expansions have been recorded. The time of relaxation of the ground state mean rotational energy was derived from the observed dependences of the rotational temperature on the concentration in the jet. A semi-classical model was used to calculate the state-to-state relaxation rate constants at room temperature. The evaluation of the time of relaxation of the mean rotational energy using semi-empirical temperature dependence laws is presented and discusse…

Jet (fluid)RadiationMaterials scienceArgon010304 chemical physicsAbsorption spectroscopychemistry.chemical_elementRotational temperature010402 general chemistry01 natural sciencesAtomic and Molecular Physics and OpticsMethane0104 chemical sciencesRotational energychemistry.chemical_compoundchemistry0103 physical sciencesRelaxation (physics)Atomic physicsGround stateSpectroscopy
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Spectroscopic tools for remote sensing of greenhouse gases CH4, CF4 and SF6

2003

International audience; Highly symmetrical molecules such as CH4, CF4 or SF6 are known to be atmospheric pollutants and greenhouse gases. High-resolution spectroscopy in the infrared is particularly suitable for the monitoring of gas concentration and radiative transfers in the earth's atmosphere. This technique requires extensive theoretical studies for the modeling of the spectra of such molecules (positions, intensities and shapes of absorption lines). Here, we have developed powerful tools for the analysis and the simulation of absorption spectra of highly symmetrical molecules. These tools have been implemented in the spherical top data system (STDS) and highly-spherical top data syste…

010504 meteorology & atmospheric sciencesAbsorption spectroscopy[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Infrared01 natural sciencesSpectral lineAtmosphereSoftware[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencesRadiative transferEnvironmental ChemistryClimate changeSpectroscopy0105 earth and related environmental sciencesRemote sensingCH4010304 chemical physicsbusiness.industryChemistryCF4Molecular spectroscopyGreenhouse gases13. Climate actionGreenhouse gasbusinessSimulationSF6
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Pressure‐induced widths and shifts for the ν3 band of methane

1994

International audience; Widths and shifts of methane lines perturbed by nitrogen are calculated using a complex-valued implementation of Robert-Bonamy (RB) theory. The static intermolecular potential is described as a sum of electrostatic forces and Lennard-Jones (6-12) atom-atom terms, using literature values for all physical parameters. Vibrational dependence of the isotropic potential is obtained from the polarizability of methane assuming a dispersion interaction. The repulsive part of the Lennard-Jones accounts for the greatest part of widths, while dispersion interactions are largely responsible for shifts. Although the average error between calculated and observed linewidths (up to J…

010304 chemical physicsMathematical modelAbsorption spectroscopyIntermolecular forceIsotropyGeneral Physics and Astronomy7. Clean energy01 natural sciencesMethane010309 opticschemistry.chemical_compoundLennard-Jones potentialchemistryPolarizability0103 physical sciencesDispersion (optics)Physics::Atomic and Molecular ClustersPhysics::Chemical PhysicsPhysical and Theoretical ChemistryAtomic physicsThe Journal of Chemical Physics
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Argon-broadened line parameters in the nu3 band of 12CH4

1997

International audience; Prompted by improved measurements of collisional line shapes in the nu3 band P, Q and R branches of 12CH4, we have performed semi-classical line broadening calculations for methane perturbed by argon. We have used the theoretical approach developed by Robert and Bonamy as an extension of the well-known Anderson-Tsao-Curnutte theory. The semi-classical theory as reformulated here is shown to fully account for the tetrahedral symmetry of methane type molecules. The variation of argon-broadened linewidth coefficients in the nu3 band of 12CH4 with the branch, J, symmetry and energy level fine structure is discussed.

PhysicsRadiationArgon010304 chemical physicschemistry.chemical_elementTetrahedral symmetry01 natural sciencesAtomic and Molecular Physics and OpticsSymmetry (physics)Methane010309 opticschemistry.chemical_compoundLaser linewidthchemistry0103 physical sciencesMoleculeAtomic physicsPhysics::Chemical PhysicsSpectroscopyLine (formation)
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Methane in Titan's atmosphere: from fundamental spectroscopy to planetology

2009

The methane molecule (CH4) is relatively abundant in the Universe and in particular in our Solar System. On Earth, it is the main compound of natural gas and is also the second greenhouse gas of anthropic origin. On Saturn's satellite Titan it plays a role similar to water on Earth and leads to a complex chemistry.

Origin of water on EarthGeneral Physics and AstronomyMethane[PHYS.PHYS.PHYS-AO-PH] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Astrobiologychemistry.chemical_compoundsymbols.namesakeNatural gasPlanetologiePhysics::Chemical PhysicsAtmosphere of TitanAstrophysics::Galaxy AstrophysicsPhysics::Atmospheric and Oceanic PhysicsSpectroscopyLife on Titanbusiness.industryPlanetary sciencechemistryGreenhouse gasPhysics::Space PhysicssymbolsEnvironmental scienceAstrophysics::Earth and Planetary AstrophysicsbusinessTitan (rocket family)Titan[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Methane
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Le méthane dans l’atmosphère de Titan - De la spectroscopie fondamentale à la planétologie

2008

Le methane (CH4) joue sur Tian, le plus gros satellite de Saturne, un role similaire a celui de l'eau sur Terre. Il y est de plus a l'origine d'une chimie organique complexe. La spectroscopie etant la technique privilegiee pour mesurer le CH4 dans les atmospheres planetaires, des modeles precis de l'absorption de la lumiere par cette molecule doivent etre developpes. Les resultats recents obtenus dans ce domaine a l'Institut Carnot de Bourgogne, en collaboration etroite avec des planetologues, permettent notamment de contribuer a l'interpretation des resultats de la mission Cassini-Huygens.

General MedicineReflets de la physique
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Helium and Argon Line Broadening in the nu2 Band of CH4

2004

Abstract The spectra of the gaseous mixtures CH 4 –He and CH 4 –Ar were obtained in the spectral region 1400–1750 cm −1 with a resolution up to 0.003 cm −1 . Helium and argon pressure broadenings for the vibration–rotation lines of the ν 2 band of CH 4 have been estimated at room temperature for some lines in the P , Q , and R branches. These values were also calculated using the theoretical approach developed by Robert and Bonamy, extended to the case of tetrahedral molecules. The helium data have been found to be in a satisfactory agreement whereas a divergence of calculated and measured broadening coefficients has been evidenced in the case of argon. Simulations of the ν 2 band shapes of…

Materials science010504 meteorology & atmospheric sciences[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Physics::Instrumentation and Detectorschemistry.chemical_element01 natural sciencesMethaneSpectral linechemistry.chemical_compound[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencesPhysics::Atomic and Molecular ClustersPhysical and Theoretical ChemistryPhysics::Chemical PhysicsLine broadeningSpectroscopyHelium0105 earth and related environmental sciencesLine (formation)Argon010304 chemical physicsResolution (electron density)Tetrahedral molecular geometryAtomic and Molecular Physics and OpticschemistryVibration-rotation linesAstrophysics::Earth and Planetary AstrophysicsAtomic physicsMethane
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Estimation of line parameters under line mixing effect: the nu3 band of CH4 in helium

2001

International audience; Spectra of CH4-He mixtures were measured in the P and R branch regions of nu3 vibration-rotation band at lower pressures of 0.26-1.0 bar and for the whole band at higher pressures up to 90 bar. The line broadening coefficients were found from lower pressure data for the lines of the P branch. These coefficients were calculated in the framework of the Robert and Bonamy semi-classical approach. In general, they agree with the experimental ones, but a small J-dependent deviation was observed. Line mixing effects were observed at all pressures. At higher pressures they were interpreted in terms of the adjusted branch-coupling model. At lower pressures line mixing effects…

Materials science010504 meteorology & atmospheric sciences[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]chemistry.chemical_element01 natural sciencesSpectral lineOptics[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]Infrared gas spectra0103 physical sciencesLine broadeningSpectroscopyMixing (physics)Helium0105 earth and related environmental sciencesLine (formation)Radiation010304 chemical physicsbusiness.industryAtomic and Molecular Physics and OpticschemistryLower pressureAtomic physicsbusinessLine shiftingLine mixing effectBar (unit)
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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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Methane line parameters in HITRAN

2003

Abstract Two editions of the methane line parameters (line positions, intensities and broadening coefficients) available from HITRAN in 2000 and 2001 are described. In both versions, the spectral interval covered was the same (from 0.01 to 6184.5 cm −1 ), but the database increased from 48,033 transitions in 2000 to 211,465 lines in 2001 because weaker transitions of 12 CH 4 and new bands of 13 CH 4 and CH3D were included. The newer list became available in 2001 in the “Update” section of HITRAN. The sources of information are described, and the prospects for future improvements are discussed.

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]Physics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]Radiation010504 meteorology & atmospheric sciences01 natural sciencesAtomic and Molecular Physics and OpticsSpectral lineMethaneComputational physicschemistry.chemical_compoundchemistry0103 physical sciencesHITRANAtomic physics010303 astronomy & astrophysicsSpectroscopy0105 earth and related environmental sciencesLine (formation)Journal of Quantitative Spectroscopy and Radiative Transfer
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Near-infrared radiative transfer modelling with different CH4 spectroscopic databases to retrieve atmospheric methane total amount

2011

International audience; Atmospheric methane content can be retrieved from measurements of solar radiation attenuated by the atmosphere in the near infrared spectral region where the space-borne and ground-based spectrometers carry out regular measurements. It is shown, in the present work, that the different spectroscopic databases can give significantly different results for both forward simulations of the atmospheric transmittance and the inverse problem solution to retrieve the CH4 total content in the atmosphere using spectra measured by ground-based FTIR spectrometer in the near infrared spectral region. These discrepancies and the problem of the reduction of their influence on the atm…

Materials science010504 meteorology & atmospheric sciencesInfrared spectroscopycomputer.software_genre01 natural sciencesAtmosphereAtmospheric radiative transfer codes0103 physical sciencesRadiative transferAstrophysics::Solar and Stellar AstrophysicsPhysics::Atmospheric and Oceanic PhysicsSpectroscopySpectroscopic databases0105 earth and related environmental sciencesRadiation010304 chemical physicsSpectrometerDatabaseAtmospheric methaneNear-infrared spectroscopyAtmospheric transmissionAtomic and Molecular Physics and Optics13. Climate actionInfrared windowAstrophysics::Earth and Planetary AstrophysicsMethanecomputerJournal of Quantitative Spectroscopy and Radiative Transfer
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Calculated line broadening parameters for methane perturbed by diatomic molecules

2013

International audience; We report semiclassical line broadening calculations for methane perturbed by diatomic molecules: nitrogen, N2, oxygen, O2 and hydrogen, H2, at room temperature. For this, we have developed a symmetrized version of the Robert and Bonamy theory. The interaction potential was built from electrostatic (octopole and hexadecapole for methane, quadrupole for the diatomic molecules) and atom-atom contributions. The relative (classical) trajectories of the molecules were computed in the frame of the usual parabolic model, through analytical formula. High orders of developments had to be used for the short range molecular interactions in the case of N2 and O2. For H2, a lower…

Line broadening coefficients010504 meteorology & atmospheric sciencesHydrogen[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Nitrogenchemistry.chemical_elementInfrared spectroscopySemiclassical physics02 engineering and technology7. Clean energy01 natural sciencesMethanechemistry.chemical_compound[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]Diatomic moleculesMoleculePhysical and Theoretical ChemistryInfrared spectroscopySpectroscopy0105 earth and related environmental sciencesLine (formation)Physics021001 nanoscience & nanotechnologyDiatomic moleculeAtomic and Molecular Physics and OpticsOxygenchemistryQuadrupoleAtomic physics0210 nano-technologyMethaneHydrogen
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Hydrogen CARS thermometry in H2-N2 mixtures at high pressure and medium temperatures: influence of linewidths models

2000

International audience; In order to improve the accuracy of H2 CARS thermometry, H2 Q-branch CARS spectra have been recorded for various H2-N2 mixtures in a high-pressure cell at different pressures and temperatures (up to 40 bar and 875 K). Due to the low spectral resolution of broadband CARS experiments, the relevant spectral lineshape factor is the linewidth ratio G(Q(3))/G(Q(1)), since Q(1) and Q(3) are the most intense lines of the Q-branch spectrum in this temperature range. For the first time, the speed-inhomogeneous effects are accounted for in the simulation of the CARS profiles. The evaluated temperatures are in good agreement with reference values obtained by thermocouples. The s…

Quantum opticsMaterials sciencePhysics and Astronomy (miscellaneous)General EngineeringAnalytical chemistryGeneral Physics and Astronomychemistry.chemical_element02 engineering and technologyAtmospheric temperature range021001 nanoscience & nanotechnology01 natural sciences7. Clean energyNitrogenSpectral line010309 opticsPACS: 33.20; 42.65Laser linewidthNuclear magnetic resonancechemistryThermocouple0103 physical sciencesSpectral resolution0210 nano-technologyHydrogen CARSBar (unit)
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Calculated Line Broadening Coefficients in the nu2 Band of CH3D Perturbed by Helium

2003

International audience; Line broadening coefficients have been calculated, at room temperature, for lines in the P and R branches of the nu2 band of monodeuterated methane. A properly symmetrized semiclassical model with parabolic relative trajectories has been used. Two interaction potential models have been considered. The first is a Lennard-Jones type atom-atom potential, while the second one was derived from ab initio calculations. The calculated line widths were compared to the available experimental data and a satisfactory agreement was found, although the model contains no other adjustable parameters than the four atomic Lennard-Jones ones. Nonetheless, failures of calculations have …

PhysicsLine broadening coefficients010304 chemical physicsCondensed matter physics[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Semiclassical physicschemistry.chemical_elementQuantum numberSemiclassical calculations01 natural sciences7. Clean energyAtomic and Molecular Physics and OpticsCH3DInteraction potentialchemistry[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]Ab initio quantum chemistry methods0103 physical sciencesPhysics::Atomic and Molecular ClustersPhysical and Theoretical ChemistryAtomic physics010303 astronomy & astrophysicsSpectroscopyHeliumLine (formation)
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CARS spectroscopy of CH4 for implication of temperature measurements in supercritical LOX/CH4 combustion

2007

International audience; Experimental and theoretical investigations of coherent anti-Stokes Raman spectroscopy of CH4 have been carried out. Experimental spectra were measured in a heated high-pressure test cell and compared with numerical simulations. Good agreement was obtained for the temperature and the pressure dependence of CARS spectra in the ranges 300-1100 K and 0.1-5.0 MPa. The observed dependencies provide useful guidance for CARS thermometry, allowing quantitative measurements of temperature in high-pressure combustors. Application of multiplex CH4 CARS thermometry for single-shot measurements in a LOX/CH4 combustion at high pressure was demonstrated at supercritical conditions …

CH4 spectroscopyMaterials scienceAnalytical chemistryAerospace EngineeringCombustion01 natural sciences7. Clean energyTemperature measurementSpectral lineMethane010305 fluids & plasmas010309 opticssymbols.namesakechemistry.chemical_compoundNuclear magnetic resonancesupercritical pressure0103 physical sciencesLOX/CH4 combustionSpectroscopy[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]temperatureSupercritical fluidchemistrysymbolscoherent anti-Stokes Raman scatteringLiquid oxygenRaman spectroscopyAerospace Science and Technology
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Line parameters and shapes of high clusters: R-branch of the nu3 band of CH4 in He mixtures

2002

International audience; The IR absorption spectra of CH4 in pure gas and in mixture with helium were studied in the region of nu3 band at higher J line clusters R(17)-R(22). The frequencies and intensities of rotation-vibration lines were estimated from the experimental spectra at Doppler shape conditions. The line frequencies and intensities were calculated and used for the attribution of overlapped lines in clusters. The calculated line intensities are close to the experimental values. The calculated frequency structure of the higher J manifolds are somewhat wider than the observed one. The shapes of helium-broadened line clusters were compared with those calculated accounting for line mi…

010504 meteorology & atmospheric sciences[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]chemistry.chemical_elementSemiclassical physics01 natural sciencesSpectral linesymbols.namesakeLine parameters[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencesRelaxation matrixSpectroscopyMixing (physics)Helium0105 earth and related environmental sciencesLine (formation)PhysicsRadiationIr absorption010304 chemical physicsVibration-rotation spectraLine mixingAtomic and Molecular Physics and OpticschemistrysymbolsAtomic physicsDoppler effectMethane
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Experimental and theoretical study of line mixing in methane spectra. III. The Q branch of the Raman ν1 band

2000

The shape of the ν1 Raman Q branch of CH4 perturbed by Ar and He at room temperature has been studied. Stimulated Raman spectroscopy (SRS) experiments have been made in the 2915–2918 cm−1 spectral region for total pressures from 0.4 to 70 atm and mixtures of ≈5% CH4 with He and Ar. Analysis of the spectra demonstrates that the shape of the Q branch is significantly influenced by line mixing and much narrower than what is predicted by the addition of individual line profiles. For the first time, a model is proposed for the calculation and analysis of the effects of collisions on the considered spectra. In this approach, the rotational part of the relaxation matrix is constructed, with no adj…

ChemistryAnalytical chemistryGeneral Physics and AstronomySemiclassical physicsSpectral linesymbols.namesakesymbolsCoherent anti-Stokes Raman spectroscopyPhysical and Theoretical ChemistryAtomic physicsRaman spectroscopySpectroscopyMixing (physics)Raman scatteringLine (formation)The Journal of Chemical Physics
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Spherical Top Theory and Molecular Spectra

2011

In this article, we present an overview of the present state of the art of the theory of high-resolution spherical-top spectra in the framework of the effective Hamiltonian approach. We describe the specific features of this class of molecules to explain the basic concepts of the theoretical methods used for the analysis (line positions and intensities) and the simulation of absorption (including pure rotation) and Raman spectra of such species. The non conventional formalism that we use is essentially based on irreducible tensor methods and is especially adapted to computational treatments and global analyses of complex interacting band systems. We give examples concerning mainly methane (…

sulfur hexafluoride010504 meteorology & atmospheric sciences[PHYS.PHYS.PHYS-GEN-PH] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]group theory01 natural sciencesSpectral linerovibronic spectrasymbols.namesakeTheoretical physicsSpherical-topsvibrational polyads0103 physical sciencesMolecule[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Physics::Chemical PhysicsSpectroscopy0105 earth and related environmental sciences010304 chemical physicsChemistrymethaneRotational–vibrational spectroscopy[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Homogeneous spacesymbolsextension to lower symmetriescollisional broadeningprograms and databasesAtomic physicsHamiltonian (quantum mechanics)Raman spectroscopyrovibrational spectroscopytensorial formalismGroup theory
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Multispectrum fits for line mixing in the ν3 band Q branch of methane

2003

International audience; First-order line-mixing coefficients and model relaxation matrix element scaling factors have been obtained for allowed transitions in the nu3 band Q branch of CH4 broadened by H2, He, N2, O2, Ar, and CH4. The broadening, shifting, Dicke-narrowing, and line-mixing parameters are determined by simultaneous least-squares fitting of spectra at pressures from 0.014 to 66.66 kPa recorded with a high-resolution difference-frequency laser. These results confirm, improve, and extend a previous analysis of the lower pressure (613.3 kPa) data [A.S. Pine, J. Chem. Phys. 97 (1992) 773] which yielded averaged coefficients of individually fit spectra where adjacent broadened lines…

[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]010504 meteorology & atmospheric sciencesSelf and foreign gas-broadened methane01 natural sciencesMethaneSpectral linelaw.inventionchemistry.chemical_compoundNuclear magnetic resonance[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]law0103 physical sciencesRelaxation matrixPhysical and Theoretical Chemistry010306 general physicsScalingSpectroscopyMixing (physics)0105 earth and related environmental sciencesLine (formation)PhysicsLine mixingLaserAtomic and Molecular Physics and OpticschemistryDicke narrowingLower pressureAtomic physicsJournal of Molecular Spectroscopy
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Methane line parameters in the HITRAN2012 database

2013

International audience; The compilation of methane molecular line parameters was updated to include new global analyses and measurements for 12CH4, 13CH4 and 12CH3D. Over 70% of the methane parameters in HITRAN2008 were replaced; existing parameters retained were the microwave lines and the Dyad of 13CH4 near 7 μm and ν6 of 13CH3D near 8.7 μm, 12CH3D (7-4076 cm-1), hot bands of 12CH4 (1887-3370 cm-1) and normal sample CH4 (4800-5550 cm-1 and 8000-9200 cm-1). With a minimum intensity at 296 K in units of cm-1/(molecule cm-2) set to 10-37 for the far-IR and 10-29 for the mid- and near-IR, the methane database increased from 290,091 lines in HITRAN2008 to 468,013 lines, and three-fourths of th…

Materials science010504 meteorology & atmospheric sciencesPlanetscomputer.software_genre01 natural sciencesSpectral lineMethaneCavity ring-down spectroscopy010309 opticschemistry.chemical_compoundLine parameters0103 physical sciencesIsotopologueSpectroscopy0105 earth and related environmental sciencesLine (formation)[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]RadiationDatabaseDifferential optical absorption spectroscopyExoplanetsRemote sensingAtomic and Molecular Physics and OpticschemistryHITRAN databaseAtomic physicsGround statecomputerMethaneMicrowaveJournal of Quantitative Spectroscopy and Radiative Transfer
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CARS methane spectra: Experiments and simulations for temperature diagnostic purposes

2007

International audience; CARS laboratory experiments were done in the 2905-2925 cm(-1) range, in the vicinity of the v, band of the methane molecule, for pressures ranging from I to 50 bar, and temperatures up to 1100 K. These experiments were carried out in order to retrieve the pressure evolution of the CH4 spectrum, as well as to confirm its temperature dependance. After a brief recall on the theory used to compute pressure broadening coefficients and relaxation rates, we consider the v(3) and v(4) infrared bands of methane for benchmark calculations purposes. Next, we present recent experimental CARS spectra and calculated ones. Lastly, we discuss flame experiments as well as comparisons…

Materials scienceInfrared010402 general chemistryCombustion7. Clean energy01 natural sciencesTemperature measurementMethaneSpectral linechemistry.chemical_compoundsymbols.namesakeline-mixingNuclear magnetic resonancepressure broadening0103 physical sciences(CH4)-C-12CARSPhysical and Theoretical ChemistryRamanSpectroscopy[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]010304 chemical physicsmethaneRelaxation (NMR)Atomic and Molecular Physics and Optics0104 chemical sciencesComputational physicschemistry13. Climate actionsymbolsRaman spectroscopytemperature measurementBar (unit)combustion
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Le méthane dans l'atmosphère de Titan. De la spectroscopie fondamentale à la planétologie

2008

Le méthane (CH4) joue sur Tian, le plus gros satellite de Saturne, un rôle similaire à celui de l'eau sur Terre. Il y est de plus à l'origine d'une chimie organique complexe. La spectroscopie étant la technique privilégiée pour mesurer le CH4 dans les atmosphères planétaires, des modèles précis de l'absorption de la lumière par cette molécule doivent être développés. Les résultats récents obtenus dans ce domaine à l'Institut Carnot de Bourgogne, en collaboration étroite avec des planétologues, permettent notamment de contribuer à l'interprétation des résultats de la mission Cassini-Huygens.

Sciences de la matière et technologiemethaneméthaneTitanspectroscopie[PHYS.PHYS.PHYS-AO-PH] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Planétologie
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Nanotubes de carbone alignés synthétisés par CCVD : optimisation de rendement de synthèse et extension sur grandes surfaces pour matériaux multifonct…

2014

International audience

[CHIM.MATE] Chemical Sciences/Material chemistry[CHIM.MATE]Chemical Sciences/Material chemistryComputingMilieux_MISCELLANEOUS
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Etat de l'Art des Analyses Raie par Raie des Spectres du Méthane

2008

[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph][CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistry[PHYS.ASTR.EP] Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP][CHIM.THEO] Chemical Sciences/Theoretical and/or physical chemistry[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph][ PHYS.ASTR.EP ] Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP][PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP][ CHIM.THEO ] Chemical Sciences/Theoretical and/or physical chemistry[SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP][SDU.ASTR.EP] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP][ SDU.ASTR.EP ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP][PHYS.PHYS.PHYS-AO-PH] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]
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The methane Raman spectrum up to 5500 cm-1. Application to the diagnostic of temperature in combustion media

2005

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]
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Self and N2 Collisional Broadening of Methane in the THz Region Measured at the SOLEIL Synchrotron

2011

[CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistry[CHIM.THEO] Chemical Sciences/Theoretical and/or physical chemistry[ CHIM.THEO ] Chemical Sciences/Theoretical and/or physical chemistry
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Experimental and theoretical study of line mixing in methane spectra. III. The Q branch of the Raman nu(1) band

2000

International audience; The shape of the nu(1) Raman Q branch of CH4 perturbed by Ar and He at room temperature has been studied. Stimulated Raman spectroscopy (SRS) experiments have been made in the 2915-2918 cm(-1) spectral region for total pressures from 0.4 to 70 atm and mixtures of approximate to 5% CH4 with He and Ar. Analysis of the spectra demonstrates that the shape of the Q branch is significantly influenced by line mixing and much narrower than what is predicted by the addition of individual line profiles. For the first time, a model is proposed for the calculation and analysis of the effects of collisions on the considered spectra. In this approach, the rotational part of the re…

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]SUM-RULESNITROGEN[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]PERTURBER DEPENDENCIESDENSITYPRESSURE-SHIFT COEFFICIENTS(CH4)-C-12CO2 INFRARED-SPECTRANU(3) BANDTEMPERATUREPARAMETERS
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Etude des effets collisionnels dans les molécules tétraédriques. Applications au méthane perturbé par l'argon

1996

This thesis is devoted to the study of relaxational and collisional line-broadening processes in the first vibrational polyads of tetrahedral molecules. In a first part, the particular internal dynamics of such molecules is discussed. The second chapter reviews the literature on phenomena induced by intermolecular interactions involving this type of molecules. More theoretical aspects are developed in the second part. The so-called tetrahedral tensorial formalism adapted to the construction of Hamiltonians and transition moments of tetrahedral molecules is described. Main features of the infrared line-shapes theories and of semi-classical line-broadening and line-shifting calculations are a…

[PHYS]Physics [physics]Symétrie tétraédriqueCollisional broadeningMéthaneRelaxation rotationnelle[ PHYS ] Physics [physics]Formalisme tensorielRotational relaxationTetrahedral symmetryTensorial formalismSélectivité[PHYS] Physics [physics]Modèle semi-classiqueSelectivityArgonSemi-classical modelElargissement collisionnel
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Femtosecond Raman Spectroscopy of C2H4 and CH4 molecules

2006

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]
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Near-Infrared Radiative Transfer Modeling with Different CH4 Databases to Retrieve Atmospheric Methane Total Amount

2010

[CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistry[CHIM.THEO] Chemical Sciences/Theoretical and/or physical chemistry[PHYS.ASTR.EP] Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP][ PHYS.ASTR.EP ] Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP][PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP][ CHIM.THEO ] Chemical Sciences/Theoretical and/or physical chemistry[SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP][SDU.ASTR.EP] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP][ SDU.ASTR.EP ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]
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