Search results for "SHIFT COEFFICIENTS"

showing 4 items of 4 documents

Applications of a new set of methane line parameters to the modeling of Titan's spectrum in the 1.58 μm window

2012

International audience; In this paper we apply a recently released set of methane line parameters (Wang et al., 2011) to the modeling of Titan spectra in the 1.58 mu m window at both low and high spectral resolution. We first compare the methane absorption based on this new set of methane data to that calculated from the methane absorption coefficients derived in situ from DISR/Huygens (Tomasko et al., 2008a; Karkoschka and Tomasko, 2010) and from the band models of Irwin et al. (2006) and Karkoschka and Tomasko (2010). The Irwin et al. (2006) band model clearly underestimates the absorption in the window at temperature-pressure conditions representative of Titan's troposphere, while the Ka…

010504 meteorology & atmospheric sciencesInfraredCASSINI VIMSHUYGENS PROBEMONODEUTERATED METHANEAtmospheric sciences01 natural sciences7. Clean energyMethaneSpectral lineTropospherechemistry.chemical_compoundsymbols.namesake0103 physical sciencesSpectral resolutionSpectroscopy010303 astronomy & astrophysicsCLOUD STRUCTURE0105 earth and related environmental sciencesPhysics[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]Astronomy and Astrophysics9500 CM(-1)SPECTROSCOPIC DATABASEM TRANSPARENCY WINDOWComputational physicsAerosolchemistry[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]TEMPERATURE-DEPENDENCE13. Climate actionSpace and Planetary SciencesymbolsSHIFT COEFFICIENTSOUTER SOLAR-SYSTEMTitan (rocket family)
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Collisional Broadening of Rotational Lines in the Stimulated Raman Pentad Q-Branch of CD4

1992

Self- and argon-broadening coefficients are reported for a number of Raman Q-branch transitions in the nu(1) and nu(2) + nu(4) bands of (C-12)D4 at room temperature (296 K). The coefficients display a variation with j and with C exp n (symmetry species A, E, F) that is essentially independent of collision partner and which is similar to the j- and C exp n-dependence found in previous measurements of the IR line-broadening coefficients. The rotationally inelastic collision rates previously measured by Foy et al. (1988) for (C-13)D4 (V4 = 0, 1) in collision with (C-13)D4 or Ar account for only a part of the Raman broadening rate, suggesting possibly significant contributions to the linewidths…

DephasingInelastic collision02 engineering and technologyLORENTZ WIDTH01 natural sciencesLOW-TEMPERATURESSpectral linesymbols.namesakeNuclear magnetic resonance0103 physical sciencesSPECTRAStimulated ramanPhysicsTUNABLE-DIODE-LASERRadiationSPECTROSCOPY010304 chemical physicsINFRARED DOUBLE-RESONANCESpectral bands021001 nanoscience & nanotechnologyAtomic and Molecular Physics and OpticsSymmetry (physics)METHANE LINESCM-1 REGIONsymbolsSHIFT COEFFICIENTSAtomic physics0210 nano-technologyRaman spectroscopyENERGY-TRANSFER
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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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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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