Search results for "HITRAN"

showing 8 items of 8 documents

The partition sum of methane at high temperature

2008

11 pages, 4 Tables, 3 Figures Computer code on line at http://icb.u-bourgogne.fr/JSP/TIPS.jsp; International audience; The total internal partition function of methane is revisited to provide reliable values at high temperature. A multi-resolution approach is used to perform a direct summation over all the rovibrational energy levels up to the dissociation limit. A computer code is executable on line at the URL : http://icb.u-bourgogne.fr/JSP/TIPS.jsp to allow the calculation of the partition sum of methane at temperatures up to 3000 K. It also provides detailed information on the density of states in the relevant spectral ranges. The recommended values include uncertainty estimates. It is …

Computational spectroscopyRovibrational spectroscopy33.20.Vq 33.70.Fd01 natural sciences[PHYS.PHYS.PHYS-AO-PH] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]MethaneDissociation (chemistry)chemistry.chemical_compound0103 physical sciencesSpectroscopy010303 astronomy & astrophysicsSpectroscopySpectroscopic databasesPhysics[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Radiation010304 chemical physicsPartition sumRotational–vibrational spectroscopyPartition function (mathematics)Atmospheric temperature rangeAtomic and Molecular Physics and OpticsComputational physicschemistry[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Density of statesHITRANAtomic physicsMethane
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XTDS and SPVIEW: Graphical tools for the analysis and simulation of high-resolution molecular spectra

2008

International audience; XTDS is a Java front-end to the different programs implementing the tensorial formalism developed in the Dijon group [see for instance: V. Boudon, J.-P. Champion, T. Gabard, M. Loëte, F. Michelot, G. Pierre, M. Rotger, Ch. Wenger, M. Rey, J. Mol. Spectrosc. 228 (2004) 620–634 ]. It allows the simulation and analysis of polyad systems for molecules of various symmetries (Td and Oh spherical tops like CH4 and SF6, C2v and C4v quasi-spherical tops like SO2F2 and SF5Cl, D2h molecules like C2H4). SPVIEW is a multiplatform Java application that allows graphical assignment of high-resolution molecular spectra. It is possible to load, display and manipulate experimental and …

JavaComputer scienceTensorial formalism02 engineering and technologyASCII01 natural sciencesGraphical toolsSpectral lineComputational scienceSoftware0103 physical sciencesGraphical interfaceAnalysis and simulationPhysical and Theoretical ChemistrySpectroscopyGraphical user interfacecomputer.programming_language[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]010304 chemical physicsbusiness.industrySpectrum assignment021001 nanoscience & nanotechnologyAtomic and Molecular Physics and Optics[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Homogeneous spaceHITRAN0210 nano-technologybusinesscomputer
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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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Filament-induced visible-to-mid-IR supercontinuum in a ZnSe crystal: Towards multi-octave supercontinuum absorption spectroscopy

2016

Abstract We report on the generation of multiple-octave supercontinuum laser source spanning from 0.5 μm to 11 μm induced by multi-filamentation in a ZnSe crystal. The generated supercontinuum is both spatially and spectrally characterized. It is then exploited in a proof-of-principle experiment for methane spectroscopy measurements by means of the supercontinuum absorption spectroscopy technique. The entire absorption spectrum is successfully recorded within the whole spectral bandwidth of the supercontinuum. Experimental results are in fairly good agreement with the HITRAN database, confirming the reliability and stability over several hours of the generated supercontinuum.

Materials scienceAbsorption spectroscopybusiness.industryOrganic Chemistry02 engineering and technology021001 nanoscience & nanotechnologyOctave (electronics)01 natural sciencesAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsSupercontinuum010309 opticsInorganic ChemistryCrystalProtein filamentOptics0103 physical sciencesOptoelectronicsHITRANElectrical and Electronic EngineeringPhysical and Theoretical Chemistry0210 nano-technologySpectroscopybusinessSpectroscopyOptical Materials
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Self-broadening coefficients and improved line intensities for the ν7 band of ethylene near 10.5μm, and impact on ethylene retrievals from Jungfraujo…

2014

Relying on high-resolution Fourier transform infrared (FTIR) spectra, the present work involved extensive measurements of individual line intensities and self-broadening coefficients for the ν7 band of 12C2H4. The measured self-broadening coefficients exhibit a dependence on both J and Ka. Compared to the corresponding information available in the latest edition of the HITRAN spectroscopic database, the measured line intensities were found to be higher by about 10% for high J lines in the P branch and lower by about 5% for high J lines of the R branch, varying between these two limits roughly linearly with the line positions. The impact of the presently measured line intensities on retrieva…

RadiationEthyleneMaterials science010504 meteorology & atmospheric sciencesSolar spectraInfraredAnalytical chemistry01 natural sciencesAtomic and Molecular Physics and OpticsSpectral linechemistry.chemical_compoundsymbols.namesakeNuclear magnetic resonanceFourier transformchemistry0103 physical sciencessymbolsHITRANFourier transform infrared spectroscopy010303 astronomy & astrophysicsSpectroscopy0105 earth and related environmental sciencesLine (formation)Journal of Quantitative Spectroscopy and Radiative Transfer
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The HITRAN2016 molecular spectroscopic database

2017

This paper describes the contents of the 2016 edition of the HITRAN molecular spectroscopic compilation. The new edition replaces the previous HITRAN edition of 2012 and its updates during the intervening years. The HITRAN molecular absorption compilation is composed of five major components: the traditional line-by-line spectroscopic parameters required for high-resolution radiative-transfer codes, infrared absorption cross-sections for molecules not yet amenable to representation in a line-by-line form, collision-induced absorption data, aerosol indices of refraction, and general tables such as partition sums that apply globally to the data. The new HITRAN is greatly extended in terms of …

SQL010504 meteorology & atmospheric sciencesRelational databaseComputer sciencePhysique atomique et moléculaireMolecular spectroscopycomputer.software_genre01 natural sciencesHITRANMolecular absorptionCollision-induced Absorption0103 physical sciencesRadiative transferChimieCollision-induced absorption[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Experimentelle Verfahren010303 astronomy & astrophysics[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]SpectroscopyComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciencescomputer.programming_languageAerosols[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]RadiationSpectroscopic database[ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]DatabaseApplication programming interfaceSpectroscopic line parametersRotation formalisms in three dimensionsMolecular spectroscopyAtomic and Molecular Physics and OpticsSpectroscopie [électromagnétisme optique acoustique][ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]HITRANAbsorption cross-sectionscomputerMolecular absorption
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Error propagation from line parameters to spectra simulations. Illustration on high temperature methane.

2010

Astrophysical investigations generally need both complete and accurate spectroscopic databases. Despite continuous efforts in experimental and theoretical spectroscopic investigations, the lack of data in some spectral regions of interest is one of the main limitation of the presently available spectroscopic databases. Unfortunately information about missing data relevant to specific experimental conditions is rarely directly accessible from spectroscopic databases (focusing naturally on available data). Such information relies essentially on theoretical investigations which are equally limited to the present state of the art of modelling. The purpose of the talk is to show how multi-resolu…

[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph][ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]13. Climate actionHITRANmolecular spectroscopymethaneabsorption coefficientAstronomical spectroscopyerror propagation[PHYS.PHYS.PHYS-AO-PH] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]
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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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