High-resolution spectroscopy and analysis ...
Type de document :
Article dans une revue scientifique: Article original
Titre :
High-resolution spectroscopy and analysis of the ν<sub>2</sub> + ν<sub>3</sub> combination band of SF<sub>6</sub> in a supersonic jet expansion
Auteur(s) :
Boudon, Vincent [Auteur]
Laboratoire Interdisciplinaire Carnot de Bourgogne [ICB]
Asselin, Pierre [Auteur]
Laboratoire de Dynamique Interactions et Réactivité [LADIR]
Soulard, Pascale [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Goubet, Manuel [Auteur]
Physique Moléculaire aux Interfaces [PMI]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Huet, Therese [Auteur]
Physique Moléculaire aux Interfaces [PMI]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Georges, Robert [Auteur]
Institut de Physique de Rennes [IPR]
Pirali, Olivier [Auteur]
Institut des Sciences Moléculaires d'Orsay [ISMO]
Synchrotron SOLEIL [SSOLEIL]
Roy, Pascal [Auteur]
Synchrotron SOLEIL [SSOLEIL]
Laboratoire Interdisciplinaire Carnot de Bourgogne [ICB]
Asselin, Pierre [Auteur]
Laboratoire de Dynamique Interactions et Réactivité [LADIR]
Soulard, Pascale [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Goubet, Manuel [Auteur]

Physique Moléculaire aux Interfaces [PMI]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Huet, Therese [Auteur]

Physique Moléculaire aux Interfaces [PMI]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Georges, Robert [Auteur]
Institut de Physique de Rennes [IPR]
Pirali, Olivier [Auteur]
Institut des Sciences Moléculaires d'Orsay [ISMO]
Synchrotron SOLEIL [SSOLEIL]
Roy, Pascal [Auteur]
Synchrotron SOLEIL [SSOLEIL]
Titre de la revue :
Molecular Physics
Pagination :
2154-2162
Éditeur :
Taylor & Francis
Date de publication :
2013-05-10
ISSN :
0026-8976
Mot(s)-clé(s) en anglais :
sulphur hexafluoride
greenhouse gas
infrared absorption
supersonic jet expansion
tensorial formalism
greenhouse gas
infrared absorption
supersonic jet expansion
tensorial formalism
Discipline(s) HAL :
Physique [physics]/Physique [physics]/Agrégats Moléculaires et Atomiques [physics.atm-clus]
Physique [physics]/Physique [physics]/Chimie-Physique [physics.chem-ph]
Physique [physics]/Physique [physics]/Chimie-Physique [physics.chem-ph]
Résumé en anglais : [en]
Sulphur hexafluoride is a very strong greenhouse gas whose concentration is increasing in the atmosphere. It is detected through infrared absorption spectroscopy in the strong ν<sub>3</sub> fundamental region. Due to the ...
Lire la suite >Sulphur hexafluoride is a very strong greenhouse gas whose concentration is increasing in the atmosphere. It is detected through infrared absorption spectroscopy in the strong ν<sub>3</sub> fundamental region. Due to the existence of low-lying vibrational states of this molecule, however, many hot bands arise at room temperature and those are still not known. We present here a contribution to the elucidation of this hot band structure, by analysing the ν<sub>2</sub> + ν<sub>3</sub> combination band. We use a supersonic jet expansion high-resolution spectrum at a rotational temperature of ca. 25 K that was recorded thanks to the Jet-AILES setup at the Source Optimisée de Lumière d'Energie Intermédiaire du LURE (SOLEIL) Synchrotron. The simplified structure of this cold spectrum allowed us to assign 444 rovibrational lines and to fit effective Hamiltonian parameters, leading to a very satisfactory spectrum simulation. The parameters obtained in this way allow to calculate the spectrum of the ν<sub>3</sub>+ν<sub>2</sub>−ν<sub>2</sub> hot band.Lire moins >
Lire la suite >Sulphur hexafluoride is a very strong greenhouse gas whose concentration is increasing in the atmosphere. It is detected through infrared absorption spectroscopy in the strong ν<sub>3</sub> fundamental region. Due to the existence of low-lying vibrational states of this molecule, however, many hot bands arise at room temperature and those are still not known. We present here a contribution to the elucidation of this hot band structure, by analysing the ν<sub>2</sub> + ν<sub>3</sub> combination band. We use a supersonic jet expansion high-resolution spectrum at a rotational temperature of ca. 25 K that was recorded thanks to the Jet-AILES setup at the Source Optimisée de Lumière d'Energie Intermédiaire du LURE (SOLEIL) Synchrotron. The simplified structure of this cold spectrum allowed us to assign 444 rovibrational lines and to fit effective Hamiltonian parameters, leading to a very satisfactory spectrum simulation. The parameters obtained in this way allow to calculate the spectrum of the ν<sub>3</sub>+ν<sub>2</sub>−ν<sub>2</sub> hot band.Lire moins >
Langue :
Anglais
Comité de lecture :
Oui
Audience :
Internationale
Vulgarisation :
Non
Source :