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CO 2 pressure broadening and shift coefficients for the 1-0 band of HCl and DCl

dc.contributor.authorTudorie, M.
dc.contributor.authorFoldes, T.
dc.contributor.authorVandaele, A.C.
dc.contributor.authorVander Auwera, J.
dc.date2012
dc.date.accessioned2016-03-29T10:07:38Z
dc.date.available2016-03-29T10:07:38Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3039
dc.descriptionCO2 broadened spectra of the 1–0 band of H35Cl and H37Cl, observed near 2886 cm−1, and the 1–0 band of D35Cl and D37Cl, located near 2089 cm−1, have been recorded at room temperature and five total pressures between 150 and 700 Torr, using a Bruker IFS125HR Fourier transform spectrometer. Spectra of pure HCl were also recorded. CO2 broadening and shift coefficients of HCl and DCl have been measured using multi-spectrum non-linear least squares fitting of Voigt profiles. The analysis of the 1–0 band of DCl was complicated by the presence of overlapping CO2 bands, which were included in the treatment as absorption coefficients calculated taking line-mixing effects into account.
dc.languageeng
dc.titleCO 2 pressure broadening and shift coefficients for the 1-0 band of HCl and DCl
dc.typeArticle
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.subject.freeDeuterium chloride
dc.subject.freeHydrogen chloride
dc.subject.freePressure shift
dc.subject.freePressure-broadening
dc.subject.freeVenus atmospheres
dc.subject.freeChlorine compounds
dc.subject.freeDeuterium
dc.subject.freeInfrared radiation
dc.subject.freeCarbon dioxide
dc.subject.freecarbon dioxide
dc.subject.freechloride
dc.subject.freedeuterium
dc.subject.freeFTIR spectroscopy
dc.subject.freehydrogen
dc.subject.freeleast squares method
dc.subject.freemixing
dc.subject.freeplanetary atmosphere
dc.subject.freepressure effect
dc.subject.freetemperature effect
dc.subject.freeVenus
dc.source.titleJournal of Quantitative Spectroscopy and Radiative Transfer
dc.source.volume113
dc.source.issue11
dc.source.page1092-1101
Orfeo.peerreviewedYes
dc.identifier.doi10.1016/j.jqsrt.2012.01.025
dc.identifier.scopus2-s2.0-84860917848


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