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dc.contributor.authorMuller, C.
dc.date1985
dc.date.accessioned2017-06-27T10:36:13Z
dc.date.available2017-06-27T10:36:13Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/5854
dc.descriptionAn upper limit to the atmospheric acetonitrile mixing ratio of 3.2 X 10-1 is deduced from the high resolution Kitt Peak infrared atlas of the solar spectrum. The survey of the spectral region of CH3CN main absorption shows only stratospheric ozone lines and one water vapor line and does not permit any positive identification of acetonitrile.
dc.languageeng
dc.titleAcetonitrile in the earth's atmosphere: An upper limit deduced from infrared solar spectra
dc.typeArticle
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.source.titleBulletin de la Classe des Sciences de l'Académie Royale de Belgique 5e Série
dc.source.volume71
dc.source.issue5
dc.source.page225-229
Orfeo.peerreviewedYes
dc.identifier.doi10.3406/barb.1985.61268


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