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dc.contributor.authorFussen, D.
dc.contributor.authorVanhellemont, F.
dc.contributor.authorDodion, J.
dc.contributor.authorBingen, C.
dc.contributor.authorWalker, K.A.
dc.contributor.authorBoone, C.D.
dc.contributor.authorMcLeod, S.D.
dc.contributor.authorBernath, P.F.
dc.date2005
dc.date.accessioned2016-12-07T10:36:06Z
dc.date.available2016-12-07T10:36:06Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/4618
dc.descriptionThe ozone and nitrogen dioxide vertical number density prrofiles measured by the solar occultation Fourier transform spectrometer ACE-FTS and the UV-Vis stellar occultation instrument GOMOS are intercompared for 370 quasi-coincident observations. A good agreement is found for ozone, mostly better than 10% between 15 and 45 km. Also, there is no evidence for a systematic altitude registration error in the ACE-FTS profiles. A considerable ACE-FTS negative bias (50-100%) is found however for the nitrogen dioxide data that cannot be explained by the use of a local photochemical model.
dc.languageeng
dc.titleInitial intercomparison of ozone and nitrogen dioxide number density profiles retrieved by the ACE-FTS and GOMOS occultation experiments
dc.typeArticle
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.subject.freeFourier transform infrared spectroscopy
dc.subject.freeMathematical models
dc.subject.freeNitrogen oxides
dc.subject.freeOzone
dc.subject.freeSpectrometers
dc.subject.freeUltraviolet instruments
dc.subject.freeAtmospheric chemistry experiment
dc.subject.freeFourier transform spectrometer
dc.subject.freeUV-VIs stellar occultation
dc.subject.freeAtmospheric chemistry
dc.subject.freeatmospheric chemistry
dc.subject.freenitrogen dioxide
dc.subject.freeozone
dc.source.titleGeophysical Research Letters
dc.source.volume32
dc.source.issue16
dc.source.pageL16S02
Orfeo.peerreviewedYes
dc.identifier.doi10.1029/2005GL022468
dc.identifier.scopus2-s2.0-25844495267


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