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GOMOS validation

dc.contributor.authorKyrölä, E.
dc.contributor.authorTamminen, J.
dc.contributor.authorSofieva, V.
dc.contributor.authorHassinen, S.
dc.contributor.authorLeppelmeier, G.W.
dc.contributor.authorBertaux, J.L.
dc.contributor.authorHauchecorne, A.
dc.contributor.authorDalaudier, F.
dc.contributor.authorCot, C.
dc.contributor.authorFanton d'Andon, O.
dc.contributor.authorBarrot, G.
dc.contributor.authorMangin, A.
dc.contributor.authorGuirlet, M.
dc.contributor.authorTheodore, B.
dc.contributor.authorKoopman, R.
dc.contributor.authorFraisse, R.
dc.contributor.authorFussen, D.
dc.contributor.authorVanhellemont, F.
dc.date2003
dc.date.accessioned2017-05-03T10:48:49Z
dc.date.available2017-05-03T10:48:49Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/5148
dc.descriptionGOMOS (Global Ozone Monitoring by Occultation of Stars) on Envisat measures ozone, NO2, NO3, H2O, aerosols, neutral air density, and temperature in the stratosphere and mesosphere by detecting the absorption of starlight in UV, visible and infrared wavelengths. During bright limb conditions GOMOS also observes scattered solar radiation. GOMOS will deliver ozone concentration profiles at altitudes 15-100 km with a vertical resolution of about 1.5 km and with a global coverage. As a self-calibrating method stellar occultation measurements provide a basis for a long-term monitoring of ozone profiles. We will present results achieved during the first year of the GOMOS validation program. The validation is based on comparisons with Mars, ozone sondes, balloon borne instruments, other satellites as well as with climatological and meteorological data.
dc.languageeng
dc.titleGOMOS validation
dc.typeConference
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.subject.freeAtmospheric aerosols
dc.subject.freeAtmospheric density
dc.subject.freeAtmospheric temperature
dc.subject.freeCalibration
dc.subject.freeClimatology
dc.subject.freeInfrared radiation
dc.subject.freeLight absorption
dc.subject.freeNitrogen oxides
dc.subject.freeOzone
dc.subject.freeScattering
dc.subject.freeSolar radiation
dc.subject.freeUltraviolet radiation
dc.subject.freeUpper atmosphere
dc.subject.freeStellar occultation
dc.subject.freeSpectrometers
dc.source.titleInternational Geoscience and Remote Sensing Symposium (IGARSS)
dc.source.volume2
dc.source.page1365-1367
Orfeo.peerreviewedNo
dc.identifier.doi10.1109/IGARSS.2003.1294110
dc.identifier.scopus2-s2.0-0242711406


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