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000041265 0247_ $$2DOI$$a10.1016/j.asr.2005.04.005
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000041265 084__ $$2WoS$$aEngineering, Aerospace
000041265 084__ $$2WoS$$aAstronomy & Astrophysics
000041265 084__ $$2WoS$$aGeosciences, Multidisciplinary
000041265 084__ $$2WoS$$aMeteorology & Atmospheric Sciences
000041265 1001_ $$0P:(DE-HGF)0$$aBracher, A.$$b0
000041265 245__ $$aCross comparison of O3 and NO2 measured by the atmospheric ENVISAT instruments GOMOS, MIPAS, and SCIAMACHY
000041265 260__ $$aAmsterdam [u.a.]$$bElsevier Science$$c2005
000041265 300__ $$a855 - 867
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000041265 440_0 $$09884$$aAdvances in Space Research$$v36$$x0273-1177$$y5
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000041265 520__ $$aVertical profiles Of O-3 and NO2 abundances from the atmospheric instruments GOMOS (Global Ozone Monitoring by the Occultation of Stars), MIPAS (Michelson Interferometer for Passive Atmospheric Sounding) and SCIAMACHY (Scanning Imaging Spectrometer for Atmospheric Chartography) all on-board the recently launched European Space Agency (ESA) Environmental Satellite (ENVISAT) are intercompared. These comparisons contribute to the validation of these data products by detecting systematic deviations, for example, wrong tangent height determinations, spectroscopic errors, and others. The cross comparison includes GOMOS data products retrieved by the GOMOS prototype processor from ACRI (Sophia Antipolis, France), the scientific SCIAMACHY data products from the Institute of Environmental Physics at University of Bremen (IUP) and the scientific MIPAS data products from the Institute for Meteorology and Climate Research in Karlsruhe (IMK) and Institute of Astrophysics in Andalusia (IAA). Coincident measurements were identified by limiting the time difference to 100 min (duration of one orbit) and less than 500 km between two observation points. When lower stratospheric ozone is strongly depleted during polar spring, a homogeneity condition was further imposed on the satellite measurements by requiring an upper limit on the potential vorticity difference at the 475 K isentrope between both observations. Since geographically coincident NO2 measurements of the three instruments are performed during different times of the day and NO2 has a rather strong diurnal variability, matches of NO2 profiles were compared only where the solar zenith angle difference was below 5 degrees. First results of the cross comparison show an agreement within 15% between 21 and 40 km altitude for O-3 profiles and an agreement within 20% between 27 and 40 km altitude for NO2 profiles among the GOMOS, MIPAS and SCIAMACHY measurements. (c) 2005 COSPAR. Published by Elsevier Ltd. All rights reserved.
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000041265 650_7 $$2WoSType$$aS
000041265 65320 $$2Author$$aENVISAT
000041265 65320 $$2Author$$astratosphere
000041265 65320 $$2Author$$aozone
000041265 65320 $$2Author$$aNO2
000041265 65320 $$2Author$$asatellite cross comparison
000041265 7001_ $$0P:(DE-HGF)0$$aBovensmann, H.$$b1
000041265 7001_ $$0P:(DE-HGF)0$$aBramsted, K.$$b2
000041265 7001_ $$0P:(DE-HGF)0$$aBurrows, J. P.$$b3
000041265 7001_ $$0P:(DE-HGF)0$$avon Clarmann, T.$$b4
000041265 7001_ $$0P:(DE-HGF)0$$aEichmann, K.-U.$$b5
000041265 7001_ $$0P:(DE-HGF)0$$aFischer, H.$$b6
000041265 7001_ $$0P:(DE-HGF)0$$aFunke, B.$$b7
000041265 7001_ $$0P:(DE-Juel1)VDB32256$$aGil-Lopez, S.$$b8$$uFZJ
000041265 7001_ $$0P:(DE-HGF)0$$aGlatthor, G. P.$$b9
000041265 7001_ $$0P:(DE-HGF)0$$aGrabowski, U.$$b10
000041265 7001_ $$0P:(DE-HGF)0$$aHöpfner, M.$$b11
000041265 7001_ $$0P:(DE-Juel1)129128$$aKaufmann, M.$$b12$$uFZJ
000041265 7001_ $$0P:(DE-HGF)0$$aKellmann, S.$$b13
000041265 7001_ $$0P:(DE-HGF)0$$aKiefer, M.$$b14
000041265 7001_ $$0P:(DE-HGF)0$$aKoukouli, M. E.$$b15
000041265 7001_ $$0P:(DE-HGF)0$$aLinden, A.$$b16
000041265 7001_ $$0P:(DE-HGF)0$$aLopez-Puertas, M. L.$$b17
000041265 7001_ $$0P:(DE-HGF)0$$aMengistu-Tsidu, G.$$b18
000041265 7001_ $$0P:(DE-HGF)0$$aMilz, M.$$b19
000041265 7001_ $$0P:(DE-HGF)0$$aNoel, S.$$b20
000041265 7001_ $$0P:(DE-HGF)0$$aRohen, G.$$b21
000041265 7001_ $$0P:(DE-HGF)0$$aRozanov, A.$$b22
000041265 7001_ $$0P:(DE-HGF)0$$aRozanov, V. V.$$b23
000041265 7001_ $$0P:(DE-HGF)0$$avon Savigny, C.$$b24
000041265 7001_ $$0P:(DE-HGF)0$$aSinnhuber, M.$$b25
000041265 7001_ $$0P:(DE-HGF)0$$aSkupin, J.$$b26
000041265 7001_ $$0P:(DE-HGF)0$$aSteck, T.$$b27
000041265 7001_ $$0P:(DE-HGF)0$$aStiller, G. P.$$b28
000041265 7001_ $$0P:(DE-HGF)0$$aWang, D.-Y.$$b29
000041265 7001_ $$0P:(DE-HGF)0$$aWeber, M.$$b30
000041265 7001_ $$0P:(DE-HGF)0$$aWuttke, M. W.$$b31
000041265 773__ $$0PERI:(DE-600)2023311-5$$a10.1016/j.asr.2005.04.005$$gVol. 36, p. 855 - 867$$p855 - 867$$q36<855 - 867$$tAdvances in space research$$v36$$x0273-1177$$y2005
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