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Sökning: onr:"swepub:oai:research.chalmers.se:a23f8381-4ca5-4144-9d56-db2d01426717" > Comparison of HDO m...

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FältnamnIndikatorerMetadata
00004770naa a2200505 4500
001oai:research.chalmers.se:a23f8381-4ca5-4144-9d56-db2d01426717
003SwePub
008171008s2011 | |||||||||||000 ||eng|
024a https://doi.org/10.5194/amt-4-1855-20112 DOI
024a https://research.chalmers.se/publication/1461832 URI
040 a (SwePub)cth
041 a engb eng
042 9 SwePub
072 7a art2 swepub-publicationtype
072 7a ref2 swepub-contenttype
100a Lossow, Stefan,d 1977u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)lossow
2451 0a Comparison of HDO measurements from Envisat/MIPAS with observations by Odin/SMR and SCISAT/ACE-FTS
264 c 2011-09-13
264 1b Copernicus GmbH,c 2011
338 a electronic2 rdacarrier
520 a Measurements of thermal emission in the mid-infrared by Envisat/MIPAS allow the retrieval of HDO information roughly in the altitude range between 10 km and 50 km. From June 2002 to March 2004 MIPAS performed measurements in the full spectral resolution mode. To assess the quality of the HDO data set obtained during that period comparisons with measurements by Odin/SMR and SCISAT/ACE-FTS were performed. Comparisons were made on profile-to-profile basis as well as using seasonal and monthly averages. All in all the comparisons yield favourable results. The largest deviations between MIPAS and ACE-FTS are observed below 15 km, where relative deviations can occasionally exceed 100%. Despite these deviations in the absolute amount of HDO the latitudinal structures observed by both instruments are consistent in this altitude range. Between 15 km and 20 km there is less good agreement, in particular in the Antarctic during winter and spring. Also in the tropics some deviations are found. Above 20 km there is a high consistency in the structures observed by all three instruments. MIPAS and ACE-FTS typically agree within 10%, with MIPAS mostly showing higher abundances than ACE-FTS. Both data sets show considerably more HDO than SMR. This bias can be explained basically by uncertainties in spectroscopic parameters. Above 40 km, where the MIPAS HDO retrieval reaches its limits, still good agreement with the structures observed by SMR is found for most seasons. This puts some confidence in the MIPAS data at these altitudes.
650 7a NATURVETENSKAPx Geovetenskap och miljövetenskapx Meteorologi och atmosfärforskning0 (SwePub)105082 hsv//swe
650 7a NATURAL SCIENCESx Earth and Related Environmental Sciencesx Meteorology and Atmospheric Sciences0 (SwePub)105082 hsv//eng
700a Steinwagner, J.u Universiteit Utrecht,Utrecht University4 aut
700a Urban, Joachim,d 1964u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)joaurb
700a Dupuy, E.u Japan National Institute of Information and Communications Technology (NICT)4 aut
700a Boone, C. D.u University of Waterloo4 aut
700a Kellmann, S.u Karlsruher Institut für Technologie (KIT),Karlsruhe Institute of Technology (KIT)4 aut
700a Linden, A.u Karlsruher Institut für Technologie (KIT),Karlsruhe Institute of Technology (KIT)4 aut
700a Kiefer, M.u Karlsruher Institut für Technologie (KIT),Karlsruhe Institute of Technology (KIT)4 aut
700a Grabowski, U.u Karlsruher Institut für Technologie (KIT),Karlsruhe Institute of Technology (KIT)4 aut
700a Glatthor, N.u Karlsruher Institut für Technologie (KIT),Karlsruhe Institute of Technology (KIT)4 aut
700a Höpfner, M.u Karlsruher Institut für Technologie (KIT),Karlsruhe Institute of Technology (KIT)4 aut
700a Röckmann, T.u Universiteit Utrecht,Utrecht University4 aut
700a Murtagh, Donal,d 1959u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)donal
700a Walker, K. A.u University of Toronto4 aut
700a Bernath, P. F.u University of York4 aut
700a Clarmann, T. vonu Karlsruher Institut für Technologie (KIT),Karlsruhe Institute of Technology (KIT)4 aut
700a Stiller, G. P.u Karlsruher Institut für Technologie (KIT),Karlsruhe Institute of Technology (KIT)4 aut
710a Chalmers tekniska högskolab Universiteit Utrecht4 org
773t Atmospheric Measurement Techniquesd : Copernicus GmbHg 4:9, s. 1855-1874q 4:9<1855-1874x 1867-1381x 1867-8548
856u http://publications.lib.chalmers.se/records/fulltext/local_146183.pdfx primaryx freey FULLTEXT
856u https://www.atmos-meas-tech.net/4/1855/2011/amt-4-1855-2011.pdf
8564 8u https://doi.org/10.5194/amt-4-1855-2011
8564 8u https://research.chalmers.se/publication/146183

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