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@ARTICLE{Wang:47916,
      author       = {Wang, D. Y. and Stiller, G. P. and von Clarmann, T. and
                      Fischer, H. and Glatthor, G. P. and Grabowski, U. and
                      Höpfner, M. and Kellmann, S. and Kiefer, M. and Linden, A.
                      and Mengistu Tsidu, G. and Milz, M. and Steck, T. and
                      Wohnsiedler, S. and Lopez-Puertas, M. and Funke, B. and
                      Gil-Lopez, S. and Kaufmann, M. and Koukouli, S. V. and
                      Murtagh, D. and Lautie, N. and Jimenez, C. and Jones, A. and
                      Eriksson, P. and Urban, J. and de la Noe, J. and Le
                      Flochmoen, E. and Dupuy, E. and Ricuad, P. and Olberg, M.
                      and Frisk, U. and Russel III, J. and Remsberg, E.},
      title        = {{C}omparison of {MIPAS}/{ENVISAT} ozone profiles with
                      {SMR}/{ODIN} and {HALOE}/{UARS} observations},
      journal      = {Advances in space research},
      volume       = {36},
      issn         = {0273-1177},
      address      = {Amsterdam [u.a.]},
      publisher    = {Elsevier Science},
      reportid     = {PreJuSER-47916},
      pages        = {927 - 931},
      year         = {2005},
      note         = {Record converted from VDB: 12.11.2012},
      abstract     = {Ozone volume mixing ratio (VMR) profiles are measured by
                      the Michelson Interferometer for passive atmospheric
                      sounding (MIPAS) on ENVISAT. The data sets produced by the
                      science data processor at Institut fur Meteorologic und
                      Klimaforschung (IMK), Germany are compared with those
                      obtained by halogen occultation experiment (HALOE) on UARS
                      and by sub-millimetre radiometer (SMR) on ODIN. For the
                      stratospheric measurements taken during September/October
                      2002, the three instruments show reasonable agreement, with
                      global mean differences within 0.1-0.3 ppmv. The typical
                      zonal mean differences are of 0.4 ppmv for HALOE and 0.6
                      ppmv for SMR $(4-6\%)$ in the ozone VMR peak region at 25-30
                      km near the equator, though larger differences of 0.8-1 ppmv
                      $(8-10\%)$ are also observed in a small latitude-altitude
                      region in the tropic. A positive bias of about 0.2-0.4 ppmv
                      in the MIPAS data in the 35-40 km region has also been
                      found. Further studies are under way to explain these
                      differences. (c) 2005 COSPAR. Published by Elsevier Ltd. All
                      rights reserved.},
      keywords     = {S (WoSType)},
      cin          = {ICG-I},
      ddc          = {520},
      cid          = {I:(DE-Juel1)VDB47},
      pnm          = {Chemie und Dynamik der Geo-Biosphäre},
      pid          = {G:(DE-Juel1)FUEK257},
      shelfmark    = {Engineering, Aerospace / Astronomy $\&$ Astrophysics /
                      Geosciences, Multidisciplinary / Meteorology $\&$
                      Atmospheric Sciences},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000235478400021},
      doi          = {10.1016/j.asr.2005.03.015},
      url          = {https://juser.fz-juelich.de/record/47916},
}