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@ARTICLE{Kaufmann:29689,
      author       = {Kaufmann, M. and Gusev, O. A. and Grossmann, K. U. and
                      Martín-Torres, F. J. and Marsh, D. R. and Kutepov, A. A.},
      title        = {{S}atellite observations of daytime and nighttime ozone in
                      the mesosphere and lower thermosphere},
      journal      = {Journal of geophysical research / Atmospheres},
      volume       = {108},
      issn         = {0022-1406},
      address      = {Washington, DC},
      publisher    = {Union},
      reportid     = {PreJuSER-29689},
      pages        = {D9},
      year         = {2003},
      note         = {Record converted from VDB: 12.11.2012},
      abstract     = {[1] The global distribution of mesospheric and lower
                      thermospheric ozone 9.6 mum infrared emissions was measured
                      by the Cryogenic Infrared Spectrometers and Telescopes for
                      the Atmosphere (CRISTA) experiment during two Space Shuttle
                      missions in November 1994 and August 1997. The radiances
                      measured by CRISTA have been inverted to O-3 number
                      densities in the 50-95 km range by using a nonlocal
                      thermodynamic equilibrium model. A detailed sensitivity
                      study of retrieved O-3 number densities has been carried
                      out. The ozone abundance profiles show volume mixing ratios
                      of 1-2 ppmv at the stratopause, 0.5 ppmv or less around 80
                      km, and typically 1 ppmv during daytime and 10 ppmv during
                      nighttime at the secondary maximum. The agreement with other
                      experiments is typically better than $25\%.$ The global
                      distribution of upper mesospheric ozone shows significant
                      latitudinal gradients and an enhancement in the equatorial
                      upper mesosphere. At the polar night terminator a third
                      ozone maximum is observed. Three-dimensional model results
                      indicate that the latitudinal gradients are significantly
                      influenced by solar tides.},
      keywords     = {J (WoSType)},
      cin          = {ICG-I},
      ddc          = {550},
      cid          = {I:(DE-Juel1)VDB47},
      pnm          = {Chemie und Dynamik der Geo-Biosphäre},
      pid          = {G:(DE-Juel1)FUEK257},
      shelfmark    = {Meteorology $\&$ Atmospheric Sciences},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000182874800002},
      doi          = {10.1029/2002JD002800},
      url          = {https://juser.fz-juelich.de/record/29689},
}