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@ARTICLE{Grossmann:40885,
      author       = {Grossmann, K. U. and Gusev, O. and Kaufmann, M. and
                      Kutepov, A. and Knieling, P.},
      title        = {{A} review of the scientific results from the {CRISTA}
                      missions},
      journal      = {Advances in space research},
      volume       = {34},
      issn         = {0273-1177},
      address      = {Amsterdam [u.a.]},
      publisher    = {Elsevier Science},
      reportid     = {PreJuSER-40885},
      pages        = {1715 - 1721},
      year         = {2004},
      note         = {Record converted from VDB: 12.11.2012},
      abstract     = {The CRyogenic Infrared Spectrometers and Telescopes for the
                      Atmosphere (CRISTA) experiment measured atmospheric limb
                      infrared emissions in the altitude regime from the upper
                      troposphere to the lower thermosphere during two Shuttle
                      missions in November 1994 and August 1997. From the recorded
                      spectra trace gas densities and temperature fields were
                      derived on a very dense spatial grid. In the mesosphere and
                      lower thermosphere trace gas and temperature retrievals were
                      carried out with the help of a state of the art non-LTE
                      (non-local thermodynamic equilibrium) model coupled to a
                      line-by-line radiative transfer code. The upper atmosphere
                      data include densities of carbon dioxide, ozone, atomic
                      oxygen, and temperature. All parameters were derived for day
                      and night with the exception of CO2 which is available for
                      daytime only. Additional trace gases in the mesosphere
                      include water vapor, methane, and carbon monoxide. The main
                      findings are a substantial depletion of CO2 between 80 and
                      100 km, high ozone concentrations in the secondary maximum
                      (upper mesosphere) during night, a tertiary ozone maximum
                      near the winter polar terminator in the middle mesosphere
                      and well developed dynamically induced structures in
                      latitude as well as in longitude. Such structures are also
                      observed in the lower thermosphere where the distribution of
                      atomic oxygen was measured up to about 180 km altitude. The
                      atomic oxygen concentrations encountered in the thermosphere
                      during solar minimum are much lower than predicted by MSIS.
                      (C) 2004 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:000225594400012},
      doi          = {10.1016/j.asr.2003.02.041},
      url          = {https://juser.fz-juelich.de/record/40885},
}