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@ARTICLE{Smith:23764,
      author       = {Smith, A. K. and Preusse, P. and Oberheide, J.},
      title        = {{M}iddle atmosphere {K}elvin waves observed in {CRISTA} 1
                      and 2 temperature and trace species},
      journal      = {Journal of Geophysical Research},
      volume       = {107},
      issn         = {0148-0227},
      address      = {Washington, DC},
      publisher    = {Union},
      reportid     = {PreJuSER-23764},
      pages        = {D23},
      year         = {2002},
      note         = {Record converted from VDB: 12.11.2012},
      abstract     = {[1] A number of tropical perturbations that have all the
                      characteristics of Kelvin waves are identified in
                      temperature measurements from the two flights of the
                      Cryogenic Infrared Spectrometers and Telescopes for the
                      Atmosphere (CRISTA) instrument. The background wind
                      conditions during the two flights were quite different due
                      to the different phases of the quasi-biennial oscillation
                      (QBO), and there were differences in the Kelvin waves
                      observed. During each flight, there were several different
                      zonal wave numbers and/or frequencies present
                      simultaneously. The observed waves conform well to theory.
                      In particular, lower-frequency waves are confined to the
                      lower stratosphere, while higher-frequency waves appear in
                      the upper stratosphere and mesosphere; the waves are
                      centered on the equator; and the frequency and structure
                      satisfy the dispersion relation. Wave signals also appear in
                      several stratospheric trace species: O-3, CFC-11 (CFCl3),
                      HNO3, N2O, and CH4. The sense of the correlation of these
                      trace species perturbations with temperature (negative for
                      CFC-11, N2O, and CH4; positive for lower stratospheric HNO3
                      and O3) confirms that vertical velocity is responsible for
                      the perturbations. There is a shift in the relative phases
                      as photochemical processes become more important with
                      increasing altitude. Upper stratospheric ozone correlates
                      negatively with temperature due to temperature-dependent
                      reaction rates that destroy ozone.},
      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:000180490000004},
      doi          = {10.1029/2001JD000577},
      url          = {https://juser.fz-juelich.de/record/23764},
}