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@ARTICLE{Funke:57978,
      author       = {Funke, B. and López-Puertas, M. and Bermejo-Pantaleón, D.
                      and von Clarmann, T. and Stiller, G. P. and Höpfner, M. and
                      Grabowski, U. and Kaufmann, M.},
      title        = {{A}nalysis of nonlocal thermodynamic equilibrium {CO} 4.7 m
                      fundamental, isotopic, and hot band emissions measured by
                      the {M}ichelson {I}nterferometer for {P}assive {A}tmospheric
                      {S}ounding on {E}nvisat},
      journal      = {Journal of Geophysical Research},
      volume       = {112},
      issn         = {0148-0227},
      address      = {Washington, DC},
      publisher    = {Union},
      reportid     = {PreJuSER-57978},
      pages        = {D11305},
      year         = {2007},
      note         = {Record converted from VDB: 12.11.2012},
      abstract     = {[1] Nonlocal thermodynamic equilibrium (non-LTE)
                      simulations of the (CO)-C-12-O-16(1 -> 0) fundamental band,
                      the (CO)-C-12-O-16(2 -> 1) hot band, and the isotopic
                      (CO)-C-13-O-16(1 -> 0) band performed with the Generic
                      Radiative Transfer and non-LTE population Algorithm
                      (GRANADA) and the Karlsruhe Optimized and Precise Radiative
                      Transfer Algorithm (KOPRA) have been compared to spectrally
                      resolved 4.7 mu m radiances measured by the Michelson
                      Interferometer for Passive Atmospheric Sounding (MIPAS). The
                      performance of the non-LTE simulation has been assessed in
                      terms of band radiance ratios in order to avoid a
                      compensation of possible non-LTE model errors by retrieval
                      errors in the CO abundances inferred from MIPAS data with
                      the same non-LTE algorithms. The agreement with the
                      measurements is within $5\%$ for the fundamental band and
                      within $10\%$ for the hot band. Simulated (CO)-C-13-O-16
                      radiances agree with the measurements within the
                      instrumental noise error. Solar reflectance at the surface
                      or clouds has been identified as an important additional
                      excitation mechanism for the CO( 2) state. The study
                      represents a thorough validation of the non-LTE scheme used
                      in the retrieval of CO abundances from MIPAS data.},
      keywords     = {J (WoSType)},
      cin          = {ICG-1},
      ddc          = {550},
      cid          = {I:(DE-Juel1)VDB790},
      pnm          = {Atmosphäre und Klima},
      pid          = {G:(DE-Juel1)FUEK406},
      shelfmark    = {Meteorology $\&$ Atmospheric Sciences},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000247141200003},
      doi          = {10.1029/2006JD007933},
      url          = {https://juser.fz-juelich.de/record/57978},
}