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@ARTICLE{Zhu:877783,
      author       = {Zhu, Yajun and Kaufmann, Martin and Chen, Qiuyu and Xu,
                      Jiyao and Gong, Qiucheng and Liu, Jilin and Wei, Daikang and
                      Riese, Martin},
      title        = {{A} comparison of {OH} nightglow volume emission rates as
                      measured by {SCIAMACHY} and {SABER}},
      journal      = {Atmospheric measurement techniques},
      volume       = {13},
      number       = {6},
      issn         = {1867-8548},
      address      = {Katlenburg-Lindau},
      publisher    = {Copernicus},
      reportid     = {FZJ-2020-02450},
      pages        = {3033 - 3042},
      year         = {2020},
      abstract     = {Hydroxyl (OH) short-wave infrared emissions arising from
                      OH(4-2, 5-2, 8-5, 9-6) as measured by channel 6 of the
                      SCanning Imaging Absorption spectroMeter for Atmospheric
                      CHartographY (SCIAMACHY) are used to derive concentrations
                      of OH(v=4, 5, 8, and 9) between 80 and 96 km. Retrieved
                      concentrations are used to simulate OH(5-3, 4-2) integrated
                      radiances at 1.6 µm and OH(9-7, 8-6) at 2.0 µm as
                      measured by the Sounding of the Atmosphere using Broadband
                      Emission Radiometry (SABER) instrument, which are not fully
                      covered by the spectral range of SCIAMACHY measurements. On
                      average, SABER “unfiltered” data are on the order of
                      $40 \%$ at 1.6 µm and $20 \%$ at 2.0 µm larger
                      than the simulations using SCIAMACHY data. “Unfiltered”
                      SABER data are a product, which accounts for the shape,
                      width, and transmission of the instrument's broadband
                      filters, which do not cover the full ro-vibrational bands of
                      the corresponding OH transitions. It is found that the
                      discrepancy between SCIAMACHY and SABER data can be reduced
                      by up to $50 \%,$ if the filtering process is carried out
                      manually using published SABER interference filter
                      characteristics and the latest Einstein coefficients from
                      the HITRAN database. Remaining differences are discussed
                      with regard to model parameter uncertainties and radiometric
                      calibration.},
      cin          = {IEK-7},
      ddc          = {550},
      cid          = {I:(DE-Juel1)IEK-7-20101013},
      pnm          = {244 - Composition and dynamics of the upper troposphere and
                      middle atmosphere (POF3-244)},
      pid          = {G:(DE-HGF)POF3-244},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000541482200001},
      doi          = {10.5194/amt-13-3033-2020},
      url          = {https://juser.fz-juelich.de/record/877783},
}