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@PHDTHESIS{Zhu:819931,
      author       = {Zhu, Yajun},
      title        = {{A}tomic oxygen derived from {SCIAMACHY} {O}($^{1}${S}) and
                      {OH} airglow measurements in the {M}esopause region},
      volume       = {340},
      school       = {Universität Wuppertal},
      type         = {Dr.},
      address      = {Jülich},
      publisher    = {Forschungszentrum Jülich GmbH Zentralbibliothek, Verlag},
      reportid     = {FZJ-2016-05505},
      isbn         = {978-3-95806-178-1},
      series       = {Schriften des Forschungszentrums Jülich Reihe Energie $\&$
                      Umwelt / Energy $\&$ Environment},
      pages        = {206 S.},
      year         = {2016},
      note         = {Universität Wuppertal, Diss., 2016},
      abstract     = {Atomic oxygen plays a crucial role in the photochemistry
                      and energy balance of the mesopause region. In particular,
                      it is the most abundant reactive species and an important
                      quantity in the derivation of temperature, ozone and other
                      constituents in this part of the atmosphere. This work deals
                      with the derivation of the atomic oxygen abundance from
                      SCIAMACHY (Scanning Imaging Absorption spectro Meter for
                      Atmospheric CHartographY) O($^{1}$S) green line and OH(9-6)
                      band nightglow measurements from 2003 to 2011. There are two
                      different photochemical models available, which describe
                      O($^{1}$S) green line volume emission rates, namely the ETON
                      and Khomich models. Differences between the two models and
                      their implicationon the derivation of atomic oxygen
                      abundance are discussed. Two atomic oxygen datasets are
                      derived from SCIAMACHY O($^{1}$S) greenline measurements at
                      90–105 km. Analyses are performed on abundance
                      uncertainties owing to rate constants and background
                      atmosphere (i.g.,temperature and total density), as well as
                      abundance differences (up to around 20\%) arising from the
                      different model schemes. One photochemical model is used to
                      simulate SCIAMACHY OH(9-6) band measurements and the
                      resulting atomic oxygen abundance is derived at 80–96 km.
                      Induced abundance uncertainties, as a result of
                      uncertainties in rate constants and background atmosphere,
                      are 20\% at 80 km, which rise intensively up to 90\% at 96
                      km.},
      cin          = {IEK-7},
      cid          = {I:(DE-Juel1)IEK-7-20101013},
      pnm          = {244 - Composition and dynamics of the upper troposphere and
                      middle atmosphere (POF3-244) / HITEC - Helmholtz
                      Interdisciplinary Doctoral Training in Energy and Climate
                      Research (HITEC) (HITEC-20170406)},
      pid          = {G:(DE-HGF)POF3-244 / G:(DE-Juel1)HITEC-20170406},
      typ          = {PUB:(DE-HGF)11},
      url          = {https://juser.fz-juelich.de/record/819931},
}