000819931 001__ 819931
000819931 005__ 20240712100842.0
000819931 0247_ $$2Handle$$a2128/12816
000819931 0247_ $$2ISSN$$a1866-1793
000819931 020__ $$a978-3-95806-178-1
000819931 037__ $$aFZJ-2016-05505
000819931 041__ $$aEnglish
000819931 1001_ $$0P:(DE-Juel1)156366$$aZhu, Yajun$$b0$$eCorresponding author$$ufzj
000819931 245__ $$aAtomic oxygen derived from SCIAMACHY O($^{1}$S) and OH airglow measurements in the Mesopause region$$f- 2016-10-31
000819931 260__ $$aJülich$$bForschungszentrum Jülich GmbH Zentralbibliothek, Verlag$$c2016
000819931 300__ $$a206 S.
000819931 3367_ $$2DataCite$$aOutput Types/Dissertation
000819931 3367_ $$2ORCID$$aDISSERTATION
000819931 3367_ $$2BibTeX$$aPHDTHESIS
000819931 3367_ $$02$$2EndNote$$aThesis
000819931 3367_ $$0PUB:(DE-HGF)11$$2PUB:(DE-HGF)$$aDissertation / PhD Thesis$$bphd$$mphd$$s1479214857_787
000819931 3367_ $$2DRIVER$$adoctoralThesis
000819931 4900_ $$aSchriften des Forschungszentrums Jülich Reihe Energie & Umwelt / Energy & Environment$$v340
000819931 502__ $$aUniversität Wuppertal, Diss., 2016$$bDr.$$cUniversität Wuppertal$$d2016
000819931 520__ $$aAtomic 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.
000819931 536__ $$0G:(DE-HGF)POF3-244$$a244 - Composition and dynamics of the upper troposphere and middle atmosphere (POF3-244)$$cPOF3-244$$fPOF III$$x0
000819931 536__ $$0G:(DE-Juel1)HITEC-20170406$$aHITEC - Helmholtz Interdisciplinary Doctoral Training in Energy and Climate Research (HITEC) (HITEC-20170406)$$cHITEC-20170406$$x1
000819931 650_7 $$xDiss.
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000819931 9141_ $$y2016
000819931 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)156366$$aForschungszentrum Jülich$$b0$$kFZJ
000819931 9131_ $$0G:(DE-HGF)POF3-244$$1G:(DE-HGF)POF3-240$$2G:(DE-HGF)POF3-200$$3G:(DE-HGF)POF3$$4G:(DE-HGF)POF$$aDE-HGF$$bErde und Umwelt$$lAtmosphäre und Klima$$vComposition and dynamics of the upper troposphere and middle atmosphere$$x0
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