Long-term behavior of the concentration of the minor constituents in the mesosphere-a model study

dc.bibliographicCitation.firstPage2779eng
dc.bibliographicCitation.issue8eng
dc.bibliographicCitation.journalTitleAtmospheric Chemistry and Physicseng
dc.bibliographicCitation.volume9eng
dc.contributor.authorGrygalashvyly, M.
dc.contributor.authorSonnemann, G.R.
dc.contributor.authorHartogh, P.
dc.date.accessioned2020-08-11T08:32:52Z
dc.date.available2020-08-11T08:32:52Z
dc.date.issued2009
dc.description.abstractWe investigate the influence the rising concentrations of methane, nitrous oxide and carbon dioxide which have occurred since the pre-industrial era, have had on the chemistry of the mesosphere. For this investigation we use our global 3-D-model COMMA-IAP which was designed for the exploration of the MLT-region and in particular the extended mesopause region. Assumptions and approximations for the trends in the Lyman-flux (needed for the water vapor dissociation rate), methane and the water vapor mixing ratio at the hygropause are necessary to accomplish this study. To approximate the solar Lyman-α flux back to the pre-industrial time, we derived a quadratic fit using the sunspot number record which extends back to 1749 and is the only solar proxy available for the Lyman-α flux prior to 1947. We assume that methane increases with a constant growth rate from the pre-industrial era to the present. An unsolved problem for the model calculations consists of how the water vapor mixing ratio at the hygropause should be specified during this period. We assume that the hygropause was dryer during pre-industrial times than the present. As a consequence of methane oxidation, the model simulation indicates that the middle atmosphere has become more humid as a result of the rising methane concentration, but with some dependence on height and with a small time delay of few years. The solar influence on the water vapor mixing ratio is insignificant below about 80 km in summer high latitudes, but becomes increasingly more important above this altitude. The enhanced water vapor concentration increasesthe hydrogen radical concentration and reduces the mesospheric ozone. A second region of stronger ozone decrease is located in the vicinity of the stratopause. Increases in CO2 concentration enhance slightly the concentration of CO in the mesosphere. However, its influence upon the chemistry is small and its main effect is connected with a cooling of the upper atmosphere. The long-term behavior of water vapor is discussed in particular with respect to its impact on the NLC region.eng
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://doi.org/10.34657/4077
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/5448
dc.language.isoengeng
dc.publisherGöttingen : Copernicuseng
dc.relation.doihttps://doi.org/10.5194/acp-9-2779-2009
dc.relation.issn1680-7316
dc.rights.licenseCC BY 3.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/eng
dc.subject.ddc550eng
dc.subject.otheratmospheric chemistryeng
dc.subject.othercarbon dioxideeng
dc.subject.otherconcentration (composition)eng
dc.subject.othermesosphereeng
dc.subject.othermethaneeng
dc.subject.othermixing ratioeng
dc.subject.othernitrous oxideeng
dc.subject.otherwater vaporeng
dc.titleLong-term behavior of the concentration of the minor constituents in the mesosphere-a model studyeng
dc.typeArticleeng
dc.typeTexteng
tib.accessRightsopenAccesseng
wgl.contributorIAPeng
wgl.subjectGeowissenschafteneng
wgl.typeZeitschriftenartikeleng
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