How robust are trends in the Brewer-Dobson circulation derived from observed stratospheric temperatures?

dc.contributor.authorOssó Castillón, Albert
dc.contributor.authorSola Salvatierra, Yolanda
dc.contributor.authorRosenlof, Karen
dc.contributor.authorHassler, Birgit
dc.contributor.authorBech, Joan
dc.contributor.authorLorente, Jeroni
dc.date.accessioned2016-05-25T16:32:39Z
dc.date.available2016-07-01T22:01:23Z
dc.date.issued2015
dc.date.updated2016-05-25T16:32:55Z
dc.description.abstractMost global circulation models and climate-chemistry models forced with increasing greenhouse gases predict a strengthening of the Brewer-Dobson circulation (BDC) in the twenty-first century, and some of them claim that such strengthening has already begun at the end of the twentieth century. However, observational evidence for such a trend remains inconclusive. The goal of this paper is to examine the evidence for observed trends in the stratospheric overturning circulation using a suite of currently available observational stratospheric temperature data. Trends are examined as ''departures'' from the global mean temperature, since such trends reflect the effects of dynamics and spatially inhomogeneous radiative forcing and are to first order independent of the direct radiative effects of increasing well-mixed greenhouse gas concentrations. The primary conclusion of the study is that temperature observations do not reveal statistically significant trends in the Brewer-Dobson circulation over the period from 1979 to the present, as covered by Microwave Sounding Unit and Stratospheric Sounding Unit temperatures. The estimated trends in the BDC are weak in all datasets and not statistically significant at the 95% confidence level. In many cases, different data products yield very different results, particularly when the trends are stratified by season. Implications for the interpretation of recent stratospheric climate change are discussed. The results illustrate the essential need to better constrain the accuracy of future stratospheric temperature datasets.
dc.format.extent17 p.
dc.format.mimetypeapplication/pdf
dc.identifier.idgrec646717
dc.identifier.issn0894-8755
dc.identifier.urihttps://hdl.handle.net/2445/98870
dc.language.isoeng
dc.publisherAmerican Meteorological Society
dc.relation.isformatofReproducció del document publicat a: http://dx.doi.org/doi:10.1175/JCLI-D-14-00295.1
dc.relation.ispartofJournal of Climate, 2015, vol. 28, num. 8, p. 3024-3040
dc.relation.urihttp://dx.doi.org/doi:10.1175/JCLI-D-14-00295.1
dc.rights(c) American Meteorological Society, 2015
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física Aplicada)
dc.subject.classificationEstratosfera
dc.subject.classificationCirculació atmosfèrica
dc.subject.classificationTemperatura
dc.subject.classificationGasos d'efecte hivernacle
dc.subject.otherStratosphere
dc.subject.otherAtmospheric circulation
dc.subject.otherTemperature
dc.subject.otherGreenhouse gase
dc.titleHow robust are trends in the Brewer-Dobson circulation derived from observed stratospheric temperatures?
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion

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