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dc.contributor.authorWeare, B. C.
dc.contributor.authorMonier, Erwan
dc.date.accessioned2015-05-04T12:37:43Z
dc.date.available2015-05-04T12:37:43Z
dc.date.issued2011-12
dc.date.submitted2011-11
dc.identifier.issn1680-7324
dc.identifier.issn1680-7316
dc.identifier.urihttp://hdl.handle.net/1721.1/96881
dc.description.abstractThe momentum budget of the Transformed Eulerian-Mean (TEM) equation is calculated using the European Centre for Medium-Range Weather Forecasts (ECMWF) reanalysis (ERA-40) and the National Centers for Environmental Prediction (NCEP) Reanalysis 2 (R-2). This study outlines the considerable contribution of unresolved waves, deduced to be gravity waves, to the forcing of the zonal-mean flow. A trend analysis, from 1980 to 2001, shows that the onset and break down of the Northern Hemisphere (NH) stratospheric polar night jet has a tendency to occur later in the season in the more recent years. This temporal shift follows long-term changes in planetary wave activity that are mainly due to synoptic waves, with a lag of one month. In the Southern Hemisphere (SH), the polar vortex shows a tendency to persist further into the SH summertime. This also follows a statistically significant decrease in the intensity of the stationary EP flux divergence over the 1980–2001 period. Ozone depletion is well known for strengthening the polar vortex through the thermal wind balance. However, the results of this work show that the SH polar vortex does not experience any significant long-term changes until the month of December, even though the intensification of the ozone hole occurs mainly between September and November. This study suggests that the decrease in planetary wave activity in November provides an important feedback to the zonal wind as it delays the breakdown of the polar vortex. In addition, the absence of strong eddy feedback before November explains the lack of significant trends in the polar vortex in the SH early spring. A long-term weakening in the Brewer-Dobson (B-D) circulation in the polar region is identified in the NH winter and early spring and during the SH late spring and is likely driven by the decrease in planetary wave activity previously mentioned. During the rest of the year, there are large discrepancies in the representation of the B-D circulation and the unresolved waves between the two reanalyses, making trend analyses unreliable.en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant ATM0733698)en_US
dc.language.isoen_US
dc.publisherCopernicus GmbHen_US
dc.relation.isversionofhttp://dx.doi.org/10.5194/acp-11-12751-2011en_US
dc.rightsCreative Commons Attributionen_US
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/en_US
dc.sourceMonieren_US
dc.titleClimatology and trends in the forcing of the stratospheric zonal-mean flowen_US
dc.typeArticleen_US
dc.identifier.citationMonier, E., and B. C. Weare. “Climatology and Trends in the Forcing of the Stratospheric Zonal-Mean Flow.” Atmospheric Chemistry and Physics 11, no. 24 (2011): 12751–12771.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Center for Global Change Scienceen_US
dc.contributor.departmentMassachusetts Institute of Technology. Joint Program on the Science & Policy of Global Changeen_US
dc.contributor.approverMonier, Erwanen_US
dc.contributor.mitauthorMonier, Erwanen_US
dc.relation.journalAtmospheric Chemistry and Physicsen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsMonier, E.; Weare, B. C.en_US
dc.identifier.orcidhttps://orcid.org/0000-0001-5533-6570
mit.licensePUBLISHER_CCen_US
mit.metadata.statusComplete


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