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dc.contributor.authorNarukull, Venkateswara Rao
dc.contributor.authorEspy, Patrick Joseph
dc.contributor.authorHibbins, Robert
dc.contributor.authorFritts, David C.
dc.contributor.authorKavanagh, Andrew J.
dc.date.accessioned2018-02-09T14:20:04Z
dc.date.available2018-02-09T14:20:04Z
dc.date.created2016-01-18T10:54:43Z
dc.date.issued2015
dc.identifier.citationGeophysical Research Letters. 2015, 42 (19), 7853-7859.nb_NO
dc.identifier.issn0094-8276
dc.identifier.urihttp://hdl.handle.net/11250/2483793
dc.description.abstractModeling results have suggested that the circulation of the stratosphere and mesosphere in spring is strongly affected by the perturbations in heating induced by the Antarctic ozone hole. Here using both mesospheric MF radar wind observations from Rothera Antarctica (67°S, 68°W) as well as stratospheric analysis data, we present observational evidence that the stratospheric and mesospheric wind strengths are highly anti-correlated, and show their largest variability in November. We find that these changes are related to the total amount of ozone loss that occurs during the Antarctic spring ozone hole and particularly with the ozone gradients that develop between 57.5°S and 77.5°S. The results show that with increasing ozone loss during spring, winter conditions in the stratosphere and mesosphere persist longer into the summer. These results are discussed in the light of observations of the onset and duration of the Antarctic polar mesospheric cloud season.nb_NO
dc.language.isoengnb_NO
dc.publisherAmerican Geophysical Unionnb_NO
dc.titleObservational evidence of the influence of Antarctic stratospheric ozone variability on middle atmosphere dynamicsnb_NO
dc.typeJournal articlenb_NO
dc.typePeer reviewednb_NO
dc.description.versionpublishedVersionnb_NO
dc.source.pagenumber7853-7859nb_NO
dc.source.volume42nb_NO
dc.source.journalGeophysical Research Lettersnb_NO
dc.source.issue19nb_NO
dc.identifier.doi10.1002/2015GL065432
dc.identifier.cristin1315558
dc.relation.projectNorges forskningsråd: 223252nb_NO
dc.description.localcode©2015. American Geophysical Union. All Rights Reserved.nb_NO
cristin.unitcode194,66,20,0
cristin.unitnameInstitutt for fysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2


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