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dc.contributor.advisorEspy, Patrick Joseph
dc.contributor.authorFritsch, Frauke Ruth Lotte
dc.date.accessioned2016-06-22T14:00:27Z
dc.date.available2016-06-22T14:00:27Z
dc.date.created2016-05-15
dc.date.issued2016
dc.identifierntnudaim:12579
dc.identifier.urihttp://hdl.handle.net/11250/2393719
dc.description.abstractThis thesis investigated the influence and conditions of vertical propagation of planetary waves on the mid-winter cooling in the southern hemispheric polar meso- sphere. MERRA zonal wind data was used to extract planetary waves with zonal wavenumber 1, 2 and 3 at 72°S in 2008 and 2009. The wave periods of 4, 5, 10 and 16 days were separated using Morlet wavelet analysis. A correlation between the wave amplitude and carbon monoxide as a tracer for vertical motion could be found from autumn until late winter (from March until late August/mid September). Between the wave amplitude and the mean zonal wind anticorrelation was shown from early winter until late winter (April until late Au- gust/mid September). Both correlations were found to stop when the mesospheric circulation restores in September. In addition agreement between calculations for the upper bound of the Charney-Drazin criterion for vertical propagation and the wave activity was found until late August/mid September.
dc.languageeng
dc.publisherNTNU
dc.subjectPhysics (MSPHYS)
dc.titleWhat causes the mid-winter cooling?
dc.typeMaster thesis
dc.source.pagenumber55


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