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dc.contributor.advisorEspy, Patrick Josephnb_NO
dc.contributor.authorOsnes, Christine Birgittenb_NO
dc.date.accessioned2014-12-19T13:16:59Z
dc.date.available2014-12-19T13:16:59Z
dc.date.created2011-09-15nb_NO
dc.date.issued2011nb_NO
dc.identifier441347nb_NO
dc.identifierntnudaim:6687nb_NO
dc.identifier.urihttp://hdl.handle.net/11250/246509
dc.description.abstractOzone and temperature data from Troll and Rothera research stations has been analyzed in order to trace planetary waves. Seasonal variations were removed and spectral analysis was performed in order to find dominating frequencies. Possible planetary wave oscillations were found in the 4, 5, 8.5, 10-11, 11-13, 14-15, 17-20, 21-24 and 26-45 day bands, some corresponding to the atmospheric normal modes. These were found consistently in both the ozone and temperature data, indicating that the millimeter wave spectroscopy used to measure the ozone is a viable technique for tracing planetary waves in a region of the atmosphere where other measurements are sparse.nb_NO
dc.languageengnb_NO
dc.publisherInstitutt for fysikknb_NO
dc.subjectntnudaim:6687no_NO
dc.subjectMTFYMA fysikk og matematikkno_NO
dc.subjectTeknisk fysikkno_NO
dc.titlePlanetary Wave Oscillations observed in Ozone and Temperature Data from Antarctica during 2009nb_NO
dc.typeMaster thesisnb_NO
dc.source.pagenumber78nb_NO
dc.contributor.departmentNorges teknisk-naturvitenskapelige universitet, Fakultet for naturvitenskap og teknologi, Institutt for fysikknb_NO


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