Local stratopause temperature variabilities and their embedding in the global context

dc.bibliographicCitation.firstPage373eng
dc.bibliographicCitation.issue2eng
dc.bibliographicCitation.journalTitleAnnales Geophysicaeeng
dc.bibliographicCitation.lastPage383eng
dc.bibliographicCitation.volume38eng
dc.contributor.authorEixmann, Ronald
dc.contributor.authorMatthias, Vivien
dc.contributor.authorHöffner, Josef
dc.contributor.authorBaumgarten, Gerd
dc.contributor.authorGerding, Michael
dc.date.accessioned2021-07-09T08:09:52Z
dc.date.available2021-07-09T08:09:52Z
dc.date.issued2020
dc.description.abstractThe stratopause is by definition the transition between the stratosphere and mesosphere. During winter the circulation at mid-latitudes and high latitudes in the stratosphere is mainly driven by quasi-stationary planetary waves (PWs), while the circulation in the mesosphere is mainly driven by gravity waves (GWs). The question arises of whether PWs or GWs dominate the variability of the stratopause. The most famous and dramatic variability of the middle atmosphere is a sudden stratospheric warming (SSW) generated by PWs interacting with the polar vortex. A similar phenomenon but smaller in magnitude and more regional is stratopause temperature enhancements (STEs) initially observed by local measurements and generated by breaking PWs. Thus it seems that PWs dominate the variability of the stratopause. In this study we want to quantify to which extent quasi-stationary PWs contribute to the stratopause variability. To do that we combine local lidar observations at Kühlungsborn (54∘ N, 11∘ E) and Andenes (69∘ N, 16∘ E) with global MERRA-2 reanalysis data bringing the local variability of the stratopause into the global context. Therefore we compare the temperature time series at Kühlungsborn and Andenes at 2 hPa, the altitude where STEs maximize, with characteristics (amplitude and phase) of PWs with wave numbers 1, 2 and 3. We found that for Kühlungsborn and Andenes 98 % of the local day-to-day variability of the stratopause can be explained by the variability of PWs with wave number 1, 2 and 3. Thus, the winter stratopause day-to-day variability is highly dominated by the variability of PWs.eng
dc.description.fondsLeibniz_Fonds
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/6231
dc.identifier.urihttps://doi.org/10.34657/5278
dc.language.isoengeng
dc.publisherGöttingen : Copernicus Publ.eng
dc.relation.doihttps://doi.org/10.5194/angeo-38-373-2020
dc.relation.essn1432-0576
dc.relation.issn0992-7689
dc.rights.licenseCC BY 4.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/eng
dc.subject.ddc550eng
dc.subject.otherstratopauseeng
dc.subject.othergravity waves (GWs)eng
dc.subject.otherplanetary waves (PWs)eng
dc.titleLocal stratopause temperature variabilities and their embedding in the global contexteng
dc.typeArticleeng
dc.typeTexteng
tib.accessRightsopenAccesseng
wgl.contributorIAPeng
wgl.subjectGeowissenschafteneng
wgl.typeZeitschriftenartikeleng
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