Five-day planetary waves in the middle atmosphere from Odin satellite data and ground-based instruments in Northern Hemisphere summer 2003, 2004, 2005 and 2007

dc.bibliographicCitation.firstPage3557
dc.bibliographicCitation.issue11eng
dc.bibliographicCitation.journalTitleAnnales Geophysicaeeng
dc.bibliographicCitation.lastPage3570
dc.bibliographicCitation.volume26
dc.contributor.authorBelova, A.
dc.contributor.authorKirkwood, S.
dc.contributor.authorMurtagh, D.
dc.contributor.authorMitchell, N.
dc.contributor.authorSinger, W.
dc.contributor.authorHocking, W.
dc.date.accessioned2018-02-24T10:07:51Z
dc.date.available2019-06-28T12:38:28Z
dc.date.issued2008
dc.description.abstractA number of studies have shown that 5-day planetary waves modulate noctilucent clouds and the closely related Polar Mesosphere Summer Echoes (PMSE) at the summer mesopause. Summer stratospheric winds should inhibit wave propagation through the stratosphere and, although some numerical models (Geisler and Dickinson, 1976) do show a possibility for upward wave propagation, it has also been suggested that the upward propagation may in practice be confined to the winter hemisphere with horizontal propagation of the wave from the winter to the summer hemisphere at mesosphere heights causing the effects observed at the summer mesopause. It has further been proposed (Garcia et al., 2005) that 5-day planetary waves observed in the summer mesosphere could be excited in-situ by baroclinic instability in the upper mesosphere. In this study, we first extract and analyze 5-day planetary wave characteristics on a global scale in the middle atmosphere (up to 54 km in temperature, and up to 68 km in ozone concentration) using measurements by the Odin satellite for selected days during northern hemisphere summer from 2003, 2004, 2005 and 2007. Second, we show that 5-day temperature fluctuations consistent with westward-traveling 5-day waves are present at the summer mesopause, using local ground-based meteor-radar observations. Finally we examine whether any of three possible sources of the detected temperature fluctuations at the summer mesopause can be excluded: upward propagation from the stratosphere in the summer-hemisphere, horizontal propagation from the winter-hemisphere or in-situ excitation as a result of the baroclinic instability. We find that in one case, far from solstice, the baroclinic instability is unlikely to be involved. In one further case, close to solstice, upward propagation in the same hemisphere seems to be ruled out. In all other cases, all or any of the three proposed mechanisms are consistent with the observations.eng
dc.description.versionpublishedVersioneng
dc.formatapplication/pdf
dc.identifier.urihttps://doi.org/10.34657/1527
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/4047
dc.language.isoengeng
dc.publisherMünchen : European Geopyhsical Unioneng
dc.relation.doihttps://doi.org/10.5194/angeo-26-3557-2008
dc.rights.licenseCC BY 3.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/eng
dc.subject.ddc530eng
dc.subject.otherbaroclinic modeeng
dc.subject.otherground-based measurementeng
dc.subject.othermesopauseeng
dc.subject.otherNorthern Hemisphereeng
dc.subject.othernumerical modeleng
dc.subject.otherplanetary waveeng
dc.subject.otherpolar mesosphere summer echoeng
dc.subject.otherpolar mesospheric cloudeng
dc.subject.othersatellite dataeng
dc.subject.otherstratosphereeng
dc.subject.othertemperature gradienteng
dc.subject.otherwave propagationeng
dc.titleFive-day planetary waves in the middle atmosphere from Odin satellite data and ground-based instruments in Northern Hemisphere summer 2003, 2004, 2005 and 2007eng
dc.typeArticleeng
dc.typeTexteng
tib.accessRightsopenAccesseng
wgl.contributorIAPeng
wgl.subjectPhysikeng
wgl.subjectGeowissenschafteneng
wgl.typeZeitschriftenartikeleng
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