NLC and the background atmosphere above ALOMAR

dc.bibliographicCitation.firstPage5701eng
dc.bibliographicCitation.issue12eng
dc.bibliographicCitation.lastPage5717eng
dc.bibliographicCitation.volume11
dc.contributor.authorFiedler, J.
dc.contributor.authorBaumgarten, G.
dc.contributor.authorBerger, U.
dc.contributor.authorHoffmann, P.
dc.contributor.authorKaifler, N.
dc.contributor.authorLübken, F.-J.
dc.date.accessioned2018-03-09T10:43:59Z
dc.date.available2019-06-26T17:19:58Z
dc.date.issued2011
dc.description.abstractNoctilucent clouds (NLC) have been measured by the Rayleigh/Mie/Raman-lidar at the ALOMAR research facility in Northern Norway (69° N, 16° E). From 1997 to 2010 NLC were detected during more than 1850 h on 440 different days. Colocated MF-radar measurements and calculations with the Leibniz-Institute Middle Atmosphere (LIMA-) model are used to characterize the background atmosphere. Temperatures as well as horizontal winds at 83 km altitude show distinct differences during NLC observations compared to when NLC are absent. The seasonally averaged temperature is lower and the winds are stronger westward when NLC are detected. The wind separation is a robust feature as it shows up in measurements as well as in model results and it is consistent with the current understanding that lower temperatures support the existence of ice particles. For the whole 14-year data set there is no statistically significant relation between NLC occurrence and solar Lyman-α radiation. On the other hand NLC occurrence and temperatures at 83 km show a significant anti-correlation, which suggests that the thermal state plays a major role for the existence of ice particles and dominates the pure Lyman-α influence on water vapor during certain years. We find the seasonal mean NLC altitudes to be correlated to both Lyman-α radiation and temperature. NLC above ALOMAR are strongly influenced by atmospheric tides. The cloud water content varies by a factor of 2.8 over the diurnal cycle. Diurnal and semidiurnal amplitudes and phases show some pronounced year-to-year variations. In general, amplitudes as well as phases vary in a different manner. Amplitudes change by a factor of more than 3 and phases vary by up to 7 h. Such variability could impact long-term NLC observations which do not cover the full diurnal cycle.eng
dc.description.versionpublishedVersioneng
dc.formatapplication/pdf
dc.identifier.urihttps://doi.org/10.34657/1146
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/729
dc.language.isoengeng
dc.publisherMünchen : European Geopyhsical Unioneng
dc.relation.doihttps://doi.org/10.5194/acp-11-5701-2011
dc.relation.ispartofseriesAtmospheric Chemistry and Physics, Volume 11, Issue 12, Page 5701-5717eng
dc.rights.licenseCC BY 3.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/eng
dc.subjectcloud microphysicseng
dc.subjectdata seteng
dc.subjectdiurnal variationeng
dc.subjectMie theoryeng
dc.subjectpolar mesospheric cloudeng
dc.subjectradar imageryeng
dc.subject.ddc550eng
dc.titleNLC and the background atmosphere above ALOMAReng
dc.typearticleeng
dc.typeTexteng
dcterms.bibliographicCitation.journalTitleAtmospheric Chemistry and Physicseng
tib.accessRightsopenAccesseng
wgl.contributorIAPeng
wgl.subjectGeowissenschafteneng
wgl.subjectPhysikeng
wgl.typeZeitschriftenartikeleng
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