Vertical profiling of convective dust plumes in southern Morocco during SAMUM

dc.bibliographicCitation.firstPage340
dc.bibliographicCitation.issue1eng
dc.bibliographicCitation.lastPage353
dc.bibliographicCitation.volume61
dc.contributor.authorAnsmann, Albert
dc.contributor.authorTesche, Matthias
dc.contributor.authorKnippertz, Peter
dc.contributor.authorBierwirth, Eike
dc.contributor.authorAlthausen, Dietrich
dc.contributor.authorMüller, Detlef
dc.contributor.authorSchulz, Oliver
dc.date.accessioned2018-02-06T16:38:27Z
dc.date.available2019-06-26T17:17:10Z
dc.date.issued2017
dc.description.abstractLifting of dust particles by dust devils and convective plumes may significantly contribute to the global mineral dust budget. During the Saharan Mineral Dust Experiment (SAMUM) in May–June 2006 vertical profiling of dusty plumes was performed for the first time. Polarization lidar observations taken at Ouarzazate (30.9◦N, 6.9◦W, 1133 m height above sea level) are analyzed. Two cases with typical and vigorous formation of convective plumes and statistical results of 5 d are discussed. The majority of observed convective plumes have diameters on order of 100–400 m. Most of the plumes (typically 50–95%) show top heights <1 km or 0.3DLH with the Saharan dust layer height DLH of typically 3–4 km. Height-to-diameter ratio is mostly 2–10. Maximum plume top height ranges from 1.1 to 2.9 km on the 5 d. 5–26 isolated plumes and clusters of plumes per hour were detected. A low dust optical depth (<0.3) favours plume evolution. Observed surface, 1 and 2–m air temperatures indicate that a difference of 17–20 K between surface and 2-m air temperature and of 0.9–1 K between the 1 and 2-m temperatures are required before convective plumes develop. Favourable horizontal wind speeds are 2–7 ms−1.eng
dc.description.versionpublishedVersioneng
dc.formatapplication/pdf
dc.identifier.urihttps://doi.org/10.34657/1390
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/312
dc.language.isoengeng
dc.publisherMilton Park : Taylor & Franciseng
dc.relation.doihttps://doi.org/10.1111/j.1600-0889.2008.00384.x
dc.relation.ispartofseriesTellus B: Chemical and Physical Meteorology, Volume 61, Issue 1, Page 340-353eng
dc.rights.licenseCC BY 4.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/eng
dc.subjectaerosoleng
dc.subjectatmospheric convectioneng
dc.subjectdust devileng
dc.subjectobservational methodeng
dc.subjectoptical deptheng
dc.subjectparticle sizeeng
dc.subjectsize distributioneng
dc.subjecttop of atmosphereeng
dc.subjectvertical profileeng
dc.subjectwind velocityeng
dc.subject.ddc550eng
dc.titleVertical profiling of convective dust plumes in southern Morocco during SAMUMeng
dc.typearticleeng
dc.typeTexteng
dcterms.bibliographicCitation.journalTitleTellus B: Chemical and Physical Meteorologyeng
tib.accessRightsopenAccesseng
wgl.contributorTROPOSeng
wgl.subjectGeowissenschafteneng
wgl.typeZeitschriftenartikeleng
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