Vertical profiling of Saharan dust with Raman lidars and airborne HSRL in southern Morocco during SAMUM

dc.bibliographicCitation.firstPage144
dc.bibliographicCitation.issue1eng
dc.bibliographicCitation.lastPage164
dc.bibliographicCitation.volume61
dc.contributor.authorTesche, Matthias
dc.contributor.authorAnsmann, Albert
dc.contributor.authorMüLLER, Detlef
dc.contributor.authorAlthausen, Dietrich
dc.contributor.authorMattis, Ina
dc.contributor.authorHeese, Birgit
dc.contributor.authorFreudenthaler, Volker
dc.contributor.authorWiegner, Matthias
dc.contributor.authorEsselborn, Michael
dc.contributor.authorPisani, Gianluca
dc.contributor.authorKnippertz, Peter
dc.date.accessioned2018-02-07T04:38:29Z
dc.date.available2019-06-26T17:17:17Z
dc.date.issued2017
dc.description.abstractThree ground-based Raman lidars and an airborne high-spectral-resolution lidar (HSRL) were operated duringSAMUM 2006 in southern Morocco to measure height profiles of the volume extinction coefficient, the extinction-to-backscatter ratio and the depolarization ratio of dust particles in the Saharan dust layer at several wavelengths. Aerosol Robotic Network (AERONET) Sun photometer observations and radiosoundings of meteorological parameters complemented the ground-based activities at the SAMUM station of Ouarzazate. Four case studies are presented. Two case studies deal with the comparison of observations of the three ground-based lidars during a heavy dust outbreak and of the ground-based lidars with the airborne lidar. Two further cases show profile observations during satellite overpasses on 19 May and 4 June 2006. The height resolved statistical analysis reveals that the dust layer top typically reaches 4–6 km height above sea level (a.s.l.), sometimes even 7 km a.s.l.. Usually, a vertically inhomogeneous dust plume with internal dust layers was observed in the morning before the evolution of the boundary layer started. The Saharan dust layer was well mixed in the early evening. The 500 nm dust optical depth ranged from 0.2–0.8 at the field site south of the High Atlas mountains, Ångström exponents derived from photometer and lidar data were between 0–0.4. The volume extinction coefficients (355, 532 nm) varied from 30–300Mm−1 with a mean value of 100Mm−1 in the lowest 4 km a.s.l.. On average, extinction-to-backscatter ratios of 53–55 sr (±7–13 sr) were obtained at 355, 532 and 1064 nm.eng
dc.description.versionpublishedVersioneng
dc.formatapplication/pdf
dc.identifier.urihttps://doi.org/10.34657/1389
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/350
dc.language.isoengeng
dc.publisherMilton Park : Taylor & Franciseng
dc.relation.doihttps://doi.org/10.1111/j.1600-0889.2008.00390.x
dc.relation.ispartofseriesTellus B: Chemical and Physical Meteorology, Volume 61, Issue 1, Page 144-164eng
dc.rights.licenseCC BY 4.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/eng
dc.subjectaerosoleng
dc.subjectairborne surveyeng
dc.subjectbackscattereng
dc.subjectdusteng
dc.subjectground-based measurementeng
dc.subjectlidareng
dc.subjectobservational methodeng
dc.subjectoptical deptheng
dc.subjectparticle sizeeng
dc.subjectphotometereng
dc.subjectsize distributioneng
dc.subjectspectral analysiseng
dc.subjectvertical profileeng
dc.subjectwavelengtheng
dc.subject.ddc550eng
dc.titleVertical profiling of Saharan dust with Raman lidars and airborne HSRL 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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