Optical properties of aerosol mixtures derived from sun-sky radiometry during SAMUM-2

dc.bibliographicCitation.firstPage635
dc.bibliographicCitation.issue4eng
dc.bibliographicCitation.lastPage648
dc.bibliographicCitation.volume63
dc.contributor.authorToledano, C.
dc.contributor.authorWiegner, M.
dc.contributor.authorGroß, S.
dc.contributor.authorFreudenthaler, V.
dc.contributor.authorGasteiger, J.
dc.contributor.authorMüller, D.
dc.contributor.authorMüller, T.
dc.contributor.authorSchladitz, A.
dc.contributor.authorWeinzierl, B.
dc.contributor.authorTorres, B.
dc.contributor.authorO’neill, N.T.
dc.date.accessioned2018-02-05T16:37:43Z
dc.date.available2019-06-26T17:17:08Z
dc.date.issued2017
dc.description.abstractThe SAMUM-2 experiment took place in the Cape Verde is lands in January–February 2008. The colocated ground-based and airborne instruments allow the study of desert dust optical and microphysical properties in a closure experiment. The Meteorological Institute of the University of Munich deployed one sun-sky photometer and two tropospheric lidar systems. A travelling AERONET-Cimel sun-sky radiometer was also deployed. During the measurement period the aerosol scenario over Cape Verde mostly consisted of a dust layer below 2 km and a smoke-dust layer above 2–4 km a.s.l. The Saharan dust arrived at the site from the NE, whereas the smoke originated in the African equatorial region. This paper describes the main results of the Sun photometer observations, supported by lidar information. An analysis of the variations in the aerosol optical depth (AOD) in the range 340–1550 nm, the Ångström exponent, volume size distributions and single scattering albedo is presented. The aerosol mixtures are analysed by means of the fine mode fraction of the AOD provided by the sun-sky inversion data and the Spectral Deconvolution Algorithm. The mean AOD (500 nm) was 0.31, with associated low ångström exponent of 0.46. Several types of events were detected within the data set, with prevalence of dust or mixtures as characterized by the Ångstr¨om exponents of extinction and absorption and the fine mode fraction. Aerosol properties derived from sunphotometry were compared to in situ measurements of size distribution, effective radius and single scattering albedo.eng
dc.description.versionpublishedVersioneng
dc.formatapplication/pdf
dc.identifier.urihttps://doi.org/10.34657/1156
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/300
dc.language.isoengeng
dc.publisherMilton Park : Taylor & Franciseng
dc.relation.doihttps://doi.org/10.1111/j.1600-0889.2011.00573.x
dc.relation.ispartofseriesTellus B: Chemical and Physical Meteorology, Volume 63, Issue 4, Page 635-648eng
dc.rights.licenseCC BY 4.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/eng
dc.subjectaerosol propertyeng
dc.subjectatmospheric modelingeng
dc.subjectatmospheric transporteng
dc.subjectbiomass burningeng
dc.subjectdusteng
dc.subjectground-based measurementeng
dc.subjectobservational methodeng
dc.subjectremote sensingeng
dc.subjectsmokeeng
dc.subjecttemporal evolutioneng
dc.subject.ddc550eng
dc.titleOptical properties of aerosol mixtures derived from sun-sky radiometry during SAMUM-2eng
dc.typearticleeng
dc.typeTexteng
dcterms.bibliographicCitation.journalTitleTellus B: Chemical and Physical Meteorologyeng
tib.accessRightsopenAccesseng
wgl.contributorTROPOSeng
wgl.subjectGeowissenschafteneng
wgl.typeZeitschriftenartikeleng
Files
Original bundle
Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
j_1600_0889_2011_00573.pdf
Size:
2.06 MB
Format:
Adobe Portable Document Format
Description: