GSTDTAP  > 地球科学
DOI10.5194/acp-18-13429-2018
Composition and mixing state of atmospheric aerosols determined by electron microscopy: method development and application to aged Saharan dust deposition in the Caribbean boundary layer
Kandler, Konrad1; Schneiders, Kilian1; Ebert, Martin1; Hartmann, Markus1,3; Weinbruch, Stephan1; Prass, Maria2; Poehlker, Christopher2
2018-09-21
发表期刊ATMOSPHERIC CHEMISTRY AND PHYSICS
ISSN1680-7316
EISSN1680-7324
出版年2018
卷号18期号:18页码:13429-13455
文章类型Article
语种英语
国家Germany
英文摘要

The microphysical properties, composition and mixing state of mineral dust, sea salt and secondary compounds were measured by active and passive aerosol sampling, followed by electron microscopy and X-ray fluorescence in the Caribbean marine boundary layer. Measurements were carried out at Ragged Point, Barbados during June-July 2013 and August 2016. Techniques are presented and evaluated, which allow for statements on atmospheric aerosol concentrations and aerosol mixing state based on collected samples. It became obvious that in the diameter range with the highest dust deposition the deposition velocity models disagree by more than 2 orders of magnitude. Aerosol at Ragged Point was dominated by dust, sea salt and soluble sulfates in varying proportions. The contribution of sea salt was dependent on local wind speed. Sulfate concentrations were linked to long-range transport from Africa and Europe, and South America and the southern Atlantic Ocean. Dust sources were located in western Africa. The dust silicate composition was not significantly varied. Pure feldspar grains were 3 % of the silicate particles, of which about a third were K-feldspar. The average dust deposition observed was 10 mg m(-2) d(-1) (range of 0.5-47 mg m(-2) d(-1) ), of which 0.67 mg m(-2) d(-1) was iron and 0.001 mg m(-2) d(-1) phosphorus. Iron deposition was mainly driven by silicate particles from Africa. Dust particles were mixed internally to a minor fraction (10 %), mostly with sea salt and less frequently with sulfate. It was estimated that the average dust deposition velocity under ambient conditions is increased by the internal mixture by 30 %-140 % for particles between 1 and 10 mu m dust aerodynamic diameter, with approximately 35 % at the mass median diameter of deposition (7.0 mu m). For this size, an effective deposition velocity of 6 4 mm s(-1) (geometric standard deviation of 3.1 over all individual particles) was observed.


领域地球科学
收录类别SCI-E
WOS记录号WOS:000445271300002
WOS关键词LONG-RANGE TRANSPORT ; COARSE PARTICULATE MATTER ; COMPLEX REFRACTIVE-INDEX ; MINERAL-DUST ; SEA-SALT ; CLOUD CONDENSATION ; ICE NUCLEATION ; NORTH-ATLANTIC ; AFRICAN DUST ; ASPIRATION EFFICIENCY
WOS类目Environmental Sciences ; Meteorology & Atmospheric Sciences
WOS研究方向Environmental Sciences & Ecology ; Meteorology & Atmospheric Sciences
引用统计
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/29524
专题地球科学
作者单位1.Tech Univ Darmstadt, Inst Appl Geosci, D-64287 Darmstadt, Germany;
2.Max Planck Inst Chem, Multiphase Chem Dept, D-55128 Mainz, Germany;
3.Tropos Leibniz Inst Tropospher Res TROPOS, Expt Aerosol & Cloud Microphys Dept, D-04318 Leipzig, Germany
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GB/T 7714
Kandler, Konrad,Schneiders, Kilian,Ebert, Martin,et al. Composition and mixing state of atmospheric aerosols determined by electron microscopy: method development and application to aged Saharan dust deposition in the Caribbean boundary layer[J]. ATMOSPHERIC CHEMISTRY AND PHYSICS,2018,18(18):13429-13455.
APA Kandler, Konrad.,Schneiders, Kilian.,Ebert, Martin.,Hartmann, Markus.,Weinbruch, Stephan.,...&Poehlker, Christopher.(2018).Composition and mixing state of atmospheric aerosols determined by electron microscopy: method development and application to aged Saharan dust deposition in the Caribbean boundary layer.ATMOSPHERIC CHEMISTRY AND PHYSICS,18(18),13429-13455.
MLA Kandler, Konrad,et al."Composition and mixing state of atmospheric aerosols determined by electron microscopy: method development and application to aged Saharan dust deposition in the Caribbean boundary layer".ATMOSPHERIC CHEMISTRY AND PHYSICS 18.18(2018):13429-13455.
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