Abstract

During the SAMUM 2006 field campaign in southern Morocco, physical and chemical properties of desert aerosols were measured. Mass concentrations ranging from 30μgm−3 for PM2.5 under desert background conditions up to 300 000μgm−3 for total suspended particles (TSP) during moderate dust storms were measured. TSP dust concentrations are correlated with the local wind speed, whereasPM10 andPM2.5 concentrations are determined by advection from distant sources. Size distributions were measured for particles with diameter between 20 nm and 500μm (parametrizations are given). Two major regimes of the size spectrum can be distinguished. For particles smaller than 500 nm diameter, the distributions show maxima around 80 nm, widely unaffected of varying meteorological and dust emission conditions. For particles larger than 500 nm, the range of variation may be up to one order of magnitude and up to three orders of magnitude for particles larger than 10μm. The mineralogical composition of aerosol bulk samples was measured by X-ray powder diffraction. Major constituents of the aerosol are quartz, potassium feldspar, plagioclase, calcite, hematite and the clay minerals illite, kaolinite and chlorite. A small temporal variability of the bulk mineralogical composition was encountered. The chemical composition of approximately 74 000 particles was determined by electron microscopic single particle analysis. Three size regimes are identified: for smaller than 500 nm in diameter, the aerosol consists of sulphates and mineral dust. For larger than 500 nm up to 50μm, mineral dust dominates, consisting mainly of silicates, and—to a lesser extent—carbonates and quartz. For diameters larger than 50μm, approximately half of the particles consist of quartz. Time series of the elemental composition show a moderate temporal variability of the major compounds. Calcium-dominated particles are enhanced during advection from a prominent dust source in Northern Africa (Chott El Djerid and surroundings). The particle aspect ratio was measured for all analysed particles. Its size dependence reflects that of the chemical composition. For larger than 500 nm particle diameter, a median aspect ratio of 1.6 is measured. Towards smaller particles, it decreases to about 1.3 (parametrizations are given). From the chemical/mineralogical composition, the aerosol complex refractive index was determined for several wavelengths from ultraviolet to near-infrared. Both real and imaginary parts show lower values for particles smaller than 500 nm in diameter (1.55–2.8 × 10−3i at 530 nm) and slightly higher values for larger particles (1.57–3.7 × 10−3i at 530 nm).

Highlights

  • Long-range transport of mineral dust influences the climatic system directly and indirectly (e.g. Levin et al, 1996; Tegen et al, 1996; Haywood and Boucher, 2000), as well as atmospheric chemistry (e.g. Bauer et al, 2004; Matsuki et al, 2005; Rastogi and Sarin, 2006; Jeong and Sokolik, 2007; Sullivan et al.,B O U N DA RY L AY E R A E RO S O L AT TINFOU, M O RO C C O2007)

  • Mass concentrations ranging from 30 μg m−3 for PM2.5 under desert background conditions up to 300 000 μg m−3 for total suspended particles (TSP) during moderate dust storms were measured

  • The complex refractive index is calculated as a function of particle size and wavelength by applying a simple volume mixture rule to optical material properties taken from the literature (Ivlev and Popova, 1972; Philipp, 1985; Tropf, 1998; Sokolik and Toon, 1999) and laboratory measurements (Muller et al, 2008)

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Summary

Introduction

Long-range transport of mineral dust influences the climatic system directly and indirectly (e.g. Levin et al, 1996; Tegen et al, 1996; Haywood and Boucher, 2000), as well as atmospheric chemistry Mass concentrations and size distributions will be presented, as well as data of the size-resolved mineral and chemical composition of the dust in the boundary layer From this data set, optical parameters can be derived, which are important input parameters for any radiative transfer calculations to be carried out by other project partners of the SAMUM consortium. Dust physical and chemical parameters, like the size distribution, mineral phases, shape and complex refractive indices, for example, cannot be implemented from the existing literature, as these data are originating from different locations, seasons, meteorological and surface morphological conditions Such parameters vary strongly in space and time, they are non-uniform over the size and wavelength spectrum and depend on the local sources and transport from distant sources. A closure experiment was necessary to characterize the whole atmospheric column from the ground up to the top of the atmosphere

Location
Aircraft measurements
Mass concentrations
Size distributions
Mineral identification and quantification
Single particle chemistry and morphology
Composition
Conclusions and summary
Full Text
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