PM10 and black carbon (BC) mass concentrations and relative humidity (RH) are considered (Figure 1) to evaluate the relative influence of marine, dust and human emissions on the atmospheric abundance and chemical composition of aerosols at the sampling site. Although no large dust events were sampled, PM10 mass concentrations (Figure 1a) are essentially influenced by supermicrometer particles composed of mineral dust like in major African source areas of Aeolian soil dust (northeast desert in Niger or the Bodélé depression in Chad) [Rajot et al., 2008]. At our coastal site, marine particles may also be dominated by the coarse fraction of aerosols. The occurrence of marine air masses can be indicated by an increase of the relative humidity (Figure 1c), as observed for the samples collected during the period from 9 to 12 February 2006 associated with marine air masses (Figure 2). Finally, BC concentrations (Figure 1b) can give an indication on the abundance of carbonaceous particles or more precisely soot, the dominant light absorbing aerosol species. Vehicle fuels in western Africa are very polluting because of their poor quality and generate severe atmospheric pollution [van Vliet and Kinney, 2007]. BC hourly concentration profiles recorded at M'Bour are in accordance with traffic, with 3 maxima at about 0800, 1600 and 2000 UT that can get up to 4000 ng.m−3. Our measurements were performed each day between 1200 and 1300 UT, out of the high traffic periods, when BC concentrations are relatively low (Figure 1). Taken into account all these parameters (RH, PM10 and BC concentrations) and meteorological data, 6 events were selected from the dry season Special Observation Period (AMMA SOP-0), as representative of the atmospheric matter leaving the coastal Sahelian zone and transported over Atlantic Ocean during dry season, except during large dust events. The period from 9 to 12 February 2006 was avoided because it could be strongly influenced by local emissions from the densely populated West African coast and more particularly the city of M'Bour (Figure 2). The 6 selected events correspond to the highest PM10 concentrations for the two other periods, and variable RH and BC concentrations (Figure 1, marked events). The nighttime BC background ranged from about 150 ng m−3 for samples collected during the period 13–15 February, to about 700 ng m−3 for samples collected from 2 to 4 February. These background values are much higher than BC concentrations measured at remote sites [Bhugwant and Brémaud, 2001] and regional and/or continental anthropogenic emissions should be considered in the following discussion concerning these 6 events.
3.1. Mixing State of Aerosol
 An overview of mixing states of atmospheric particles obtained from SEM-EDX data is presented in Table 2. Externally mixed particles are defined here as particles containing only one chemical compound according to the identification criteria reported in Table 1. Aluminosilicate, silica, calcite, iron oxide, gypsum, titanium dioxide, carbonaceous, sodium chloride and sodium nitrate particles are identified as externally mixed particles (Table 3). However, they also often contain unexpected elements in a low fraction (less than 3 at. %, excluding carbon), like aluminum and silicon in the case of calcium carbonate particles. Moreover, they contain on average a significant fraction of carbon ranging from 6.3 to 11.3 at. %. Since volatile and semivolatile carbonaceous compounds are eliminated by the oxygen plasma cleaner of the microscope, the residual carbon content does not come from volatile organic carbon, but rather from higher molecular mass compounds, more resistant to oxidation reactions during the oxygen plasma cleaning, like graphite carbon, humic substances, heavy aliphatic or aromatic compounds. In fact, truly pure particles are quasi-nonexistent in the atmosphere. If stricter criteria were set for the particle identification, almost all atmospheric particles would be considered as unique mixtures of different compounds, practically impossible to interpret. Because of their volatilities, ammonium sulfate particles were not included in this discussion.
Table 2. Relative Abundances of Externally Mixed, Binary Internally Mixed, and Ternary Internally Mixed Particles for Six Selected Eventsa
|Particles||2 Feb||3 Feb||4 Feb||13 Feb||14 Feb||15 Feb|
|Externally mixed particles||82.1%||89.5%||75.7%||51.5%||83.5%||73.8%|
| (dust, carbonaceous and marine particles)||(1477)||(2017)||(1726)||(1002)||(1838)||(1617)|
|Binary internally mixed particles||17.2%||10.5%||24.3%||46.5%||16.1%||25.1%|
| (mixed carbonaceous/dust, mixed carbonaceous/marin, and mixed dust/marine particles)||(310)||(236)||(554)||(905)||(355)||(550)|
|Ternary internally mixed particles||0.7%||0.0%||0.0%||2.0%||0.4%||1.1%|
| (mixed carbonaceous/dust/marine particles)||(12)||(1)||(0)||(38)||(9)||(25)|
Table 3. Elemental Composition of Externally Mixed Particles
|Compound||Total Number of Particles||Particle Typea||Average Chemical Composition (in Atomic %)b|
|Aluminosilicate||4954||D||C(8.4) O(57.3) Mg(1.4) Al(11.3) Si(15.8) Fe(1.8)|
|Calcium carbonate||755||D||C(20.3) O(55.4) Na(1.1) Mg(1.1) Al(1.5) Si(2.1) Ca(16.0)|
|Carbonaceous||776||C||C(82.8) O(11.3) Si(1.0)|
|Gypsum||106||D||C(7.6) O(60.2) Na(1.7) Mg(1.2) Al(1.0) Si(1.4) S(12.8)Ca(12.1)|
|Iron oxide||75||D||C(7.6) O(61.0) Al(2.6) Si(2.6) Fe(22.0)|
|Mg Aluminosilicate||187||D||C(8.2) O(55.2) Mg(8.5) Al(6.5) Si(15.8) Fe(1.8)|
|Silica||636||D||C(6.3) O(58.0) Al(2.4) Si(30.4)|
|Sodium chloride||645||M||C(8.9) O(16.8) Na(38.4) Mg(1.9) Cl(29.5)|
|Sodium nitrate||366||M||C(6.7) N(12.1) O(51.8) Na(21.3) Mg(1.9) Al(1.2) Si(1.5)|
|Titanium oxide||58||D||C(11.3) O(57.4) Al(2.6) Si(3.0) Ti(21.4) Fe(1.3)|
 Dust, carbonaceous and marine compounds are mostly found externally mixed (Table 2), i.e., not present in the same particles. The particles containing internally mixed crustal compounds (e.g., iron enriched or calcium enriched aluminosilicates) are also assigned to the dust particle category. Dust, marine and carbonaceous particles account for respectively 78, 12 and 9% of externally mixed particles. The chemical composition of dust depends on the soil type in the source region. Considering the trajectories of sampled air masses (Figure 2), most of dust particles associated to the selected events probably come from northwestern Sahara. According to the literature, mineral dust transported from deserts of North Africa are rich in calcite and dolomite, whereas mineral dust emitted from Niger and Mauritania are rich in iron oxides [Formenti et al., 2003]. The presence of a significant fraction of calcite particles (Table 3; about 11% of dust particles) and a very low fraction of iron oxide particles (about 1% of dust particles) in our mineral dust samples with an origin in the northwestern Sahara corroborates this. C particles are relatively small particles compared to mineral dust: the mean equivalent diameter of C and dust particles analyzed by SEM-EDX are respectively 0.66 μm (1 SD = 0.66 μm) and 1.17 μm (1 SD = 1.11 μm). This is consistent with the formation of carbonaceous particles by gaseous phase condensation in the near field of incomplete combustion (primary particles) or during atmospheric transport (secondary organic particles), while mineral dust particles are generated in the atmosphere by mechanical wind erosion of soils [Seinfeld and Pandis, 1998]. Among marine particles, sodium chloride and sodium nitrate compounds account for about 12% of externally mixed particles, with mean equivalent diameters of 1.75 μm (1 SD = 1.51 μm) and 1.27 μm (1 SD = 0.81 μm), respectively. Supermicrometer particles are thus predominant in the marine particle group.
 Binary internally mixed particles can also account for a high proportion (from 10.5 to 46.5% of analyzed particles), whereas the relative abundances of ternary internally mixed particles are always very low, with a maximum of 2% of analyzed particles for the sample collected on 13 February 2006. Relative abundances of individual particles sorted into external (i.e., carbonaceous, dust, or marine) and binary internal mixture types (i.e., mixed carbonaceous/dust, mixed dust/marine, mixed carbonaceous/marine) are presented in Figure 3. Considering all events, the major internal binary mixtures are mixed carbonaceous/dust and dust/marine particles. Although carbonaceous particles have always the lowest mean diameters, the comparison of the mean diameters of mixed carbonaceous/dust particles with those of dust particles do not reveal a clear tendency. Sometimes they are lower than those of dust particles (as for 3, 4, and 15 February 2006), and in the others cases they are higher. On the same way, no systematic significant relation (Mann-Whitney test, p = 0.05) between the mean diameters of mixed dust/marine particles and those of dust or marine is observed.
Figure 3. Relative abundances of individual particles sorted into external (i.e., carbonaceous, dust, or marine) and binary internal mixture types (i.e., mixed carbonaceous/dust, mixed dust/marine, mixed carbonaceous/marine) for six selected events (see Figure 1). Ternary internally mixed carbonaceous/dust/marine particles are not considered here. The average diameter of particles is indicated for categories accounting for more than 100 particles.
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3.2. Scavenging of Marine Compounds by Dust
 Regarding the six selected events, particles containing marine compounds are relatively abundant when relative humidity is equal to, or higher than 20% (samples collected on 2 and 12–15 February 2006). For these four cases, the ratio of mixed marine (with dust or carbonaceous compounds) to “pure” marine particles ranges from 0.7 to 3.3. Marine compounds are thus often associated with other compounds to form mixed particles. The elemental mappings of mixed dust/marine particles, illustrated in Figure 4, indicate that aluminosilicate particles are often completely coated by marine compounds (principally NaNO3 in Figure 4). This coating was confirmed by Raman microspectrometry observations. These mixed particles, already observed in other studies [Ma et al., 2004; Sullivan et al., 2007], were probably formed by coagulation of dust and marine particles. The ambient relative humidity during sampling (Figure 1) is lower than the efflorescence relative humidity (ERH) of micrometer-sized NaCl particles (45 ± 3%), but sea-salt particles are probably liquid since ERH drastically decreases in the presence of organic compounds [Gao et al., 2008], as suspected for our marine particles that systematically contain some carbon (Table 3). Deliquescence can affect physical processes. Coagulation processes can easily take place between particles in a deliquescent state. Moreover, the homogeneous distribution of marine compounds at the surface of dust could be explained by cloud processes: at high relative humidity, mixed dust/marine particles could evolve into a solid core (the insoluble mineral dust particle) completely coated by a liquid salt layer. Consequently, when the relative humidity decreases under the crystallization point, solid sea salts are homogeneously distributed at the surface of particles. The back trajectories of sampled air masses were calculated using the HYSPLIT model with dumping RH data along them (not presented here). These calculations highlight that for the last studied period (13–15 February 2006), when dust particles are mostly mixed with sea salts (Figure 3), more than 60% of time trajectories are associated with RH higher than 70%. That corroborates the hypothesis of a homogenisation of the sea-salt distribution at the surface of dust particles by deliquescence of salts. The rate of aggregation of marine compounds on dust particles does not seem to be linked with the residence time of sea-salt particles in the atmosphere. Newly formed sea salts are mainly composed of genuine NaCl. They can react in polluted air masses with gaseous species such as H2SO4 or/and HNO3 to form partly or completely converted sea salts [Finlayson-Pitts and Pitts, 2000]. Completely converted sea salts are characterized by the absence of chloride, lost to the gas phase as HCl, and are typically composed of Na2SO4 or/and NaNO3. 98.7% of marine particles are partially or totally converted sea salts for the sample collected on 14 February 2006. These particles are not local sea-salt particles freshly emitted since they had time to be converted during their atmospheric transport. Such aged marine particles only represent 41.5, 54.4 and 63.8% of marine particles for samples collected on 13, 15 and 2 February, respectively. And yet, the relative abundances of mixed compared to pure marine particles are not significantly lower for these last 3 samples, evidencing the rapid aggregation of sea salts with dust. Other parameters like relative humidity and atmospheric turbulence have probably a key role on the mixing state of marine particles with dust. This scavenging of marine compounds by dust has a large impact on their optical properties. During the long-range transport of Saharan air masses over the Atlantic Ocean, the formation probability of mixed dust/marine particles is significant, as observed by Worobiec et al.  for soil dust particles collected in the Amazon Basin and coming from the Sahara. These hygroscopic mixed particles have a spectral absorption of solar radiation different than that of pure dust particles. The high capacity of marine particles to mix with dust has to be considered in the radiative budget calculation.
Figure 4. Scanning electron microscopy (SEM) image and elemental energy-dispersive X-ray (EDX) mappings (Al, Si, Na, Cl, and N) of individual internally mixed dust/marine particles (marked with white arrows). Scale marker bars correspond to 4 μm.
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3.3. Scavenging of Carbonaceous Compounds by Dust
 In western Africa, gaseous and particulate carbonaceous compounds (excluded carbon monoxide and dioxide) are predominantly of anthropogenic origin. Two major key sources can be distinguished: The widespread burning of agricultural biomass, notably during December–February, first constitutes a large source of carbonaceous pollutant in the North African continent [Johnson et al., 2008]. Second, urban emissions from growing African cities can largely contribute to atmospheric carbonaceous compounds inventory, because of vehicle fleets, high per vehicle emissions, limited road infrastructure and road congestion [van Vliet and Kinney, 2007]. This urban source also includes domestic charcoal and wood fires used for cooking. All these combustion sources generate both gaseous and particulate carbonaceous compounds that can interact by condensation or aggregation with mineral dust particles during atmospheric transport to form mixed carbonaceous/dust particles. For all the measured events, mixed carbonaceous/dust particles collected at M'Bour are relatively more abundant than pure carbonaceous particles (Figure 3). Even if the condensing material is not the same as the unmixed primary carbon material, the identification of these pure carbonaceous particles can give insights into the origin of carbonaceous compounds constituting internally mixed carbonaceous particles. More than 60% of analyzed pure carbonaceous particles (C particles) contain more than 90 at.% of carbon and are associated with a low oxygen content (1.7 at.% on average). This suggests freshly emitted C particles, not oxygenated by photochemical processes. For the others C particles (containing relatively high oxygen content), stochiometric calculations indicate that this oxygen is due to the presence of inorganic impurities like aluminum, silicon or sulphur that are in an oxidized form. Morphological parameters obtained by electron microscopy allow two major kinds of C particles to be distinguished: Soot with a fractal-like chain structure, and tar balls identified as separate spherules (Figure 5). The low intensity of the oxygen edge in EELS spectra of soot and tar balls (Figure 5) confirms the low oxygen content of carbonaceous compounds.
Figure 5. Transmission electron microscopy (TEM) image of (a) a spherical tar ball and (b) soot particles on a lacey carbon film with corresponding high-resolution TEM images and electron energy loss spectroscopy (EELS) spectra.
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 Soot accounts for an important fraction of the C particles. They are known to be a chemically complex mixture of amorphous carbonaceous compounds and graphitic elemental carbon [Buseck et al., 1987]. The crystallinity and the graphitic nature of soot depend upon the conditions of the combustion process in which they were formed [Roessler et al., 1981]. High-resolution TEM images of soot particles collected at M'Bour (Figure 5b) show no structural organization and no observation of nanocrystalline graphite with an onion shell structure as sometimes mentioned in the literature [Pósfai et al., 2003; Wentzel et al., 2003]. However, the 1 s σ* peak of the carbon edge on EELS spectra (Figure 5b) is systematically sharp and tall, indicating a high proportion of sp2 hybridized carbon, but the following fine structure of the shape is smoothed compared to the C-K edge of graphite spectra [Bernier et al., 2008; Gloter et al., 2003], so the structural ordering is not extended.
 The other major type of C particles is tar balls. They are exclusively observed in biomass burning and biofuel emissions and absorb light in the UV, visible and near-IR regions of the electromagnetic spectrum [Alexander et al., 2008; Hand et al., 2005; Pósfai et al., 2004]. They are spherical and amorphous C particles (Figure 5a) and typically not aggregated with other particles. The carbon edge of tar balls in EELS spectra is typical of amorphous carbon. Potassium containing particles, generally associated with C particles when they come from biomass burning and natural forest fires [Chou et al., 2008; Liu et al., 2000; Pósfai et al., 2003], were not significantly encountered in our samples. The biomass burning origin of these C particles is unquestionable but they could come from domestic wood fire rather than forest fire because of the absence of potassium containing particles [Echalar et al., 1995]. The low K concentrations obtained from bulk analysis (not presented here) in associated PM10 samples and the absence of long-range transport of air masses from equatorial Africa (Figure 2) where intensive forest fires generate biomass burning aerosols confirm this. In conclusion, C particles collected at M'Bour during the dry season (both soot and tar balls) are likely to have come from urban emissions, probably from Dakar and other neighboring densely populated areas. Carbonaceous compounds associated with mixed carbonaceous/dust particles probably come from the same urban areas.
 The formation of carbonaceous particles by combustion processes is accompanied by the emission of numerous volatile and semivolatile organic compounds and mixed dust/carbonaceous particles could be formed in the atmosphere by two different physical processes: on the one hand, carbonaceous compounds could condense on dust particles to form a carbonaceous layer. Indeed, volatile and semivolatile organic compounds can adsorb onto dust particles when a dust plume is mixed with polluted plumes containing emissions from human activities, forests or marine areas [Usher et al., 2003] and form a carbonaceous coating. On the other hand, carbonaceous particles (more probably tar balls or soot particles in our study) could coagulate with dust particles to form carbonaceous aggregates at the surface of dust particles. Organics were often found mixed with sulphates in atmospheric particles [Buseck and Pósfai, 1999; Ebert et al., 2004; Lee et al., 2002] and only few studies reported the presence of organic compounds on mineral dust particles [Falkovich et al., 2004; Hobert, 1995; Russell et al., 2002]. Leaitch et al.  notably observed carbonaceous compounds attached to coarse dust particles, suggesting a scavenging of organic compounds by Asian dust near anthropogenic sources. Arimoto et al.  observed that Asian dust collected below about 2 km altitude during ACE-Asia was commonly mixed with carbonaceous pollutants, to give a mixing with black carbon by aggregation. The presence of light-absorbing carbonaceous matter on mineral dust particles is important since it can strongly affect the light absorption spectrum, hence the radiative impact of dust [Kirchstetter et al., 2004]. The sp2-hybridation in graphitic carbon contained in soot or black carbon is related to photoabsorption and index of refraction [Bond and Bergstrom, 2006]. The aggregation of soot particles with mineral dust will increase the light absorption of these dust particles and the magnitude of their contribution to radiative forcing. But other carbonaceous compounds, also called “brown carbon,” can also significantly contribute to light absorption with strong wavelength dependence, even if they constitute weak-absorbing compounds [Andreae and Gelencser, 2006]. As illustrated for a typical mixed carbonaceous/dust particle collected at M'Bour (Figure 6), the elemental EDX mappings seem to indicate that carbon is homogeneously distributed over the surface of particles. Although the lacey carbon film reduces the sharpness of the C maps, the perimeter of the mixed carbonaceous/dust particles is always very similar to that on the Al or Si maps. A typical Raman spectrum of a mineral dust particle identified as internally mixed with carbonaceous compounds from previous SEM-EDX analysis is presented in Figure 7. Curve fitting of the first-order spectral region characteristic of carbonaceous species (800–2000 cm−1) was carried out using five band fits (denoted G, D1, D2, D3, and D4). The D1 band full width at half maximum (FWHM) enables a clear distinction of carbonaceous materials with variable degree of structural order [Ivleva et al., 2007]. Figure 8 reports experimental values of D1 band FWHM for five reference samples (i.e., highly oriented pyrolytic graphite, graphite flakes, activated carbon, urban soot and SRM 1650b diesel soot) and nine individual mineral dust particles in the size range 1.5–2.8 μm, identified as internally mixed with carbonaceous compounds from previous SEM-EDX analysis. The average value of the D1 band FWHM for African dust particles was found at 195 cm−1, close to the values obtained for urban soot and diesel soot reference samples, found at 173 and 175 cm−1, respectively. Such high D1 band FWHM indicates a low degree of graphitization (prevalence of amorphous domains). The absence of fractal shape for these mixed carbonaceous/dust particles evidenced by TEM observations and a smooth shape of the broad carbon edge in their EELS spectra, typical from amorphous carbon, exclude an aggregation of dust with soot particles. Therefore, the high D1 band FWHM in Raman spectra is consistent with the formation of an amorphous coating by adsorption of carbonaceous compounds on mineral dust particles during their atmospheric transport. These carbonaceous compounds could be constituted from carboxylic acids as already observed in other studies [Sullivan and Prather, 2007; Takahama et al., 2010].
Figure 6. SEM image and elemental EDX mappings (Al, Si, and C) of a mixed carbonaceous/dust particle on lacey carbon film.
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Figure 7. Typical Raman spectrum of a mineral dust particle internally mixed with carbonaceous compounds. The mineral particle is composed of dolomite, identified at 209 and 1097 cm−1, and Na-feldspar, identified at 290, 478, and 509 cm−1. Curve fitting of the first-order spectral region characteristic of carbonaceous species (800–1800 cm−1) was carried out with five band fits (G, D1, D2, D3, D4).
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Figure 8. Full widths at half maximum (FWHM) of the D1 band for five reference samples and nine individual African dust particles (mean values ± standard deviations) identified as internally mixed with carbonaceous compounds from previous SEM-EDX analysis. HOPG stands for highly oriented pyrolytic graphite. The dashed line corresponds to the average value of D1 band FWHM for the African dust particles.
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 In conclusion, mixed dust/carbonaceous particles observed at M'Bour are probably the result of adsorption on dust particles of organic compounds from local anthropogenic emissions. These emissions can come from domestic wood fire or urban activities as suspected for pure carbonaceous particles. Moreover, volatile carbon and/or inorganic materials like sulphate were also probably present at the surface of atmospheric particles but were lost in the analytical process. As a light-absorbing component of aerosols, the carbonaceous coating probably plays an important role in the radiative properties of the atmosphere. Moreover, such carbonaceous coating (as volatile compounds probably associated with it) can affect the cloud condensation nuclei (CCN) behavior of the core dust, considering the higher hygroscopicity of carbonaceous compounds in the outer layer relative to that of mineral dust [Takahama et al., 2010].