Effect of local and long-range transport emissions on the elemental composition of PM10–2.5 and PM2.5 in Beirut
Introduction
The Mediterranean basin is considered one of the most controversial regions for aerosol transportation due to its location at the intersection of air masses circulating among the three continents (Lelieveld et al., 2002). It is situated just North of the Saharan Desert of Africa, and South of the heavily populated and highly industrialized European continent. Other studies conducted in the North-Western (Spain, France, Italy) (Bergametti et al., 1989; Chester et al., 1999; Dulac et al., 1987; Migon et al., 1991; Querol et al., 2001; Sandroni and Migon, 1997) and eastern (Greece, Turkey, Israel) Mediterranean regions (Chabas and Lefevre, 2000; Erduran and Tuncel, 2001; Erel et al., 2006; Ganor et al., 1991; Graham et al., 2004; Gullu et al., 2000; Maenhaut et al., 1999; Mamane et al., 1980; Manalis et al., 2005; Manoli et al., 2002; Mihalopoulos et al., 1997; Thomaidis et al., 2003; Vousta et al., 2002; Yatin et al., 2000) emphasized the diversity of the atmosphere over the Mediterranean basin. In Lebanon, seasonal dust storms coming from the Arabian (South-East) and Saharan Deserts (South-West) in the Fall and Spring mild seasons, constitute the major source of mineral elements (Kubilay et al., 2000). Long-range transport of pollutants coming from central Europe enrich the air with sulfur dioxide (SO2) (Ganor et al., 2000; Luria et al., 1996; Sciare et al., 2003; Tsitouridou et al., 2003; Zerefos et al., 2000), whereas marine aerosols contribute to sea-salt aerosols. Moreover, local emission cause an increase in the levels of nitrate and sulfate aerosols derived from oxides of nitrogen and SO2, respectively (Danalatos and Glavas, 1999; Erduran and Tuncel, 2001; Kassomenos et al., 1999). Sulfur (S) concentration increases in the hot and humid summer (June, July and August) due to the enhancement of photochemical oxidation of SO2, and drops in the rainy winter (December, January, and February) (Kouyoumdjian and Saliba, 2006). The purpose of this study was to determine the elemental content of PM10–2.5 and PM2.5 in Beirut during selected days in winter, summer, stormy and non-stormy episodes, using the particulate-induced X-ray emission (PIXE) technique. Also, a comparison between the elemental composition of the two particle sizes and the source apportionment through elemental–meteorological correlations are established.
Section snippets
Sampling
The sampling was conducted in one of the busiest areas of Beirut; Bourj Hammoud (33°53′N, 35°32′E) (Fig. 1) located in the North-Eastern suburb of Beirut at about 1 km away from the Mediterranean coast at an elevation of less than 10 m above sea level. This site is characterized by a high density of residential and commercial premises, and a very high volume of vehicular traffic. It also experiences a high volume of sea-spray, exhausts from Beirut harbor operations and some waste-mass burning
Results and discussion
The mass concentrations of PM10–2.5 and PM2.5 and their corresponding elemental composition (Si, S, Cl, K, Ca, Ti, Mn, Fe, Cu, Zn, and Pb) are presented in Table 2. Other elements such as V, Cr, Co, Ni, Cd, As, Se and Br were found to be below the limit of detection. Ca, Si and Fe prevailed in the PM10–2.5 samples forming an average of 17% of the total mass average. In PM2.5, this percentage decreased to 3%, while S; the most abundant element, constituted almost 4.6% of the average mass
Conclusions
Elemental analysis of PM10–2.5 and PM2.5 particles using PIXE analysis showed the presence of Si, S, Cl, K, Ca, Ti, Mn, Fe, Cu, Zn, and Pb. Based on the E.F. calculation, the crustal elements were defined as Si, K, Ti, Mn, Ca and Fe while the rest were classified as non-crustal. Their distribution between PM10–2.5 and PM2.5 and their source apportionment were as follows:
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Elevated concentrations of crustal elements, mostly present in PM10–2.5, were associated with desert storms coming from the
Acknowledgements
This study was supported by the University Research Board (URB) at the American University of Beirut. The authors would like to thank the California Air resources Board, specifically Dr. Bart Croes, for the donation of the virtual impactor. A special thank is also extended to the municipality of Bourj Hammoud, especially (Mrs. Arpiné Mangasarian), for their great cooperation and help, and the NOAA Laboratory for making HYSPLIT model available to researchers all over the world.
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