期刊
ATMOSPHERIC ENVIRONMENT
卷 45, 期 24, 页码 3996-4001出版社
PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.atmosenv.2011.04.059
关键词
Dust storm; Particle concentration; Particle size; Visibility; Air pollution
Particle number concentrations and size distributions, visibility and particulate mass concentrations and weather parameters were monitored in Brisbane, Australia, on 23 September 2009, during the passage of a dust storm that originated 1400 km away in the dry continental interior. The dust concentration peaked at about mid-day when the hourly average PM(2.5) and PM(10) values reached 814 and 6460 mu g m(-3), respectively, with a sharp drop in atmospheric visibility. A linear regression analysis showed a good correlation between the coefficient of light scattering by particles (Bsp) and both PM(10) and PM(2.5). The particle number in the size range 0.5-20 mu m exhibited a lognormal size distribution with modal and geometrical mean diameters of 1.6 and 1.9 mu m, respectively. The modal mass was around 10 mu m with less than 10% of the mass carried by particles smaller than 2.5 mu m. The PM(10) fraction accounted for about 68% of the total mass. By mid-day, as the dust began to increase sharply, the ultrafine particle number concentration fell from about 6 x 10(3) cm(-3) to 3 x 10(3) cm(-3) and then continued to decrease to less than 1 x 10(3) cm(-3) by 14 h, showing a power-law decrease with Bsp with an R(2) value of 0.77 (p < 0.01). Ultrafine particle size distributions also showed a significant decrease in number during the dust storm. This is the first scientific study of particle size distributions in an Australian dust storm. (C) 2011 Elsevier Ltd. All rights reserved.
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