洛杉矶大气中痕量金属的大小分布

James M. Lyons , Chandra Venkataraman , Hilary Hafner Main , S.K. Friedlander
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引用次数: 40

摘要

1989年冬季和夏季,在洛杉矶地区的两个地点用级联冲击器测量了Fe、Pb、Mz、Zn、Cu和Ni的粒度分布。采取措施尽量减少颗粒反弹,并进行了x射线荧光元素分析。测得的铁粒度分布一致,悬浮粉尘是主要来源。铅的分布具有多模态,主要受汽车尾气排放、颗粒生长和悬浮尘埃的影响。以铁为示踪剂,考察了悬浮尘的重要性以及铁与铅等金属的悬浮尘比。锰的分布与铅的分布相似,汽车尾气和悬浮粉尘是重要的污染源。Zn、Cu和Ni的粒度分布表明,这些金属在直径小于1μm的颗粒中含量显著,表明它们是人为来源。在直径大于2 μm的颗粒中,悬浮粉尘是Zn的重要来源,而不是Cu和Ni的主要来源。
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Size distributions of trace metals in the Los Angeles atmosphere

Particle size distributions of Fe, Pb, Mz, Zn, Cu and Ni were measured at two locations in the Los Angeles area during the winter and summer of 1989 using a cascade impactor. Measures were taken to minimize particle bounce and elemental analysis was performed by X-ray fluorescence. Measured Fe size distributions were consistent, with suspended dust being the major source. Pb distributions were observed to be multimodal with modes due to automotive emissions, particle growth and suspended dust. The importance of suspended dust was investigated using Fe as tracer and suspended dust ratios of Fe to Pb and other metals. Mn distributions were observed to be similar to those of Pb with automotive emissions and suspended dust being important sources. Particle size distributions of Zn, Cu and Ni showed significant amounts of these metals to be persent in particles less than 1μm in diameter, indicating anthropogenic sources. Suspended dust was found to be an important source of Zn, but not of Cu or Ni, in particles with diameters greater than 2 μm.

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