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Identifying regional soil as the potential source of PM_(2.5) particulate matter on air filters collected in Imperial Valley, California - A Raman micro-spectroscopy study

机译:确定区域土壤是在加利福尼亚帝国谷收集的空气过滤器上PM_(2.5)颗粒物的潜在来源-拉曼光谱研究

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This work explores the use of Raman micro-spectroscopy to determine sources of airborne particulate matter collected on PM2.5 air filters in Imperial Valley, California. The goal is to examine if nearby soil is a potential source of particles sampled on air filters deployed in an urbanized desert area during events of unusually high PM2.5 excursions. Particle specific composition information can be an indicator of potential origin. This can provide insights into the source of unexpectedly high proportion of large particles sampled on PM2.5 filters in the vicinity of Imperial Valley. The measured spectral correspondence between the filter and soil particles, in the size range of 2.5-10 mu m, is consistent with windblown dust being a likely source of the larger (>2.5 mu m) particles collected on the PM(2.5 )filters. Additionally, these particles were identified as components of commonly occurring crustal minerals in the vicinity of the sampling site, such as iron oxides, hydroxides, sulfides, titanium dioxides and aluminosilicates. A substantial portion of the analyzed filter particles displayed a strong broadband fluorescence signal, which is consistent with the presence of organic matter and has been recognized as a marker for soil related origin of the filter particles. Elemental carbon (soot) was found to be prevalent among the particles as well, suggesting the existence of combustion related sources. Comparison between a heavily loaded filter sample and a filter with a more typical, lower loading did not show any obvious difference in chemical compositions. In both cases the particles appeared to be of crustal origin with the prevalence of elemental carbon. The primary difference between these two filter samples appear to be their particle size distribution - the heavily loaded filter sample contained greater proportion of large particles (>2.5 mu m), and was more consistent with spectral signature of soils analyzed from the region. Published by Elsevier Ltd.
机译:这项工作探索了使用拉曼显微光谱法确定加利福尼亚帝国谷PM2.5空气滤清器上收集的空气中颗粒物的来源。目的是检查在异常高PM2.5漂移事件期间,附近土壤是否是在城市沙漠地区部署的空气滤清器上采样的潜在颗粒源。特定于颗粒的成分信息可以指示潜在来源。这可以洞悉帝国谷附近PM2.5过滤器上采样到的大颗粒的比例出乎意料地高。在2.5-10微米的尺寸范围内,过滤器与土壤颗粒之间测得的光谱对应关系与风吹尘埃(可能是PM(2.5)过滤器上收集的较大颗粒(> 2.5微米)的可能来源)一致。此外,这些颗粒被确定为采样点附近常见的地壳矿物的成分,例如氧化铁,氢氧化物,硫化物,二氧化钛和硅铝酸盐。分析的过滤器颗粒的很大一部分显示出很强的宽带荧光信号,这与有机物的存在是一致的,并且已被认为是与土壤相关的过滤器颗粒起源的标记。还发现元素碳(烟灰)在颗粒中也很普遍,表明存在与燃烧有关的来源。重载过滤器样品与更典型,更低载量的过滤器之间的比较未显示出化学成分的任何明显差异。在这两种情况下,颗粒似乎都是地壳起源的元素碳。这两个过滤器样品之间的主要区别似乎在于它们的粒径分布-重载的过滤器样品包含较大比例的大颗粒(> 2.5微米),并且与从该区域分析的土壤的光谱特征更加一致。由Elsevier Ltd.发布

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