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Aircraft measurements reveal vertical distribution of atmospheric ammonia over the North China Plain in early autumn

机译:飞机测量揭示了初秋北中国北方大气氨的垂直分布

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Ammonia (NH3) is an atmospheric contaminant contributing to the formation of fine particles, e.g., particulate matter (PM2.5), which induces respiratory diseases. In the atmosphere, horizontal NH(3)levels in the stratosphere, middle-upper troposphere, and planetary boundary layer have been studied using surface monitoring and satellite data, yet NH(3)vertical distribution above the planetary boundary layer within the lower troposphere is poorly known. In particular, vertical NH(3)data would provide information on the role of NH(3)in secondary aerosol formation in the lower troposphere. Here, two NH(3)profiles on September 2 and 3, 2017, were obtained by in situ aircraft measurement, plus temperature, dew point temperature, and relative humidity over the North China Plain. We also used synoptic analysis and WRF-CHEM modeling. We observed one pollution layer from 2800 to 3500 m on September 2, and two pollution layers, 1750-2250 m and 2500-3450 m, on September 3. Results show that the highest NH(3)concentration above the planetary boundary layer was 28.0 ppb at 2500-3450 m over Baoding, comparable to that observed in the planetary boundary layer, of 33.1 ppb, on September 3, 2017. The transport of clean air masses from the northwest of China led to a sharp decrease in NH(3)concentration between 2300 and 2800 m and highlighted a relatively high NH(3)concentration of 20.0 ppb at approximately 3000 m, which led to the formation of an elevated pollution layer on September 2. The highest pollution layer of 28.0 ppb at 2500-3450 m on September 3, 2017, appears to be driven by the westerly wind, whereas the lower pollution layer of 20.1 ppb at 1750-2250 m was influenced by both local pollutants of the North China Plain and a vertical entrainment effect.
机译:氨(NH3)是一种大气污染物,有助于形成细颗粒,例如颗粒物质(PM2.5),其诱导呼吸系统疾病。在大气中,使用表面监测和卫星数据研究了平流层,中上层对流层和行星边界层中的水平NH(3)水平,然而NH(3)较低对流层内行星边界层上方的垂直分布是众所周知。特别地,垂直NH(3)数据将提供有关NH(3)在较低对流层中的二级气溶胶形成中的作用的信息。在这里,2017年9月2日和3日的两种NH(3)个概况是通过原位飞机测量,加上温度,露点温度和华北平原相对湿度获得的。我们还使用了Synoptic分析和WRF-Chem建模。 9月2日,我们观察了一个污染层,从2800到3500米,和2月3日,两种污染层,1750-2250 m和2500-3450 m,结果表明,行星边界层上方的最高NH(3)浓度为28.0在2017年9月3日,在行星边界层的平行边界层中观察到的PPB,与行星边界层观察到的,在2017年9月3日。来自中国西北部的清洁空气群众的运输导致NH(3)的急剧下降浓度在2300和2800米之间,并在约3000米处突出相对高的NH(3)浓度为20.0ppb,导致9月2日的污染层的形成。28.0 ppb的最高污染层2500-3450 m 2017年9月3日,似乎是由西风的驱动,而1750-2250米的20.1ppb的较低污染层受到华北平原的当地污染物和垂直夹带效果的影响。

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