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杭州灰霾天气超细颗粒浓度分布特征
引用本文:陈秋方,孙在,谢小芳. 杭州灰霾天气超细颗粒浓度分布特征[J]. 环境科学, 2014, 35(8): 2851-2856
作者姓名:陈秋方  孙在  谢小芳
作者单位:中国计量学院计量测试工程学院, 杭州 310018;中国计量学院计量测试工程学院, 杭州 310018;中国计量学院计量测试工程学院, 杭州 310018
基金项目:国家自然科学基金项目(10972209);国家自然科学基金重点项目(11132008);浙江省自然科学基金项目(Y6090607)
摘    要:利用快速迁移率粒径谱仪(FMPS)对杭州2013年12月6~11日连续灰霾天气和灰霾消退过程超细颗粒进行监测,分析颗粒物浓度变化和粒径谱分布特征及其与气象的相关性.结果表明,颗粒物日变化特征为夜晚数浓度较高,凌晨数浓度开始降低,08:00和18:00上下班高峰期出现一个小峰值,体现出明显的交通源峰值,表明交通排放对大气污染影响较大.灰霾天气下颗粒物最高数浓度达到8.0×104cm-3.粒径谱呈双峰分布,峰值粒径分别为15 nm和100 nm,粒径在100 nm附近的粒子占大多数,粒子以爱根核模态和积聚模态为主,平均数量中位径CMD(count medium diameter)为85.89 nm.而在灰霾消退过程,颗粒物数浓度降低,峰值粒径向小粒径演变,粒径在100 nm附近的粒子逐渐减少,核模态粒子增多,大于积聚模态,平均CMD为58.64 nm.气象因素中能见度和风力与数浓度主要呈负相关,相关系数R分别为-0.225和-0.229,相对湿度与数浓度正相关,相关系数R为0.271,冬季大气比较稳定,水平温度与数浓度的相关性较小.研究灰霾天气数浓度分布和气象因素的综合影响对其形成机制及控制有重要意义.

关 键 词:灰霾  超细颗粒  数浓度  粒径谱  气象因子
收稿时间:2014-01-06
修稿时间:2014-03-01

Distribution of Atmospheric Ultrafine Particles During Haze Weather in Hangzhou
CHEN Qiu-fang,SUN Zai and XIE Xiao-fang. Distribution of Atmospheric Ultrafine Particles During Haze Weather in Hangzhou[J]. Chinese Journal of Environmental Science, 2014, 35(8): 2851-2856
Authors:CHEN Qiu-fang  SUN Zai  XIE Xiao-fang
Affiliation:College of Metrology & Measurement Engineering, China Jiliang University, Hangzhou 310018, China;College of Metrology & Measurement Engineering, China Jiliang University, Hangzhou 310018, China;College of Metrology & Measurement Engineering, China Jiliang University, Hangzhou 310018, China
Abstract:Atmospheric ultrafine particles(UFPs)were monitored with fast mobility particle sizer(FMPS) in continuous haze weather and the haze fading process during December 6 to 11, 2013 in Hangzhou. Particle concentration and size distribution were studied associated with meteorological factors. The results showed that number concentrations were the highest at night and began to reduce in the morning. There was a small peak at 8 o'clock in the morning and 18 o'clock in the afternoon. It showed an obvious peak traffic source, which indicated that traffic emissions played a great role in the atmospheric pollution. During haze weather, the highest number concentration of UFPs reached 8×104 cm-3. Particle size spectrum distribution was bimodal, the peak particle sizes were 15 nm and 100 nm respectively. Majority of UFPs were Aitken mode and Accumulation mode and the size of most particles concentrated near 100 nm. Average CMD(count medium diameter)was 85.89 nm. During haze fading process,number concentration and particles with size around 100 nm began to reduce and peak size shifted to small size. Nuclear modal particles increased and were more than accumulation mode. Average CMD was 58.64 nm. Meteorological factors such as the visibility and wind were negatively correlated with the particle number concentration. Correlation coefficient R were -0.225 and -0.229.The humidity was correlated with number concentration. Correlation coefficient R was 0.271.The atmosphere was stable in winter and the level temperature had small correlation with number concentration. Therefore, study on distribution of atmospheric ultrafine particles during haze weather had the significance on the formation mechanism and control of haze weather.
Keywords:haze weather  ultrafine particles  number concentration  size distribution  meteorological factors
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