Precise size distribution measurement of aerosol particles and fog droplets in the open atmosphere
Precise size distribution measurement of aerosol particles and fog droplets in the open atmosphere
复制标题
大气中气溶胶颗粒和雾滴的精确尺寸分布测量
DOI:
10.1364/oe.27.00a890
复制
发表时间:
2019-06-10
期刊:
影响因子:
3.8
通讯作者:
Hua, Dengxin
中科院分区:
文献类型:
--
作者:
Di, Huige;Wang, Zhixiang;Hua, Dengxin
A precise measurement for the aerosol particle size distribution and fog droplet size distribution simultaneously in the open atmosphere is proposed. The extinction coefficient and small-angle forward scattering measurement are integrated into the detection for particle size distribution in the open atmosphere, and can achieve the fine detection of the particles in the atmosphere with radius between 0.1 to 30 Ant The key technology including optimal scattering angle in small-angle forward scattering measurement and optimal wavelengths selection are discussed and solved in detail. The fourteen different particle size distributions including aerosol size distributions and fog droplet size distributions are used for the determination of optimal forward scattering angle and wavelengths. The optimal forward scattering angle is calculated to be 1.1 degrees. Seven wavelengths for extinction coefficients and five wavelengths for forward scattering coefficients are chosen for the retrieval of particle size distribution in the measurement. The regularization inversion of optical parameters for the retrieval of particle size distribution is described. The aerosol particle size distributions measured by particle spectrometer and actual fog particle size distributions are used for the method test and the reconstructions of particle size distributions. The inversion results show that the method can achieve the precise measurements of aerosol particle size distribution and fog droplet size distribution. The error influence on the inversion results of distributions is discussed. Based on the sensitivity analysis of inversion results, the feasibility of measurement in the real atmosphere is analyzed and discussed, and the scheme of detection system is provided. (C) 2019 Optical Society of America under the terms of the OSA Open Access Publishing Agreement