Molecular weight-dependent abundance, absorption, and fluorescence characteristics of water-soluble organic matter in atmospheric aerosols

被引:9
|
作者
Fan, Xingjun [1 ]
Cai, Feng [1 ,4 ]
Xu, Cuncun [1 ,2 ,3 ]
Yu, Xufang [1 ]
Wang, Yan [1 ]
Xiao, Xin [1 ]
Ji, Wenchao [1 ]
Cao, Tao [2 ,3 ]
Song, Jianzhong [2 ]
Peng, Ping'an [2 ]
机构
[1] Anhui Sci & Technol Univ, Coll Resource & Environm, Fengyang 233100, Peoples R China
[2] Chinese Acad Sci, Guangzhou Inst Geochem, State Key Lab Organ Geochem, Guangzhou 510640, Peoples R China
[3] Univ Chinese Acad Sci, Beijing 100049, Peoples R China
[4] Nanjing Forestry Univ, Coll Biol & Environm, Coinnovat Ctr Sustainable Forestry Southern China, Longpan Rd 159, Nanjing 210037, Jiangsu, Peoples R China
关键词
Water-soluble organic matter; Ultrafiltration; Apparent molecular weight; Light absorption; EEM-PARAFAC; HUMIC-LIKE SUBSTANCES; SEPARATED BROWN CARBON; FENTON-LIKE OXIDATION; PARTICULATE MATTER; OPTICAL-PROPERTIES; LIGHT-ABSORPTION; SIZE; HULIS; EXCITATION; URBAN;
D O I
10.1016/j.atmosenv.2020.118159
中图分类号
X [环境科学、安全科学];
学科分类号
08 ; 0830 ;
摘要
Water-soluble organic matter (WSOM) plays a significant role in solar radiative forcing and atmospheric chemistry. Its chemical composition and properties are highly molecular weight (MW)-dependent, but are still poorly understood. In this study, 10 PM2.5 samples were collected at a rural site in China, and the WSOM therein was fractionated into three MW fractions, >5 kDa (F1), 1-5 kDa (F2), and <1 kDa (F3), using an ultrafiltration (UF) system. The abundance, optical properties, and fluorescence properties of the three MW fractions were comprehensively determined using a total organic carbon (TOC) analyzer, ultraviolet-visible (UV-vis) spectroscopy, and excitation-emission matrix (EEM) fluorescence spectroscopy combined with parallel factor (PARAFAC) modeling. The proportional TOC and Abs(365) distributions of the MW fractions were F1:F2:F3 approximate to 24:22:54 and 40:24:36, respectively. This suggested that the major OC species in bulk WSOM were partitioned into the low MW (<1 kDa) fraction, while the major light-absorbing chromophores were partitioned into the large MW (F1 + F2, >1 kDa) fraction, and were especially prevalent in the >5 kDa fraction. The optical parameters, i.e., SUVA(254) and MAE(365), generally increased with the apparent increase in MW, suggesting that the higher MW fractions might have a stronger aromaticity and light absorption capacity. The EEM-PARAFAC analysis identified three humic-like substances (HULIS) (C1-C3) and one protein-like (C4) substance for all MW fractions, of which the proportional distributions were observed as C1:C2:C3:C4 approximate to 20:24:41:15, 21:23:44:12, and 41:22:13:24 for F1, F2, and F3, respectively. This indicated that the >1 kDa fraction was enriched in highly-oxygenated HULIS (C3), whereas the <1 kDa fraction had more less-oxygenated HULIS (C1) and protein-like (C4) substances than the >1 kDa fraction. The study provided a detailed insight of the MWdependent characteristics of WSOM by reducing their heterogeneity and complexity, which is of great significance for further understanding the chemical properties and structures of WSOM.
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页数:9
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