Source and Distribution of Emerging and Legacy Persistent Organic Pollutants in the Basins of the Eastern Indian Ocean

被引:23
|
作者
Cong, Bailin [1 ,2 ]
Li, Shuang [1 ]
Liu, Shenghao [1 ]
Mi, Wenying [3 ]
Liu, Shengfa [1 ]
Zhang, Zhaohui [1 ]
Xie, Zhiyong [4 ]
机构
[1] Minist Nat Resources, Inst Oceanog 1, Qingdao 266061, Peoples R China
[2] Fuzhou Univ, Sch Adv Mfg, Fuzhou 350108, Peoples R China
[3] MINJIE Inst Environm Sci & Hlth Res, D-21502 Geesthacht, Germany
[4] Helmholtz Zentrum Hereon, Inst Coastal Environm Chem, D-21502 Geesthacht, Germany
关键词
persistent organic pollutants (POPs); Eastern Indian Ocean (EIO); basins; pollutants sources; depositional flux (DF); mass inventory (MI); POLYBROMINATED DIPHENYL ETHERS; ORGANOPHOSPHORUS FLAME RETARDANTS; POLYCYCLIC AROMATIC-HYDROCARBONS; DECHLORANE PLUS; PHTHALATE-ESTERS; ACID-ESTERS; BISPHENOL-A; LAND-USE; SEDIMENTS; WATER;
D O I
10.1021/acs.est.1c08743
中图分类号
X [环境科学、安全科学];
学科分类号
08 ; 0830 ;
摘要
Persistent organic pollutants (POPs) have received significant and ongoing attention. To establish favorable regulatory policies, it is vital to investigate the occurrence, source, and budgets of POPs worldwide. POPs including phthalic acid esters (PAEs), organophosphate esters (OPEs), brominated flame retardants (BFRs), and highly chlorinated flame retardants (HFRs) have not yet been examined in the Eastern Indian Ocean (EIO). In this study, the distribution of POPs has been investigated from surface sediments with the depth of 4369-5742 m in the Central Indian Ocean Basin (CIOB) and Wharton Basin (WB) of EIO. The average (+/- SD) concentrations of Sigma(11)PAEs, Sigma 11OPEs, Sigma(4) BFRs, and Sigma(5)HFRs were 1202.0 +/- 274.36 ng g(-1) dw, 15.3 +/- 7.23 ng g(-1) dw, 327.6 +/- 211.74 pg g(-1) dw, and 7.9 +/- 7.45 pg g(-1) dw, respectively. The high abundance of low-molecular-weight (LMW) PAEs, chlorinated OPEs, LMW BDEs, and anti-Dechlorane Plus indicated the pollution characteristics in the EIO. Correlation analysis demonstrated that LMW compounds may be derived from the high-molecular-weight compounds. The monsoon circulation, currents, and Antarctic Bottom Water may be the main drivers. POP accumulation rate, depositional flux, and mass inventory in the Indian Ocean were also estimated.
引用
收藏
页码:4199 / 4209
页数:11
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