the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Heterogeneous Phototransformation of Halogenated Polycyclic Aromatic Hydrocarbons: Influencing Factors, Mechanisms and Products
Abstract. Chlorinated and brominated polycyclic aromatic hydrocarbons (XPAHs) are emerging pollutants widely found in atmospheric particulate matter (PM). However, their environmental transformation mechanisms remain poorly understood. In this study, we collected PM samples of varying sizes over a year for XPAH analysis and found the average concentrations of XPAHs peaked in winter and were dominated by PM1 (47.0 %). Correlation analysis with relevant meteorological parameters showed strong associations between XPAH fluctuations and PM, temperatures, and humidity. Hence, controlled laboratory experiments were conducted to explore the influence of particle size, sunlight duration, temperature, humidity, and oxidant concentrations on XPAH transformation. Our results indicated that the transformation rates of XPAHs were influenced by the parent polycyclic aromatic hydrocarbon structures, with phenanthrene < fluoranthene < pyrene < benz[a]anthracene ≈ anthracene < benzo[a]pyrene, as well as the substitution of halogens: chlorinated < brominated. Furthermore, the photo irradiation promoted the heterogeneous transformation of XPAHs, with this process being accelerated by the increased concentrations of reactive oxygen species and elevated temperature, peaking at the humidity level of 45 %. The transformation products were identified by nontarget analysis. We then proposed phototransformation pathways for XPAHs, suggesting a mechanism involving dechlorination followed by oxidation. Predictions were made regarding the persistence, bioaccumulation, long-range transportation, and toxicities of XPAHs and their transformation products, showing a decrement in environmental risks as the transformation progressed. This study provides novel insights into the primary influencing factors for particulate XPAH variations and the mechanisms of heterogeneous phototransformation.
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Status: open (until 12 Dec 2024)
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RC1: 'Comment on egusphere-2024-2814', Ahsan Habib, 01 Nov 2024
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The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2814/egusphere-2024-2814-RC1-supplement.pdf
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