Seasonal variations of C 1 -C 4 alkyl nitrates at a coastal site in Hong Kong: Influence of photochemical formation and oceanic emissions

Five C -C alkyl nitrates (RONO ) were measured at a coastal site in Hong Kong in four selected months of 2011 and 2012. The total mixing ratios of C -C RONO (Σ RONO ) ranged from 15.4 to 143.7 pptv with an average of 65.9 ± 33.0 pptv. C -C RONO (2-butyl nitrate and 2-propyl nitrate) were the most ab...

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Veröffentlicht in:Chemosphere (Oxford) 2018-03, Vol.194, p.275
Hauptverfasser: Song, Junwei, Zhang, Yingyi, Huang, Yu, Ho, Kin Fai, Yuan, Zibing, Ling, Zhenhao, Niu, Xiaojun, Gao, Yuan, Cui, Long, Louie, Peter K K, Lee, Shun-Cheng, Lai, Senchao
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Sprache:eng
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Zusammenfassung:Five C -C alkyl nitrates (RONO ) were measured at a coastal site in Hong Kong in four selected months of 2011 and 2012. The total mixing ratios of C -C RONO (Σ RONO ) ranged from 15.4 to 143.7 pptv with an average of 65.9 ± 33.0 pptv. C -C RONO (2-butyl nitrate and 2-propyl nitrate) were the most abundant RONO during the entire sampling period. The mixing ratios of C -C RONO were higher in winter than those in summer, while the ones of methyl nitrate (MeONO ) were higher in summer than those in winter. Source analysis suggests that C -C RONO were mainly derived from photochemical formation along with biomass burning (58.3-71.6%), while ocean was a major contributor to MeONO (53.8%) during the whole sampling period. The photochemical evolution of C -C RONO was investigated, and found to be dominantly produced by the parent hydrocarbon oxidation. The notable enrichment of MeONO over C -C RONO was observed in a summer episode when the air masses originating from the South China Sea (SCS) and MeONO was dominantly derived from oceanic emissions. In order to improve the accuracy of ozone (O ) prediction in coastal environment, the relative contribution of RONO from oceanic emissions versus photochemical formation and their coupling effects on O production should be taken into account in future studies.
ISSN:1879-1298
DOI:10.1016/j.chemosphere.2017.11.104