کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
4425017 | 1619206 | 2012 | 8 صفحه PDF | دانلود رایگان |

∑30PAH gas phase concentrations (13–86 and 22–40 ng m−3 in the Mediterranean and Black Seas, respectively) dominated the atmospheric levels due to the high contribution of phenanthrene, dibenzothiophene and their alkylated derivates. The high variability of PAH atmospheric concentrations in the different sub-basins is due to several factors (i.e. air-mass trajectory, proximity to sources and losses by deposition). The ∑30PAH atmospheric deposition (dominated by low MW PAH net air–water diffusive fluxes) is estimated to be ∼3100 ton y−1 (Mediterranean) and ∼500 ton y−1 (Black Sea). Net volatilization for certain PAHs was estimated. Deposition fluxes (1–2 orders of magnitude higher than reported PAH settling fluxes in the water column) confirm an important depletion/sink of water column PAH in the photic zone, especially for low MW PAHs. Degradation processes in the water column may be responsible for this decoupling. Conversely, high MW PAHs dry deposition fluxes are similar to their settling fluxes.
Figure optionsDownload as PowerPoint slideHighlights
► First comprehensive assessment of atmospheric PAH levels and deposition across the Mediterranean Sea.
► PAH atmospheric concentrations are highly variable across the Mediterranean Sea.
► Mediterranean Sea open waters receive ∼3100 ton of PAHs each year from the atmosphere.
► Important depletion of low MW PAH water column concentrations in the photic zone.
► Degradation processes most likely responsible of the atmospheric deposition – settling fluxes decoupling.
Journal: Environmental Pollution - Volume 166, July 2012, Pages 40–47