Mercury Pollution In Snow Cover Around Thermal Power Plants In Cities (Omsk, Kemerovo, Tomsk Regions, Russia)

Although snow cover is studied as an efficient scavenger for atmospheric mercury (Hg), up to now little is known about Hg behaviour in urban snow cover impacted by thermal power plants (TPPs) during the winter heating season. This study is focused on quantification of Hg in the particulate phase in...

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Bibliographic Details
Published in:GEOGRAPHY, ENVIRONMENT, SUSTAINABILITY
Main Authors: Anna V. Talovskaya, Egor G. Yazikov, Nina A. Osipova, Elena E. Lyapina, Victoria V. Litay, George Metreveli, Junbeum Kim
Other Authors: The experimental procedures were carried out at Tomsk Polytechnic University within the framework of Tomsk Polytechnic University Competitiveness Enhancement Program Grant in the Group of Top Level World Research and Academic Institutions. This work was partially supported by the Russian Foundation for Basic Research (grant number 16-45-700184p_a, 2016–2018) and in the framework of the state budget theme No. AAAA-A17-117013050031-8. We are grateful Sergey Ilenok for his assistance in SEM-EDX analysis and Ekaterina Filimonenko for her help in Hg measurements (Uranium Geology International Centre, TPU), Raisa Abramova and Muriel Whitchurch for their comments during the manuscript preparation.
Format: Article in Journal/Newspaper
Language:English
Published: Russian Geographical Society 2019
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Online Access:https://ges.rgo.ru/jour/article/view/906
https://doi.org/10.24057/2071-9388-2019-58
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Summary:Although snow cover is studied as an efficient scavenger for atmospheric mercury (Hg), up to now little is known about Hg behaviour in urban snow cover impacted by thermal power plants (TPPs) during the winter heating season. This study is focused on quantification of Hg in the particulate phase in snow cover and estimation of atmospheric particulate Hg (HgP) depositional fluxes around urban TPPs in cities of Omsk, Kemerovo, Yurga, Tomsk (the south part of Western Siberia, Russia) to provide new insight into Hg occurrence in urban snow. The results demonstrate that the mean Hg content in the particulate phase of snow varied from 0.139 to 0.205mg kg-1, possibly depending on thermal power of TPPs and fuel type used. The estimated mean atmospheric HgP depositional fluxes ranged from 6.6 to 73.1 mg km-2 d-1. Around thermal power plants atmospheric HgP depositional flux was controlled by particulate load. Higher Hg contents in the particulate phase of snow and higher atmospheric HgP depositional fluxes observed in relation to the background values, as well as high enrichment factors determined for Hg in the particulate phase of snow relative to the mean Hg content in the Earth’s crust showed that the snow pollution with Hg is of anthropogenic origin. The coexistence of Hg and S observed for the particulate phase of snow indicated the possible presence of mercury sulfide in this phase. The parameters like Hg content in the particulate phase of snow and HgP atmospheric flux can be used as markers for the identification of coal combustion emission sources.