Five-year records of mercury wet deposition flux at GMOS sites in the Northern and Southern hemispheres

Author:

Sprovieri FrancescaORCID,Pirrone Nicola,Bencardino Mariantonia,D'Amore Francesco,Angot Helene,Barbante CarloORCID,Brunke Ernst-Günther,Arcega-Cabrera Flor,Cairns Warren,Comero Sara,Diéguez María del CarmenORCID,Dommergue AurélienORCID,Ebinghaus Ralf,Feng Xin BinORCID,Fu XuewuORCID,Garcia Patricia Elizabeth,Gawlik Bernd Manfred,Hageström Ulla,Hansson Katarina,Horvat Milena,Kotnik Jože,Labuschagne CasperORCID,Magand Olivier,Martin Lynwill,Mashyanov Nikolay,Mkololo ThumekaORCID,Munthe John,Obolkin VladimirORCID,Ramirez Islas Martha,Sena Fabrizio,Somerset Vernon,Spandow Pia,Vardè Massimiliano,Walters Chavon,Wängberg Ingvar,Weigelt Andreas,Yang Xu,Zhang Hui

Abstract

Abstract. The atmospheric deposition of mercury (Hg) occurs via several mechanisms, including dry and wet scavenging by precipitation events. In an effort to understand the atmospheric cycling and seasonal depositional characteristics of Hg, wet deposition samples were collected for approximately 5 years at 17 selected GMOS monitoring sites located in the Northern and Southern hemispheres in the framework of the Global Mercury Observation System (GMOS) project. Total mercury (THg) exhibited annual and seasonal patterns in Hg wet deposition samples. Interannual differences in total wet deposition are mostly linked with precipitation volume, with the greatest deposition flux occurring in the wettest years. This data set provides a new insight into baseline concentrations of THg concentrations in precipitation worldwide, particularly in regions such as the Southern Hemisphere and tropical areas where wet deposition as well as atmospheric Hg species were not investigated before, opening the way for future and additional simultaneous measurements across the GMOS network as well as new findings in future modeling studies.

Funder

Seventh Framework Programme

Publisher

Copernicus GmbH

Subject

Atmospheric Science

Reference83 articles.

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