Articolo in rivista, 2015, ENG, 10.1021/acs.est.5b00969

A model study of global mercury deposition from biomass burning

De Simone F., Cinnirella S., Gencarelli C., Yang X., Hedgecock I., Pirrone N,

CNR-IIA

Mercury emissions from biomass burning are not well characterized and can differ significantly from year to year. This study utilizes three recent biomass burning inventories (FINNv1.0, GFEDv3.1, and GFASv1.0) and the global Hg chemistry model, ECHMERIT, to investigate the annual variation of Hg emissions, and the geographical distribution and magnitude of the resulting Hg deposition fluxes. The roles of the Hg/CO enhancement ratio, the emission plume injection height, the Hg(g) 0 oxidation mechanism and lifetime, the inventory chosen, and the uncertainties with each were considered. The greatest uncertainties in the total Hg deposition were found to be associated with the Hg/CO enhancement ratio and the emission inventory employed. Deposition flux distributions proved to be more sensitive to the emission inventory and the oxidation mechanism chosen, than all the other model parametrizations. Over 75% of Hg emitted from biomass burning is deposited to the world's oceans, with the highest fluxes predicted in the North Atlantic and the highest total deposition in the North Pacific. The net effect of biomass burning is to liberate Hg from lower latitudes and disperse it toward higher latitudes where it is eventually deposited.

Environmental science & technology (Wash., D.C., Online) 49 , pp. 6712–6721

Keywords

Gaseous Elemental Mercury, Emission, Deposition

CNR authors

De Simone Francesco, Pirrone Nicola, Hedgecock Ian Michael, Gencarelli Christian Natale, Cinnirella Sergio

CNR institutes

IIA – Istituto sull'inquinamento atmosferico

ID: 330130

Year: 2015

Type: Articolo in rivista

Creation: 2015-05-04 12:51:00.000

Last update: 2023-11-09 22:34:56.000

External links

OAI-PMH: Dublin Core

OAI-PMH: Mods

OAI-PMH: RDF

DOI: 10.1021/acs.est.5b00969

External IDs

CNR OAI-PMH: oai:it.cnr:prodotti:330130

DOI: 10.1021/acs.est.5b00969