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Published on: September 6, 2018
Using Mercury Stable Isotopes to Quantify Directional Soil-Atmosphere Hg(0) Exchanges in Rice Paddy Ecosystems:
Kun Zhang1,2, Qiang Pu1, Jiang Liu1,3
1State Key Laboratory of Environmental Geochemistry, Institute of Geochemistry, Chinese Academy of Sciences, Guiyang 550081, China.
Gaseous elemental mercury emissions from soils are significant. This study used mercury isotopes to differentiate reduction pathways, revealing photoreduction as the main source, but also quantifying microbial and abiotic contributions to atmospheric mercury release.
Area of Science:
- Environmental Chemistry
- Geochemistry
- Biogeochemistry
Background:
- Gaseous elemental mercury (Hg(0)) emissions from soils represent a substantial portion of global Hg(0) emissions.
- Previous research often overlooks distinct biotic and abiotic reduction pathways, potentially underestimating soil Hg(0) emissions, particularly from paddy soils.
- Understanding these diverse emission sources is crucial for accurate atmospheric mercury budget assessments.
Purpose of the Study:
- To differentiate and quantify mercury (Hg) reduction pathways (photoreduction, microbial reduction, abiotic dark reduction) in paddy soils using stable Hg isotopes.
- To determine the relative contributions of these pathways to gaseous elemental mercury (Hg(0)) emissions from paddy soils.
- To improve the estimation of Hg(0) emissions from rice paddy ecosystems by accounting for multiple reduction processes.
Main Methods:
- Utilized stable mercury (Hg) isotopes to analyze the isotopic composition (δ202Hg and Δ199Hg) of Hg(0) produced via different reduction pathways.
- Employed an isotopic signature-based ternary mixing model to apportion Hg(0) emissions among photoreduction, microbial reduction, and abiotic dark reduction.
- Measured Hg(0) exchange fluxes between the atmosphere and paddy soils under various conditions.
Main Results:
- Significantly distinct isotopic signatures were observed for Hg(0) originating from photoreduction, microbial reduction, and abiotic dark reduction.
- Hg(0) emissions from paddy soils were predominantly driven by release into the atmosphere, with average fluxes ranging from 2.2 to 16.8 ng m-2 h-1.
- Photoreduction was identified as the primary contributor to Hg(0) emissions, while microbial and abiotic dark reduction accounted for up to 36% and 25% respectively on day 110.
Conclusions:
- Mercury isotope analysis provides a powerful tool for distinguishing Hg(0) reduction pathways in soils.
- Paddy soils are significant sources of atmospheric Hg(0), with contributions from multiple biotic and abiotic processes.
- Accurate estimation of soil Hg(0) emissions requires consideration of photoreduction, microbial reduction, and abiotic dark reduction pathways.
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