Detalhes bibliográficos
Ano de defesa: |
2024 |
Autor(a) principal: |
Almeida, Bernardo Sartori Chede Rosauro de |
Orientador(a): |
Não Informado pela instituição |
Banca de defesa: |
Não Informado pela instituição |
Tipo de documento: |
Dissertação
|
Tipo de acesso: |
Acesso aberto |
Idioma: |
eng |
Instituição de defesa: |
Não Informado pela instituição
|
Programa de Pós-Graduação: |
Não Informado pela instituição
|
Departamento: |
Não Informado pela instituição
|
País: |
Não Informado pela instituição
|
Palavras-chave em Português: |
|
Link de acesso: |
https://app.uff.br/riuff/handle/1/35691
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Resumo: |
Mercury (Hg) is released via natural and anthropogenic sources. Atmospheric deposition via dry and wet deposition is the main source of Hg to the continents and oceans. Organic matter (OM) is the primary driver of Hg accumulation in marine sediments. Previous studies reported that Hg is sensitive to past climate changes and that global and regional climatic factors can control its environmental dynamics. Here, we used sediment core M125-95-3 collected at the western tropical South Atlantic to investigate Hg deposition and accumulation changes in the marine realm over the last 70 ka. Our records show higher concentration during the glacial period than in the interglacial period probably due to increased atmospheric dust. On millennial-scale events, the increased residence time of North Atlantic Deep Water (NADW) enhanced the regenerative scavenging of Hg, which reduced Hg concentration in M125-95-3 core. In addition, the dilution effect might have reduced the Hg concentration further during Heinrich stadials (HS) due to increased terrigenous input via the São Francisco River. Altogether, the results suggest a strong influence of deep ocean circulation on the deposition and accumulation of Hg in marine sediments in the western tropical South Atlantic on millennial timescales, highlighting long-term oceanic processes that act on the geochemical cycle of Hg. |