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1.
Ciênc. cult. (Säo Paulo) ; 51(5/6): 363-71, set.-dez. 1999. mapas, tab, graf
Artigo em Inglês | LILACS | ID: lil-260624

RESUMO

Atmospheric Hg deposition over Brazil is presented for the past 30,000 years as a tracer of the different natural and anthropogenic processes affecting the atmospheric environment of Brazil. During most of the prehistoric period, atmospheric deposition rates were rather constant with an average of about 2 mug m(-2) yr(-1). Peak deposition, ranging from 4 to 6 mug m2 y(-1), occurred at least during two periods between 3,300 and 3,600 BP and between 8,500 to 12,000 BP, and during the last glacial maximum (LGM), at about 18,000 years BP. These periods were characterized by drier, colder climates with high frequency of fores fires, as shoen by correlation with coal and pollen distribution data. During the colonial period Hg atmospheric deposition rates were much higher, about four times the prehistoric background and reached 6 to 8 mug m(-2) yr(-1). These increasing Hg deposition rates can only be explained by the large Hg emissions in South and Central America from Spanish silver mines, which emitted to the continent's environment about 200,000 tons of Hg from 1580 to 1820. During the present century, Hg deposition rates varied according to the region of the country. In the Amazon region, where gold mining is the major source of Hg emission to the atmosphere, deposition rates increased continuously during the last 40 years, reaching 8 to 10 mug m(-2) yr(-1). In the industrialized Southeast, Hg deposition was higher during the mild 1960s and 1970s, ranging from 80 to 130 mug m(-2) yr(-1), but decreased to 20 to 30 mug m(-2) yr(-1) in the 1990s, due to the enforcement of emission control policies. However, where Hg emissions are mostly from urban, nonpoint sources, such as along the high urbanized coastal area, Hg deposition, although smaller, increased steadily from the 1940s reaching a maximum at surface sediment layers of about 40.0 mug (-2) yr(-1). The results presented suggest Hg as a reliable tracer of natural (paleoclimatic changes) and anthropogenic (industrial and mining emissions) processes able to affect the atmosphere in Brazil.


Assuntos
Atmosfera/análise , Mercúrio/análise , Brasil
2.
Ciênc. cult. (Säo Paulo) ; 50(4): 293-7, jul.-ago. 1998. mapas, tab
Artigo em Inglês | LILACS | ID: lil-262168

RESUMO

Mercury emissions to soil, waters, and the atmosphere in the Sepetiba Bay basin were estimated by means of emission factors and data base of major industrial and urban sources of Hg. This approach is the most effective in assessing pollutant loads from diffuse sources, as in the case of Hg in the Sepetiba Bay basin. Total Hg emission ranges from 20 to 364 kg yr(-1). A significant fraction of this input is to the atmosphere, ranging from 115 to 149 kg yr(-1) (41 to 58 per cent), mostly due to emissions from iron and steel production and an oil fired power plant. Inputs to soil range from 84 to 215 kg yr(-1) (42 to 59 per cent), mostly from an urban ladfill and from metal manufacturing. Direct inputs to surface water are small (<1.0 kg yr(-1). Estimated total and atmospheric emissions agree with measurements of atmospheric Hg deposition and with preliminary data on fluvial systems.


Assuntos
Humanos , Poluentes Ambientais/análise , Mercúrio/análise , Poluentes Atmosféricos/análise , Brasil , Poluentes Industriais , Poluentes da Água/análise , Poluição de Rios , Poluentes do Solo/análise
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