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Kabupaten Nias Selatan

Badan Riset dan Inovasi Nasional

Informasi Dataset

07-11-2022

12-08-2024

78b5002c-4762-4425-8ae2-29e862a6de7a

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INFORMASI: Data berikut ini masih dalam proses pemenuhan Prinsip SDI.

Using native epiphytic ferns to estimate the atmospheric mercury levels in a small-scale gold mining area of West Java, Indonesia

Terbatas

Mercury pollution is caused by artisanal and small-scale gold mining (ASGM) operations along the Cikaniki River (West Java, Indonesia). The atmosphere is one of the primary media through which mercury can disperse. In this study, atmospheric mercury levels are estimated using the native epiphytic fern Asplenium nidus complex (A. nidus) as a biomonitor; these estimates shed light on the atmospheric dispersion of mercury released during mining. Samples were collected from 8 sites along the Cikaniki Basin during September–November, 2008 and September–November, 2009. The A. nidus fronds that were attached to tree trunks 1–3 m above the ground were collected and measured for total mercury concentration using cold vapor atomic absorption spectrometry (CVAAS) after acid-digestion. The atmospheric mercury was collected using porous gold collectors, and the concentrations were determined using double-amalgam CVAAS. The highest atmospheric mercury concentration, 1.8 × 103 ± 1.6 × 103 ng m−3, was observed at the mining hot spot, and the lowest concentration of mercury, 5.6 ± 2.0 ng m−3, was observed at the remote site from the Cikaniki River in 2009. The mercury concentrations in A. nidus were higher at the mining village (5.4 × 103 ± 1.6 × 103 ng g−1) than at the remote site (70 ± 30 ng g−1). The distribution of mercury in A. nidus was similar to that in the atmosphere; a significant correlation was observed between the mercury concentrations in the air and in A. nidus (r = 0.895, P < 0.001, n = 14). The mercury levels in the atmosphere can be estimated from the mercury concentration in A. nidus using a regression equation: log (HgA.nidu/ng g−1) = 0.740 log (HgAir/ng m−3) − 1.324. Chemosphere, 2012. Volume 89, Issue 3: 241–248

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