2014
DOI: 10.1016/j.ecss.2014.09.016
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Natural causes of changes in marine environment: Mercury speciation and distribution in anchialine caves

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Cited by 11 publications
(4 citation statements)
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“…Relatively few studies have attempted to record the full diversity of microbial communities in anchialine ecosystems [13][14][15], even though these studies resulted in descriptions of new species using novel molecular tools. In the region of the eastern Adriatic Sea, the majority of anchialine ecological studies have been based on the taxonomic research of stygobiotic metazoans [16], the distribution of trace metals [17], and iodine species and nutrients [18]. Technical difficulties in sampling anchialine ecosystems limit the ability to study microbial communities.…”
Section: Introductionmentioning
confidence: 99%
“…Relatively few studies have attempted to record the full diversity of microbial communities in anchialine ecosystems [13][14][15], even though these studies resulted in descriptions of new species using novel molecular tools. In the region of the eastern Adriatic Sea, the majority of anchialine ecological studies have been based on the taxonomic research of stygobiotic metazoans [16], the distribution of trace metals [17], and iodine species and nutrients [18]. Technical difficulties in sampling anchialine ecosystems limit the ability to study microbial communities.…”
Section: Introductionmentioning
confidence: 99%
“…Classical and genomic-taxonomic descriptions have further cataloged the macro and microbiota inhabiting the anchialine environment (Yager, 1987(Yager, , 1994Alcocer et al, 1999;Seymour et al, 2007;Martinez-García et al, 2009;Humphreys et al, 2012;Hoenemann et al, 2013). Geochemical and stable isotope-based studies have described the carbon cycle (Pohlman et al, 1997), nutrient dynamics (Moore, 1999), iodine speciation (Žic et al, 2008), trace metal cycles (Cuculić et al, 2011;Kwokal et al, 2014) and the general (Iliffe,Fig. 1.…”
mentioning
confidence: 99%
“…Mercury produced by coal combustion mainly exists in three forms: zero-valent element mercury (Hg 0 ), divalent mercury (Hg 2+ ), and particulate-bound mercury (Hg p ). We can use a wet flue gas desulfurization (WFGD) system to remove divalent mercury effectively, and dust collectors such as an electrostatic precipitator (ESP) or a bag filter (FF) can be used to capture particulate-bound mercury . However, zero-valent mercury is extremely difficult to remove and can exist in the atmosphere for 1–2 years.…”
Section: Introductionmentioning
confidence: 99%