Please use this identifier to cite or link to this item: https://saber.ucv.ve/jspui/handle/10872/14484
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dc.contributor.authorMurillo, Miguel-
dc.contributor.authorCarrión, Nereida-
dc.contributor.authorChirinos, José-
dc.contributor.authorGammeiro, Alexis-
dc.contributor.authorFassano, Edmondo-
dc.date.accessioned2017-02-16T15:36:25Z-
dc.date.available2017-02-16T15:36:25Z-
dc.date.issued2001-
dc.identifier.citationTalanta 54 (2001) 389–395en_US
dc.identifier.issn0039- 9140-
dc.identifier.urihttp://hdl.handle.net/10872/14484-
dc.description.abstractA system using a microwave induced plasma, as an emission source was optimized for total mercury determinations. The system contains a flow injection section in which mercury is reduced and deposited on a gold:platinum collector, and carried to the emission source. The microwave was generated in a Surfatron cavity. An experimental design was applied to optimize parameters concerning plasma conditions, amalgamation, desorption and mercury vapor generation. The limit of detection of the method was 14 pg ml 1 of mercury, using peak area mode while LDs was 1.3 pg ml 1 using peak height mode, with a 2% RSD and a linear dynamic range of almost three orders of magnitude. The accuracy was assessed using a certified reference material of atmospheric particulate National Institute of Standards and Technology (NIST) 2704. No significant difference at 95% confidence level was observed between the certified value and our results.en_US
dc.language.isoenen_US
dc.publisherAtlantaen_US
dc.subjectMicrowave Plasma MIPen_US
dc.subjectSurfatronen_US
dc.subjectMercury determinationen_US
dc.titleOptimization of experimental parameters for the determination of mercury by MIP:AESen_US
dc.typeArticleen_US
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