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https://saber.ucv.ve/jspui/handle/10872/14484Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Murillo, Miguel | - |
| dc.contributor.author | Carrión, Nereida | - |
| dc.contributor.author | Chirinos, José | - |
| dc.contributor.author | Gammeiro, Alexis | - |
| dc.contributor.author | Fassano, Edmondo | - |
| dc.date.accessioned | 2017-02-16T15:36:25Z | - |
| dc.date.available | 2017-02-16T15:36:25Z | - |
| dc.date.issued | 2001 | - |
| dc.identifier.citation | Talanta 54 (2001) 389–395 | en_US |
| dc.identifier.issn | 0039- 9140 | - |
| dc.identifier.uri | http://hdl.handle.net/10872/14484 | - |
| dc.description.abstract | A 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.iso | en | en_US |
| dc.publisher | Atlanta | en_US |
| dc.subject | Microwave Plasma MIP | en_US |
| dc.subject | Surfatron | en_US |
| dc.subject | Mercury determination | en_US |
| dc.title | Optimization of experimental parameters for the determination of mercury by MIP:AES | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | Artículos Publicados | |
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