Removal mechanism of elemental mercury by using non-thermal plasma
► The removal mechanism of the elemental mercury (Hg 0) has been investigated within the atmosphere of non-thermal plasma. ► A sudden increase in the removal efficiency is observed after several minutes of the reaction time. ► The formation of HgO 3(s) species deposited on the reactor surface accele...
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Veröffentlicht in: | Chemosphere (Oxford) 2011-03, Vol.83 (1), p.69-75 |
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Sprache: | eng |
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Zusammenfassung: | ► The removal mechanism of the elemental mercury (Hg
0) has been investigated within the atmosphere of non-thermal plasma. ► A sudden increase in the removal efficiency is observed after several minutes of the reaction time. ► The formation of HgO
3(s) species deposited on the reactor surface accelerates the removal rate of Hg
0.
The removal mechanism of elementary mercury (Hg
0) by non-thermal plasma (NTP) has been investigated, where dielectric barrier discharge and O
3 injection methods as oxidation techniques are employed, together with the analysis of mercury species deposited on the reactor surface using temperature-programmed desorption and dissociation (TPDD) and scanning electron microscopy–energy dispersive spectroscopy. The removal of Hg
0 by NTP is found to be time-dependent and proceed through three domains; the Hg
0 concentration just slightly decreases as soon as NTP is initiated and then becomes constant for several minutes (Region 1), thereafter starts to decrease rapidly for 1
h (Region 2) and, after passing fall-off region, very slowly decreases for about 4
h (Region 3). The deposited mercury species on the reactor surface were conglomerated like islands, rather than dispersed uniformly, and their ratio of Hg
0 to O composition is observed to be 1:2. Additionally, the new peak in TPDD spectra observed in the region of 260–380
°C is proposed as HgO
3. These results lead us to conclude that the deposited mercury species by NTP have extra O atoms to oxidize the adsorbed Hg
0, resulting in the acceleration of removal rate as the oxidation of Hg
0 proceeds. |
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ISSN: | 0045-6535 1879-1298 |
DOI: | 10.1016/j.chemosphere.2010.12.003 |