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Mercury Interaction with the Fine Fraction of Coal-Combustion Fly Ash in a Simulated Coal Power Plant Flue Gas Stream

机译:汞与模拟燃煤电厂烟气中燃煤粉煤灰的精细相互作用

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摘要

Mercury associated with fly ash is a significant contaminant released in flue gas emissions from coal-fixed power plants. This work focuses on the association of Hg with other elements and phases as well as the molecular-level speciation of Hg in bulk and <0.1 mu m sized fly ash particles reacted with a Hg-containing simulated flue gas stream. Following reaction under conditions chosen to simulate an electrostatic precipitator operating at 140 degrees C, fly ash (bulk and <= 0.1 mu m) from a Kentucky power plant was analyzed using microscopic and spectroscopic techniques. The <= 0.1 mu m fraction dominates Hg uptake, with total Hg concentrations increasing from 100 ppb to 610 ppm after reaction, whereas bulk ash concentrations increase from 11 to 164 ppb. Synchrotron-based micro-X-ray fluorescence mapping of the reacted <= 0.1 mu m fraction showed that Hg is present in two major regions: Fe-rich areas and Hg hot spots not associated with Fe. X-ray absorption spectroscopic analysis revealed that Hg is associated with Br and Cl, is bound to iron oxides, and occurs as HgS (cinnabar). Fourier transform infrared (FTIR) spectroscopic analysis of the fine fraction revealed carboxylic, alcoholic, and alkane functional groups. Density functional theory simulation of the vibrational frequencies of a carboxylic group bonded to Hg reproduced the same frequency shifts and peak intensity reductions (relative to carboxylic acid alone) observed in the experimental FTIR spectrum of the Hg-reacted fly ash fine fraction, suggesting Hg(II) binding to organic matter. Our results reveal complex interactions between Hg and coal fly ash in the combustion stream that produces less bioavailable forms of Hg than He present in the unreacted flue gas. Such information is critical for safe disposal of Hg-containing fly ash in landfills or use in cementitious products.
机译:与粉煤灰相关的汞是燃煤电厂发烟气中释放的重要污染物。这项工作的重点是汞与其他元素和相的缔合,以及大块汞和<0.1微米大小的粉煤灰颗粒与含汞模拟烟道气反应的汞分子形态。在为模拟在140摄氏度下运行的静电除尘器所选择的条件下进行反应后,使用显微镜和光谱技术分析了肯塔基州一家发电厂的粉煤灰(散装且≤0.1微米)。 ≤0.1微米的部分占主要的Hg吸收,反应后总Hg浓度从100 ppb增加到610 ppm,而总灰分浓度从11 ppb增加到164 ppb。反应后的<= 0.1μm馏分的基于同步加速器的微X射线荧光图谱显示,汞存在于两个主要区域:富铁区域和与铁无关的汞热点。 X射线吸收光谱分析表明,Hg与Br和Cl缔合,与氧化铁结合,并以HgS(朱砂)形式存在。细级分的傅里叶变换红外(FTIR)光谱分析显示了羧基,醇基和烷烃官能团。结合Hg的羧基的振动频率的密度泛函理论模拟在Hg反应的粉煤灰细小颗粒的实验FTIR光谱中观察到了相同的频移和峰强度降低(仅相对于羧酸),表明Hg( II)与有机物结合。我们的研究结果表明,燃烧流中的汞与粉煤灰之间存在复杂的相互作用,与未反应烟道气中的He相比,产生的Hg生物利用形式较少。此类信息对于安全处置垃圾填埋场中的汞或水泥产品中的使用至关重要。

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  • 来源
    《Energy & fuels》 |2015年第sepaaocta期|6025-6038|共14页
  • 作者单位

    Stanford Univ, Sch Earth Energy & Environm Sci, Dept Geol Sci, Stanford, CA 94305 USA|Stanford Univ, Sch Earth Energy & Environm Sci, Dept Energy Resources Engn, Stanford, CA 94305 USA;

    Stanford Univ, Sch Earth Energy & Environm Sci, Dept Energy Resources Engn, Stanford, CA 94305 USA;

    Stanford Univ, Sch Earth Energy & Environm Sci, Dept Energy Resources Engn, Stanford, CA 94305 USA;

    Stanford Univ, Sch Earth Energy & Environm Sci, Dept Energy Resources Engn, Stanford, CA 94305 USA;

    Stanford Univ, Sch Earth Energy & Environm Sci, Dept Geol Sci, Stanford, CA 94305 USA;

    Stanford Univ, Sch Earth Energy & Environm Sci, Dept Energy Resources Engn, Stanford, CA 94305 USA;

    Univ Kentucky, Ctr Appl Energy Res, Lexington, KY 40511 USA;

    Stanford Univ, Sch Earth Energy & Environm Sci, Dept Geol Sci, Stanford, CA 94305 USA|Stanford Univ, Dept Chem Engn, Stanford, CA 94305 USA|SLAC Natl Accelerator Lab, Dept Photon Sci & Stanford Synchrotron Radiat Lig, Menlo Pk, CA 94025 USA;

    Stanford Univ, Sch Earth Energy & Environm Sci, Dept Energy Resources Engn, Stanford, CA 94305 USA;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);美国《生物学医学文摘》(MEDLINE);
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  • 正文语种 eng
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