首页> 外文会议>Twenty-Ninth International Symposium on Combustion Hokkaido University >SPATIALLY RESOLVED SMALL-ANGLE X-RAY SCATTERING STUDIES OF SOOT INCEPTION AND GROWTH
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SPATIALLY RESOLVED SMALL-ANGLE X-RAY SCATTERING STUDIES OF SOOT INCEPTION AND GROWTH

机译:烟尘吸收和生长的空间分辨小角度X射线散射研究

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The high spectral brilliance of x-rays produced at the Basic Energy Sciences Synchrotron Radiation Center of Argonne's Advanced Photon Source allows us to perform small-angle x-ray scattering (SAXS) measurements of the distributions of soot particles in flames. SAXS provides an in situ probe of the size and distribution of particles in the region between 1 and 100 nm. Detailed measurements on a propylene/ air diffusion flame allow us to extract a spatially dependent background, which occurs in gas-phase combustion systems, and to perform Abel inversions, which provide the radial dependence of the scattering intensity. A bimodal distribution of soot particles is needed to describe our results. The radial behavior of the two modes of this distribution implies that the chemistry and fluid dynamics are strongly coupled in this simple diffusion flame. The larger particles of this distribution correspond to the previously observed primary particles, which have a relatively complex radial dependence. Midway between the fuel source and the widest part of the flame, the primary particles have a mean radius of 6 nm or less and their concentration is symmetrically distributed about the flame front. At the widest part of the flame, two distinct distributions of primary particles are observed. Near the center of the flame, the particles have a mean radius of 10 nm and a polydispersity of 0.3 and beyond a transition region they have a mean radius of 21 nm and a polydispersity of 0.2. The smaller particles, which require additional experiments before they can be identified, correspond to soot nuclei, polycyclic aromatic hydrocarbon species such as naphthalene, and/or disordered carbons with graphitic basal planes.
机译:在Argonne先进光子源的基础能源科学同步加速器辐射中心产生的X射线高光谱亮度,使我们能够对火焰中烟尘颗粒的分布进行小角度X射线散射(SAXS)测量。 SAXS提供了一个在1到100 nm之间区域的颗粒大小和分布的原位探针。对丙烯/空气扩散火焰的详细测量使我们能够提取在气相燃烧系统中发生的与空间相关的背景,并进行阿贝尔反演,从而提供了散射强度的径向相关性。需要烟灰颗粒的双峰分布来描述我们的结果。两种分布模式的径向行为表明,在这种简单的扩散火焰中,化学反应和流体动力学密切相关。该分布的较大颗粒对应于先前观察到的初级颗粒,其具有相对复杂的径向依赖性。在燃料源和火焰的最宽部分之间的中间,一次粒子的平均半径为6 nm或更小,并且它们的浓度围绕火焰前沿对称分布。在火焰的最宽处,观察到两种不同的一次颗粒分布。在火焰中心附近,粒子的平均半径为10 nm,多分散度为0.3,在过渡区域之外,粒子的平均半径为21 nm,多分散度为0.2。较小的颗粒需要进一步的实验才能确定,这些颗粒对应于烟灰核,多环芳烃物种(如萘)和/或具有石墨基面的无序碳。

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