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首页> 外文期刊>Experimental Thermal and Fluid Science: International Journal of Experimental Heat Transfer, Thermodynamics, and Fluid Mechanics >An experimental study on the spectral dependence of light extinction in sooting ethylene counterflow diffusion flames
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An experimental study on the spectral dependence of light extinction in sooting ethylene counterflow diffusion flames

机译:烟灰乙烯反流扩散火焰光消隐光谱依赖性的实验研究

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A light extinction technique is widely-adopted for quantitative measurement of soot volume fractions. The measurement accuracy is dependent on the optical properties of soot, which are expected to vary with the wavelength of incident light and the physicochemical environments in which soot is formed. In the present study, a diode laser-based light extinction setup, capable of providing light with variable wavelengths ranging from 405 to 1064 nm, was utilized to investigate the in-situ spectral dependence of light absorption for soot formed in counterflow diffusion flames. Soot volume fractions (F-v ) were inferred from the extinction level of these laser beams for a series of flames parameterized by oxygen/fuel mole fractions, nozzle exit velocities, and fuel types. Special attention was given to distinguish between the soot formation (SF) and soot formation/ oxidation (SFO) flames, considering their notable differences in soot evolutions. It was found that the inferred F-v as measured with visible light (405-670 nm) was always significantly higher than those measured with near - infrared light ( 780 nm). In addition, the quantitative decrease of F-v with the increase in light wavelength (lambda) was found to be different for soot particles formed at different flame locations and/or flame conditions, even in the spectral range above 780 nm for which polycyclic aromatic hydrocarbon (PAH) interferences are expected to be minimal. This confirms the wavelength dependence of the soot optical property E(m). In particular, the value of E(m) tends to decrease with increasing wavelength and the rate of decrease is lower for more mature soot particles. Furthermore, by fitting the extinction coefficient with wavelength in the near-infrared range, the quantitative relation of E(m) with lambda was derived and compared among various flame conditions. The present study demonstrates that soot formed at different conditions have different optical properties. The results are als
机译:广泛采用光消光技术,用于烟灰体积分数的定量测量。测量精度取决于烟灰的光学性质,这预计将随着入射光的波长和形成烟灰的物理化学环境而变化。在本研究中,利用了一种基于二极管激光的光消光设置,其能够提供具有405至1064nm的可变波长的光,以研究光吸收在反流扩散火焰中形成的光吸收的原位谱依赖性。从这些激光束的消光水平推断出通过氧/燃料摩尔分数,喷嘴出口速度和燃料类型参数的一系列火焰的消光水平推断出烟灰体积分数(F-V)。考虑到烟灰演变中的显着差异,特别注意区分烟灰地层(SF)和烟灰形成/氧化(SFO)火焰。发现具有可见光(405-670nm)测量的推断的F-V始终明显高于近红外光(& 780nm)测量的F-V。此外,发现在不同火焰位置和/或火焰条件下形成的烟雾颗粒的光波长(Lambda)的增加的定量降低是不同的,即使在780nm以上的多环芳烃( PAH)干扰预计将是最小的。这证实了烟灰光学特性E(M)的波长依赖性。特别地,E(m)的值趋于随着波长的增加而降低,并且对于更成熟的烟灰颗粒,降低的速率较低。此外,通过在近红外范围内与波长的消光系数拟合,通过各种火焰条件衍生并比较e(m)与λ与λ的定量关系。本研究表明,在不同条件下形成的烟灰具有不同的光学性质。结果是als

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