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Comparison of in situ measurements and Rayleigh-Debye-Gans theory for optical properties of flame generated monodispersive soot particles

机译:对原位测量和Rayleigh-deby-GANS理论的比较火焰产生的单双管煤颗粒光学性质

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Soot particles, formed as a result of incomplete fuel combustion, have been an active subject of research for decades for the scientists and researchers from all walks of life. This is primarily because of the challenge which soot's complex formation mechanism and its structure throws to the researchers thereby making the task arduous for studying its optical and physical properties. The knowledge of optical and physical properties is essential in a number of areas such as environmental applications involving visibility and radiation transfer and for optical diagnostics of aerosols and colloids. When it comes to our earth's atmosphere, carbonaceous aerosols stand out as the single most dominant particles residing in the troposphere.Quantifying the optical properties of soot particles using conventional electromagnetic theory has always been a great challenge mainly because of their complex particle morphology. Soot particles formation by combustion is a complex process, and there is a large body of literature on the subject. The combustion fuel first undergoes pyrolysis, a process of thermal degradation and cracking of complex fuel molecules, which produces lowmolecular weight radicals. PAHs are formed subsequently by a series of radical reactions with soot precursors such as acetylene radicals. Further reactions with small precursor molecules result in the growth of the PAH structures until they become large enough to serve as particle nuclei. The high temperature of the flame causes most of the hydrogens to be stripped away, leaving small spherules with a high carbon-to hydrogen ratio. These spherules, under the unavoidable influence of Brownian motion, coagulate to form aggregate particles. The individual spherules that form these aggregate particles are generally small compared to the wavelength of light so that they satisfy the Rayleigh limit of the Lorentz-Mie Scattering theory. Optical cross sections of these complex shaped aggregates cannot be treated adequately by relatively simple electromagnetic theories for spheres or cylinders. Hence, to solve for the optical cross sections of these aggregates using conventional electromagnetic theory, one has to rely on intensive computational capabilities and power, which often yields little insight in terms of one's physical understanding of the problem. In recent years however, thanks to the introduction of the concept of Fractal geometry, a simple formulation known as the Rayleigh-Debye-Gans (RDG) approximation has received much attention and recognition for providing a simple andaccurate solution to the calculation of the optical scattering and absorption by aggregates. Experimental tests of RDG scattering and absorption coefficients of aggregates have been indirect. In this paper, we provide preliminary results obtained from comparison of RDG scattering and absorption coefficients with experimental scattering and absorption coefficients. The aerosol sample used in our case was flame generated soot.
机译:烟尘颗粒,形成不完全的燃料燃烧的结果,一直是活跃的研究课题数十年的科学家和研究人员来自各行各业。这主要是黑烟复杂的形成机制及其结构罚球研究人员从而使艰苦的研究其光学和物理性质任务的挑战,因为。光学和物理特性的知识是在许多领域必要如涉及可视性和辐射传输环境的应用程序和用于气溶胶和胶体的光学诊断。当涉及到我们的地球大气,碳气溶胶脱颖而出,成为居住在troposphere.Quantifying使用传统的电磁理论的烟尘颗粒的光学特性的最主导的颗粒一直因为其复杂的颗粒形态的一个巨大的挑战为主。煤烟颗粒形成由燃烧是一个复杂的过程,并且有大量文献的被摄对象。燃烧燃料首先经历热解,热降解的过程和复杂的燃料分子的裂解,从而产生低分子量的基团。多环芳烃是由一系列与烟灰前体如乙炔基团的自由基反应的随后形成的。小的前体分子进一步反应导致PAH结构的生长,直到它们变得足够大以用作颗粒核。火焰的高温使大部分氢被剥离掉,使小球体小具有高的碳 - 氢比例。这些小球,布朗运动的不可避免的影响下,凝结形成的聚集体颗粒。相比的光,从而波长使它们满足洛伦兹Mie散射理论的限制瑞利形成这些聚集体颗粒的球粒个体通常很小。这些复杂形状的聚集体的光学截面不能被用于球形或圆柱形相对简单的电磁理论充分治疗。因此,解决使用传统的电磁理论,这些聚集体的光学截面,一个必须依靠密集的计算能力和权力,这往往产生于这个问题的人的身体的理解方面很少见地。然而,在近年来,由于引入分形几何,被称为瑞利 - 德拜 - 甘斯(RDG)近似的简单制剂的概念的已受到很大关注,并识别用于向所述光学散射的计算提供了一种简单andaccurate溶液和由聚集体的吸收。聚集的RDG散射和吸收系数的实验测试是间接的。在本文中,我们提供了从与实验散射和吸收系数RDG散射和吸收系数的比较中获得的初步结果。在我们的例子中使用的气溶胶样品的火焰产生的烟灰。

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