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首页> 外文期刊>Applied optics >ELECTROSTATICS ANALYSIS OF RADIATIVE ABSORPTION BY SPHERE CLUSTERS IN THE RAYLEIGH LIMIT - APPLICATION TO SOOT PARTICLES
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ELECTROSTATICS ANALYSIS OF RADIATIVE ABSORPTION BY SPHERE CLUSTERS IN THE RAYLEIGH LIMIT - APPLICATION TO SOOT PARTICLES

机译:瑞利极限中球团的辐射吸收的静电学分析-在烟尘颗粒中的应用。

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摘要

An analysis of radiative absorption and scattering by clusters of spheres in the Rayleigh limit is developed with an electrostatics analysis. This approach assumes that the largest dimension of the cluster is significantly smaller than the wavelength of the radiation. The electric field that is incident upon and scattered by the cluster can then be represented by the gradient of a potential that in turn satisfies Laplace's equation. An analytical solution for the potential that exactly satisfies the boundary conditions at the surfaces of the spheres is obtained with a coupled spherical harmonics method. The components of the polarizability tenser and the absorption, scattering, and depolarization factors are obtained from the solution. Calculations are performed on fractallike clusters of spheres, with refractive-index values that are characteristic of carbonaceous soot in the visible and the IR wavelengths. Results indicate that the absorption cross sections of fractal soot clusters can be significantly larger in the mid-IR wavelengths than what is predicted for Rayleigh-limit spheres that have the same total volume. The absorption cross section (relative to a sphere of the same volume) is dependent on the number of spheres in the aggregate for aggregates with up to approximately 100 primary spheres, and for larger aggregates the relative absorption becomes constant. The predicted spectral variation of soot absorption in the visible and the mid-IR wavelengths is shown to agree well with experimental measurements. [References: 21]
机译:通过静电分析,对瑞利极限范围内的球簇辐射吸收和散射进行了分析。该方法假定簇的最大尺寸显着小于辐射的波长。入射到团簇上并由团簇散射的电场然后可以用电势梯度来表示,该电势又满足拉普拉斯方程。通过耦合球谐函数方法获得了精确满足球体边界条件的势的解析解。可从溶液中获得极化率张量的成分以及吸收,散射和去极化因子。对球形的分形簇进行计算,其折射率值是可见光和IR波长中碳烟尘的特征。结果表明,分形碳黑团簇的吸收截面在中红外波长处可能比总体积相同的瑞利极限球所预测的要大得多。吸收截面(相对于相同体积的球体)取决于聚集体中具有多达大约100个主球体的聚集体中球体的数量,对于较大的聚集体,相对吸收率是恒定的。可见,在可见光和中红外波长的烟尘吸收的预测光谱变化与实验测量非常吻合。 [参考:21]

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