Abstract
AbstractWe consider scattering of electromagnetic waves by a finite discrete random medium composed of spherical particles. The size of the random medium can range from microscopic sizes of a few wavelengths to macroscopic sizes approaching infinity. The size of the particles is assumed to be of the order of the wavelength. We extend the numerical Monte Carlo method of radiative transfer and coherent backscattering (RT‐CB) to the case of dense packing of particles. We adopt the ensemble‐averaged first‐order incoherent extinction, scattering, and absorption characteristics of a volume element of particles as input for the RT‐CB. The volume element must be larger than the wavelength but smaller than the mean‐free path length of incoherent extinction. In the radiative transfer part, at each absorption and scattering process, we account for absorption with the help of the single‐scattering albedo and peel off the Stokes parameters of radiation emerging from the medium in predefined scattering angles. We then generate a new scattering direction using the joint probability density for the local polar and azimuthal scattering angles. In the coherent backscattering part, we utilize amplitude scattering matrices along the radiative‐transfer path and the reciprocal path and utilize the reciprocity of electromagnetic waves to verify the computation. We illustrate the incoherent volume element scattering characteristics and compare the dense‐medium RT‐CB to asymptotically exact results computed using the Superposition T‐matrix method (STMM). We show that the dense‐medium RT‐CB compares favorably to the STMM for the current cases of sparse and dense discrete random media studied.
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