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离散和离散非均匀随机介质电磁散射的第一性原理建模

First-principles modeling of electromagnetic scattering by discrete and discretely heterogeneous random media.

作者信息

Mishchenko Michael I, Dlugach Janna M, Yurkin Maxim A, Bi Lei, Cairns Brian, Liu Li, Panetta R Lee, Travis Larry D, Yang Ping, Zakharova Nadezhda T

机构信息

NASA Goddard Institute for Space Studies, 2880 Broadway, New York, NY 10025, USA.

Main Astronomical Observatory of the National Academy of Sciences of Ukraine, 27 Zabolotny Str., 03680, Kyiv, Ukraine.

出版信息

Phys Rep. 2016 May 16;632:1-75. doi: 10.1016/j.physrep.2016.04.002. Epub 2016 Apr 12.

DOI:10.1016/j.physrep.2016.04.002
PMID:29657355
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC5896873/
Abstract

A discrete random medium is an object in the form of a finite volume of a vacuum or a homogeneous material medium filled with quasi-randomly and quasi-uniformly distributed discrete macroscopic impurities called small particles. Such objects are ubiquitous in natural and artificial environments. They are often characterized by analyzing theoretically the results of laboratory, , or remote-sensing measurements of the scattering of light and other electromagnetic radiation. Electromagnetic scattering and absorption by particles can also affect the energy budget of a discrete random medium and hence various ambient physical and chemical processes. In either case electromagnetic scattering must be modeled in terms of appropriate optical observables, i.e., quadratic or bilinear forms in the field that quantify the reading of a relevant optical instrument or the electromagnetic energy budget. It is generally believed that time-harmonic Maxwell's equations can accurately describe elastic electromagnetic scattering by macroscopic particulate media that change in time much more slowly than the incident electromagnetic field. However, direct solutions of these equations for discrete random media had been impracticable until quite recently. This has led to a widespread use of various phenomenological approaches in situations when their very applicability can be questioned. Recently, however, a new branch of physical optics has emerged wherein electromagnetic scattering by discrete and discretely heterogeneous random media is modeled directly by using analytical or numerically exact computer solutions of the Maxwell equations. Therefore, the main objective of this Report is to formulate the general theoretical framework of electromagnetic scattering by discrete random media rooted in the Maxwell-Lorentz electromagnetics and discuss its immediate analytical and numerical consequences. Starting from the microscopic Maxwell-Lorentz equations, we trace the development of the first-principles formalism enabling accurate calculations of monochromatic and quasi-monochromatic scattering by static and randomly varying multiparticle groups. We illustrate how this general framework can be coupled with state-of-the-art computer solvers of the Maxwell equations and applied to direct modeling of electromagnetic scattering by representative random multi-particle groups with arbitrary packing densities. This first-principles modeling yields general physical insights unavailable with phenomenological approaches. We discuss how the first-order-scattering approximation, the radiative transfer theory, and the theory of weak localization of electromagnetic waves can be derived as immediate corollaries of the Maxwell equations for very specific and well-defined kinds of particulate medium. These recent developments confirm the mesoscopic origin of the radiative transfer, weak localization, and effective-medium regimes and help evaluate the numerical accuracy of widely used approximate modeling methodologies.

摘要

离散随机介质是一种物体,其形式为有限体积的真空或充满被称为小颗粒的准随机且准均匀分布的离散宏观杂质的均匀物质介质。这类物体在自然和人工环境中无处不在。它们通常通过从理论上分析光和其他电磁辐射散射的实验室测量、现场测量或遥感测量结果来表征。粒子的电磁散射和吸收也会影响离散随机介质的能量收支,进而影响各种周围的物理和化学过程。在任何一种情况下,电磁散射都必须根据适当的光学可观测量来建模,即场中的二次或双线性形式,这些形式量化了相关光学仪器的读数或电磁能量收支。一般认为,时谐麦克斯韦方程组能够准确描述宏观颗粒介质的弹性电磁散射,这种介质随时间的变化比入射电磁场慢得多。然而直到最近,对于离散随机介质直接求解这些方程都是不切实际的。这导致在其适用性可能受到质疑的情况下,各种唯象方法被广泛使用。然而,最近出现了物理光学的一个新分支,其中离散和离散非均匀随机介质的电磁散射直接通过使用麦克斯韦方程组的解析或数值精确计算机解来建模。因此,本报告的主要目的是构建基于麦克斯韦 - 洛伦兹电磁学的离散随机介质电磁散射的一般理论框架,并讨论其直接的解析和数值结果。从微观麦克斯韦 - 洛伦兹方程组出发,我们追溯第一性原理形式体系的发展,该体系能够精确计算静态和随机变化的多粒子群的单色和准单色散射。我们说明了这个一般框架如何与麦克斯韦方程组的最新计算机求解器相结合,并应用于对具有任意堆积密度的代表性随机多粒子群的电磁散射进行直接建模。这种第一性原理建模产生了唯象方法无法获得的一般物理见解。我们讨论了一阶散射近似、辐射传输理论以及电磁波的弱局域化理论如何能够作为麦克斯韦方程组对于非常特殊且定义明确的颗粒介质类型的直接推论而导出。这些最新进展证实了辐射传输、弱局域化和有效介质 regime 的介观起源,并有助于评估广泛使用的近似建模方法的数值精度。