首页> 外文会议>Conference on Targets and Backgrounds VI: Characterization, Visualization, and the Detection Process 24-26 April 2000 Orlando, USA >Effects of multiple scattering and thermal emission on targetbackground signatures sensed through obscuring atmospheres
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Effects of multiple scattering and thermal emission on targetbackground signatures sensed through obscuring atmospheres

机译:多重散射和热辐射对通过遮蔽气氛感知的目标背景特征的影响

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We report on the application of a recently developed method for producing exact solutions of the thermal version of the radiative transfer equation~1. The method is demonstrated to be accurate to within five significant figures when compared with the one dimensional plane layer solutions published by van de Hulst~2; and, has the added capability for treating discrete, localized, aerosol clouds of spherical and cylindrical symmetry. The method, described in detail in a companion paper~1, is only briefly summarized here, where our main purpose is to demonstrate the utility of the method for calculating emissivity functions of finite aerosol clouds of arbitrary optical thickness and albedo, and most likely to occur on the modern "cluttered" battlefield. The emissivity functions are then used to determine apparent temperatures including effects of both internal thermal emission and in-scatter from the ambient surroundings. We apply the results to four generic scenarios including the mid and far IR and a hypothetical "full spectrum" band. In all cases, calculations show that errors on the order of several degrees in the sensed temperature can occur if cloud emissivity is not accounted for, with errors being most pronounced at the higher values of optical depth and albedo. We also demonstrate that significant discrepancies can occur when comparing results from different spectral bands, especially for the mid IR which consistently shows higher apparent temperatures than the other bands, including the full spectrum case. Results of emissivity calculations show that in almost no case can one justify the simple Beer's Law model that essentially ignores emissive/scattering effects; however, there is reason for optimism in the use of other simplyfing first and higher order approximations used in some contemporary models. The present version of the model treats only Gaussian aerosol distributions and isotropic scattering; although neither assumption necessarily represents a restriction on the method.
机译:我们报告了最近开发的方法在产生辐射传递方程〜1的热形式的精确解中的应用。与van de Hulst〜2发表的一维平面层解决方案相比,该方法被证明在5个有效数字内准确。并且具有处理球形和圆柱形对称的离散局部气雾的附加功能。此方法仅在随附论文〜1中进行了详细介绍,此处仅作简要概述,其主要目的是演示该方法在计算任意光学厚度和反照率的有限气溶胶云的发射率函数中的实用性,并且最有可能发生在现代的“杂乱无章”的战场上。然后,使用发射率函数确定视在温度,包括内部热辐射的影响以及来自周围环境的散射。我们将结果应用于四个通用场景,包括中红外和远红外以及假设的“全频谱”频段。在所有情况下,计算表明,如果不考虑云的发射率,则可能会在感测到的温度上出现几度的误差,在较高的光学深度和反照率下,误差最为明显。我们还证明,当比较不同光谱带的结果时,尤其是对于中红外光谱(与全光谱情况相比,其他光谱带始终显示更高的表观温度)的结果,可能会出现重大差异。发射率计算结果表明,在几乎任何情况下都无法证明简单的比尔定律模型是合理的,该模型基本上忽略了发射/散射效应。但是,在某些现代模型中使用其他简单的一阶和高阶近似有理由感到乐观。该模型的当前版本仅处理高斯气溶胶分布和各向同性散射。尽管两种假设都不一定代表对该方法的限制。

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