Sedarsky David, Berrocal Edouard, Linne Mark
Department of Physics, Lund University, Lund, Sweden.
Opt Express. 2011 Jan 31;19(3):1866-83. doi: 10.1364/OE.19.001866.
Experimental work in turbid media has shown that trans-illumination images can be significantly improved by limiting light collection to a subset of photons which are minimally distorted by scattering. The literature details numerous schemes (commonly termed ballistic imaging), most often based on time-gating and/or spatially filtering the detected light. However, due to the complex nature of the detected signal, analysis of this optical filtering process has been heretofore limited to qualitative comparisons of image results. In this article we present the implementation of a complete system model for the simulation of light propagation, including both the scattering medium and all stages of the optical train. Validation data from ballistic imaging (BI) measurements of monodisperse scatterers with diameter, d = 0.7 µm, at optical depths 5, 10, and 14, are compared with model results, showing excellent agreement. In addition, the validated model is subsequently applied to a modified time-gated optical system to probe the comparative performance of the BI system used in validation and the modified BI system. This instrument comparison examines scatterers with diameters of 0.7 and 15 µm at optical depths 10 and 14, and highlights the benefits of each system design for these specific scattering conditions. These results show that the modified optics configuration is more suitable for particles which are much larger than the incident wavelength, d >> λ, while the configuration employed in the validation system provides a better contrast for particle diameters on the order of the wavelength, d ~λ, where the scattering process exhibits a more homogeneous phase function. The insights and predictions made available by the full numerical model are important for the design of optimized imaging systems suited to specific turbid media, and make possible the quantitative understanding of both the effects of light propagation in the measurement and the performance of the complete imaging system.
在浑浊介质中的实验工作表明,通过将光收集限制在受散射影响最小的光子子集,可以显著改善透照图像。文献中详细介绍了许多方案(通常称为弹道成像),这些方案大多基于对检测到的光进行时间选通和/或空间滤波。然而,由于检测信号的复杂性,迄今为止,对这种光学滤波过程的分析仅限于对图像结果的定性比较。在本文中,我们展示了一个完整系统模型的实现,用于模拟光传播,包括散射介质和光学系统的所有阶段。将直径d = 0.7 µm的单分散散射体在光学深度为5、10和14时的弹道成像(BI)测量的验证数据与模型结果进行比较,显示出极好的一致性。此外,随后将经过验证的模型应用于一个改进的时间选通光学系统,以探究验证中使用的BI系统和改进后的BI系统的比较性能。这种仪器比较研究了在光学深度为10和14时直径为0.7和15 µm的散射体,并突出了每种系统设计在这些特定散射条件下的优势。这些结果表明,改进后的光学配置更适合于比入射波长大得多的粒子,即d >> λ,而验证系统中采用的配置对于直径与波长相当的粒子,即d ~λ,提供了更好的对比度,此时散射过程表现出更均匀的相位函数。完整数值模型提供的见解和预测对于设计适用于特定浑浊介质的优化成像系统非常重要,并且使得对测量中光传播的影响和完整成像系统的性能进行定量理解成为可能。