首页> 外文会议>Atmospheric Propagation and Remote Sensing II >Depth mode characteristics of light propagation in real turbid media
【24h】

Depth mode characteristics of light propagation in real turbid media

机译:真实浑浊介质中光传播的深度模式特性

获取原文
获取原文并翻译 | 示例

摘要

Abstract: A study, performed outside the framework of the Fokker-Planck approximation, is presented of the depth mode of light propagation in turbid media with slowly decreasing scattering phase function X($gamma@), when the scattering probability decreases more slowly, than $gamma$+$MIN@4$/, as the single scattering angle $gamma is enhanced. Postulating the approximate shape of the angular spectrum in the depth mode, we propose and realize a regular procedure for optimum determination of the parameters of this spectrum. The dispersion in the depth mode and the depth damping coefficient are found analytically. The obtained results are in good agreement with the results of numerical calculations and transform, in the limit, into known results of the diffusion approximation. !8
机译:摘要:在Fokker-Planck近似框架之外进行的一项研究提出了当散射概率降低的速度慢于散射相位函数X($ gamma @)的浊介质中光传播的深度模式。 $ gamma $ + $ MIN @ 4 $ /,因为单个散射角$ gamma增强了。假设在深度模式下角谱的近似形状,我们提出并实现了用于最佳确定该谱的参数的常规程序。通过分析发现了深度模式下的色散和深度阻尼系数。所获得的结果与数值计算的结果非常吻合,并在一定程度上转换为扩散近似的已知结果。 !8

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号