基于远场模式的散射体形状成像

对线性抽样法的电磁场逆散射求解进行了研究。为避免迭代和优化法的正问题求解，用积分算子将散射物边界数据映射到散射场的远场模式，针对第一类积分方程的不适定性，用Tikhonov正则化法求解，并用高阶收敛算法确定正则化参数以快速数值实现。数值计算结果表明：线性抽样法＋确定正则化参数的高阶收敛算法可较好地滤除噪声，减少了确定正则化参数的计算量。     

Comment: On the different approaches of Rayleigh optical depth determination

Srivastava et al. (2009) presented Rayleigh scattering cross-sections and optical depths for Earth’s atmosphere that are approximately 3% smaller than previously accepted. Their analysis was based on quantum-mechanical theory for anisotropic scattering in the Cabannes line published in papers that seem to have introduced some confusion about determining the anisotropy and King factors. This comment clarifies these factors and shows that including the frequency-shifted rotational Raman lines gives the traditional King factor and the correct Rayleigh scattering for the optical depth.     

基于空域滤波的二维全极化散射中心快速提取

在全极化逆合成孔径雷达(ISAR)体制下,二维相干极化几何绕射(CP-GTD)模型能够精确描述雷达目标高频电磁极化散射特性。针对CP-GTD模型,提出了一种基于空域滤波的二维全极化散射中心参数快速提取方法。该方法利用空域滤波将二维全极化散射中心参数提取问题分解为多个一维全极化散射中心提取问题,进而利用一维旋转不变技术(1D-ESPRIT)分步对全极化散射中心各维参数进行联合估计,最后利用最小二乘方法获得相干极化散射矩阵的估计。此外,采用这样的分步估计过程,可以实现二维参数的自动配对。复杂度分析和仿真实验表明:该方法不仅能够显著降低运算量,并且还能获得较好的估计精度,可以有效地用于目标全极化散射中心提取。     

银纳米结构的电化学制备及表面增强拉曼效应

利用电化学沉积的方法在氧化铟锡(ITO,Indium Tin Oxide)导电玻璃表面成功地制备出了形貌均一的银纳米结构.所制备银纳米结构的形貌和密度与前驱体AgNO₃的浓度、沉晶种电位、生长电位以及柠檬酸钠的加入均有着重要的关系,只有合理地设置这些参数才能制得形貌和密度均较为理想的银纳米粒子.此外以对巯基苯胺(p-ATP,p-aminothiophenol)为探针分子,在633 nm的激光激发下对银纳米结构进行了表面增强拉曼效应(SERS,Surface Enhanced Raman Scattering)的研究,结果表明其在SERS领域有着潜在的应用价值.     

改进的极化SAR图像三分量分解方法

针对原始三分量分解方法中,偶次散射和表面散射类地物的体散射分量可能会过估计的问题,提出了一种基于H/α珔参数和一般散射机理模型的改进的三分量分解方法。首先在进行极化分解之前利用H/α珔参数判定目标的主导散射类型。对于主导散射类型明确的像素点,利用一般散射机理模型优先计算主导散射成分的相关扩展系数,然后再从剩余成分中提取非主导散射分量。对于主导散射类型不明确的像素点,采用传统的去取向三分量分解方法进行分解。对实测极化SAR图像进行实验表明,新方法不仅继承了传统三分量分解方法的优点,而且能在分解结果中更加有效地突出雷达目标的主导散射特征。     

Studies on the imaging characteristics of Yohkoh Soft X-ray Telescope: Optical aberration and scattering

In order to better understand the characteristics of Yohkoh Soft X-ray Telescope (SXT) mirror, we have analyzed the in-flight overexposed image (the starburst image) obtained during the solar flare observation. It has been revealed from our study that the intensity distribution inside the shadows shown in the scattering difference image contains little of the scattered component of the PSF and matches almost correctly the extension of the PSF core profile. Also it is found that the scattering wing of the SXT PSF is connected smoothly to the PSF core within the distance of about 100–200 arcsec from the peak. With numerical simulations we have shown that an increase in energy affects not only the level of scattering wing, but also both the shape and the absolute level of the PSF core. The results have revealed, however, that the energy dependence for the SXT PSF cannot be easily estimated with the data obtained from one filter alone, which implies that the data analysis using multiple filters will enable us to determine the absolute amount of scattered component as well as the energy dependence of the SXT PSF. Details on the analysis of starburst image and the results from numerical simulations will be introduced and discussed thoroughly.     

应用粒子激光散射测量混合反应器分散相浓度场分布

研究了圆管反应器中四束侧向对撞射流与轴向流形成的混合流动.应用激光粒子散射成像测量了侧向分散相在混合流中的浓度场分布,得到了不同的浓度分布图形随侧向流与轴向流速比关系,揭示了内在有规律的独特的浓度分布结构.     

基于雷达散射矩阵的多模型融合极化目标识别

雷达目标极化特性测量在目标极化增强和极化识别等领域都具有重要应用。研究了功率矩阵的相似度与共交极化比,并据此对各种目标进行识别,提出了一种新的雷达散射矩阵多模融合目标识别模型。通过仿真分析验证了该模型的可行性和有效性。     

Forest biomass monitoring with GNSS-R: Theoretical simulations

GNSS-Reflectometry (GNSS-R) is a remote sensing technique which performs bistatic measurements of the earth surface scattering. This paper presents some theoretical simulations of the specular scattering coefficient of a forested area, with the aim of demonstrating the potentiality of GNSS-R in monitoring forest biomass. The study is performed by means of an electromagnetic model developed in the past years and tested over several vegetation covered sites in its active and passive version. Here, after showing a comparison between model results and measurements over a forest site in the monostatic configuration, and after summarizing other previous validations, the extension to the specular configuration, typical of GNSS-R systems, will be presented. Namely, simulations are carried out at circular polarization and a sensitivity analysis of the received power in the specular configuration to some soil and forest parameters is shown.