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.     

采用连续旋转检偏器的天空偏振光探测装置设计与实现

为了实现对运动目标与天空散射光的偏振分布模式进行快速、有效的探测,根据连续旋转检偏器光强度透射的数学模型,利用光电传感器的积分特性,设计并构建了采用连续旋转检偏器的偏振成像探测装置。测试结果表明,该装置对偏振光的角度的测量精度优于0.069°（3σ）,偏振度的测量精度优于0.12%（3σ）。一幅偏振图像的探测时间达到0.7s。在偏振度低于4%的情况下,仍可以探测到有规律的偏振分布模式,其抵抗恶劣天气的性能优于现有的偏振导航探测装置。     

一种地空3D-Massive MIMO信道模型

为了研究地空3D-Massive MIMO系统信道特性,提出一种基于三维单跳同心圆环散射体的地空3D-Massive MIMO信道模型。相比传统地空3D MIMO信道模型有两方面改进,首先是建立了基于单跳圆环散射体3D几何精确位置关系的球面波天线阵元相位偏移模型,其次采用生灭过程对Massive MIMO阵列上的非平稳特性进行建模。推导了该模型的信道统计特征函数,通过对特征函数理论推导值与蒙特卡洛统计值进行仿真对比,验证了理论推导正确性。此外,对所提信道模型与基于平面波的传统地空3D MIMO信道模型的空间相关性进行了分析及仿真对比,结果表明:在远场环境下,两者基本一致;在近场环境下,传统平面波模型不再适用,两者存在差异。最后,对若干组表征信道特征的仿真结果与公开文献中地空信道实际测试数据进行对比分析。表明本模型作为普遍适用性模型,可以根据信道的测试条件、测试环境和测试结果来优化参数配置以趋近于实际信道,以对特定信道进行精确建模。     

High-precision RCS measurement of aircraft’s weak scattering source

The radar cross section(RCS) of weak scattering source on the surface of an aircraft is usually less than 40 d Bsm.How to accurately measure the RCS characteristics of weak scattering source is a technical challenge for the aircraft's RCS measurement.This paper proposes separating and extracting the two-dimensional(2D) reflectivity distribution of the weak scattering source with the microwave imaging algorithm and spectral transform so as to enhance its measurement precision.Firstly,we performed the 2D microwave imaging of the target and then used the 2D gating function to separate and extract the reflectivity distribution of the weak scattering source.Secondly,we carried out the spectral transform of the reflectivity distribution and eventually obtained the RCS of the weak scattering source through calibration.The prototype experimental results and their analysis show that the measurement method is effective.The experiments on an aircraft's low-scattering conformal antenna verify that the measurement method can eliminate the clutter on the surface of aircraft.The precision of measuring a 40 d Bsm target is 3–5 d B better than the existing RCS measurement methods.The measurement method can more accurately obtain the weak scattering source's RCS characteristics.     

终端为“半球＋平面叶片”时进气道的RCS

首先分析了进气道等效圆波导中发动机等效“半球＋ 平面扇形金属叶片”终端的不连续性,根据电磁场互易定理和物理光学法（ Ｐ Ｏ） 计算了这种终端的反射系数;然后利用“传输模式叠加法”计算了进气道的雷达散截面（ Ｒ Ｃ Ｓ） 。计算结果与实验结果比较吻合,优于文献给出的计算结果。这种方法采用模式迭加求和,避免了普通模式法需进行大型矩阵计算以及对计算机内存的过高要求。     

测量表面粗糙度参数的反散射计算研究

用光的角散射分布技术测量工件表面的粗糙度参数是近几年来发展起来的新的测量技术。它具有分辨力高、非接触、区域平均和快速测量等优点,可获得多个表面粗糙度参数。采用该技术测量的实验装置角分辨力为0.1°,测量范围为0.6328μm<λ_s(空间平均波长)<40μm,0.0001<△_a(轮廓的算术平均斜率)<0.0088,2nm相似文献   

频率选择表面(FSS)在天线隐身技术中的应用

本文简要叙述了飞行器隐身技术中通常采用的三种方法。飞行器采取上述隐身技术措施后,机载雷达天线对电磁波的散射成为飞行器的主要散射源。因此,天线隐身技术的研究就显得十分重要。本文介绍的频率选择表面(FSS)是一种由无源谐振单元,按一定排列方式组成的准二维平面周期结构,利用其对电磁波具有频率及极化的双重滤波的概念,以达到降低天线雷达截面积(RCS)的效果。文中用谱域分析法对十字形振子阵FSS的特性进行了分析计算,并应用于天线罩或低RCS反射面天线中。对已加工出的面积为42×42cm~2,在聚四氟乙烯玻璃纤维布上的十字形振子阵FSS样品进行了性能测试,从测试曲线看出方法是有效的。     

对空时自适应处理技术的欺骗干扰研究

介绍了机载相控阵雷达STAP技术的基本原理,提出一种针对目标保护的相干散射干扰方法。将接收到的雷达信号用数字射频存储器（DRFM）存储,经频率调制形成密集的相干脉冲串干扰信号,使得最优二维频率响应,在目标所在的距离单元上除了真实目标外,还存在多个欺骗假目标。理论分析和仿真结果表明了该方法的有效性。     

GNSS无源 MIMO雷达系统及其探测性能分析

提出一种综合使用多GNSS系统可用导航卫星信号源和基于MIMO信号处理体制的无源多基地雷达系统结构,利用M IM O处理获得的空间分集增益来改善雷达探测性能。分析了系统的可用信号源情况,讨论了系统中前向散射区的确定和目标前向散射RCS的计算问题,在此基础上,对基于GNSS信号的无源MIMO雷达系统的探测性能进行了深入研究并给出了仿真计算结论。     

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.