共查询到20条相似文献,搜索用时 140 毫秒
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波达方向DOA估计是雷达阵列信号处理的一个重要方向,传统的MUSIC算法对均匀阵列条件下独立信号源的估计有很强的适应性,但实际的雷达工作中,稀疏布阵下多相干源测角是一个经常出现的应用场景。文中针对二维稀疏阵列的相干源测角,提出了一种基于虚拟阵列的相干源DOA估计方法。该方法利用虚拟阵列内插的方法,将一个任意二维稀疏阵列内插为一个均匀面阵,再通过二维空间平滑方法对相干源进行测角,能够同时获得信号的方位角和俯仰角信息。稀疏面阵和稀疏圆阵的仿真实验结果表明,该方法可以有效的解决二维稀疏阵列的相干源测角问题。 相似文献
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针对相干信源DOA估计提出了一种修正ESPRIT算法,利用时域白噪声信号在不同时刻是不相关的性质,通过对在虚拟平移天线阵列过程中所得阵列的输出数据协方差矩阵进行修正,可减小白噪声的影响.该算法对独立源和相干信源的DOA估计有较高的分辨率,计算量较小,即使在低信噪比、低快拍数和小阵元数的条件下,仍具有很小的估计误差.能较准确地进行相干源的DOA估计.仿真结果验证了修正ESPRIT算法的正确性和有效性. 相似文献
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根据天线阵列接收到的数据,提出了一种基于Toeplitz矩阵重构的宽带相干源方位估计算法.该算法先由Toeplitz 阵列接收到的数据得到包含波达方向信息的协方差矩阵,再对该协方差矩阵进行聚焦处理,得到同一频率的阵列协方差矩阵,最后由高分辨子空间处理方法得到宽带相干信号的波达方向估计.仿真实验证明了该方法的有效性. 相似文献
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天波超视距雷达(OTHR)的观测范围非常广,实战中经常要求在短相干积累条件下检测出舰船目标.然而短相干积累时间带来的低多普勒分辨率很难从强大的海杂波中区分出舰船。为了解决这一问题.可以采用海杂波循环对消法,这就要求对杂波参数进行精确估计。传统方法直接利用Fourier谱中的最大幅度估计杂波参数,估计精度不高从而导致对消性能不太理想.该文提出了一种新的基于FFT相位分析的杂波对消法.该方法与传统的杂波对消相比,有效提高了参数估计精度,减小了剩余杂波强度和扩散程度,有利于舰船目标的峰值显露和从剩余杂波中区分出舰船.以上分析和比较得到了实测数据的检验。 相似文献
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针对水中声源深度分辨问题,该文提出一种基于干涉条纹斜率分布的声源深度分辨方法。该方法利用存在负跃层的浅海波导中水面和水下声源简正波激发能力的差异,建立了辐射噪声干涉条纹分布随声源深度变化的模型,分析了水面和水下声源激发的辐射噪声干涉条纹斜率分布差异性的物理机理。利用图像处理算法,将该差异表征为辐射噪声干涉图像Radon变换矩阵列方差向量的峰值个数,并据此进行水面和水下目标辨别。仿真和海试数据验证结果证明,该文提出的方法可应用于存在负跃层的浅海波导中,能有效分辨水面和水下目标,且与传统方法相比,不需要声源距离与海洋声学环境参数的先验信息。 相似文献
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被动微波遥感是海洋遥感的一项重要手段,可以测量一些重要的海洋参数,如海表面盐度、海表面风矢量等。综合孔径微波辐射计是目前被动微波遥感领域的一个研究热点。然而,由于综合孔径辐射计在空间频率上只能覆盖有限的带宽,无法获取观测目标的高频分量,所以即使不存在G矩阵误差和辐射噪声情况下,依然存在固有的系统误差。针对固有的系统误差,提出了一种系统误差降低方法应用于FPIR 系统中。仿真结果表明:该方法能够有效降低FPIR 系统误差,获取高精确度的亮温数据以满足测量海表面盐度和海表面风矢量等应用需求。 相似文献
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Reul N. Tenerelli J.E. Floury N. Chapron B. 《Geoscience and Remote Sensing, IEEE Transactions on》2008,46(3):675-688
We examine how the rough sea surface scattering of L-band celestial sky radiation might affect the measurements of the future European Space Agency Soil Moisture and Ocean Salinity (SMOS) mission. For this purpose, we combined data from several surveys to build a comprehensive all-sky L-band celestial sky brightness temperature map for the SMOS mission that includes the continuum radiation and the hydrogen line emission rescaled for the SMOS bandwidth. We also constructed a separate map of strong and very localized sources that may exhibit L-band brightness temperatures exceeding 1000 K. Scattering by the roughened ocean surface of radiation from even the strongest localized sources is found to reduce the contributions from these localized strong sources to negligible levels, and rough surface scattering solutions may be obtained with a map much coarser than the original continuum maps. In rough ocean surface conditions, the contribution of the scattered celestial noise to the reconstructed brightness temperatures is not significantly modified by the synthetic antenna weighting function, which makes integration over the synthetic beam unnecessary. The contamination of the reconstructed brightness temperatures by celestial noise exhibits a strong annual cycle with the largest contamination occurring in the descending swaths in September and October, when the specular projection of the field of view is aligned with the Galactic equator. Ocean surface roughness may alter the contamination by over 0.1 K in 30% of the SMOS measurements. Given this potentially large impact of surface roughness, an operational method is proposed to account for it in the SMOS level 2 sea surface salinity algorithm. 相似文献
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Shu-Qing Li Chi Hou Chan Leung Tsang Lin Zhou 《Geoscience and Remote Sensing, IEEE Transactions on》2002,40(3):574-582
Microwave emission of ocean surfaces with full spatial spectrum is studied in this paper. For ocean surfaces with full spectrum, the rms height of roughness can be many wavelengths, and the surface size must be chosen to be larger than the longest scale wave in the spectrum. Due to computer resources, it is not straightforward to conduct numerical simulations of emission from rough surfaces with large rms height and size since a large number of unknowns will be involved. In this paper, the multilevel expansion of the sparse matrix canonical grid (SMCG) method, which is available for surfaces with large rms heights, is used to study the emission of one-dimensional (1-D) ocean surfaces. The computational complexity and the memory requirement are still on the order of O(N log (N)) and O (N), respectively, as in the SMCG method. Ocean surfaces with size 1024 wavelengths (21.9 m at 14 GHz) and spatial spectrum bandwidth between 0.858 rads/m (corresponding to the longest scale of 341.3 wavelengths) and 4691.5 rads/m (corresponding to the shortest scale of 1/16 wavelengths), which is rather wide to be regarded as a full spectrum, are studied. The maximum of the electromagnetic wavenumber-surface rms height product is up to 25.18. The surface is modeled as a lossy dielectric surface with large relative permittivity rather than as a perfectly conducting surface, which is often adopted as an approximation in the active remote sensing of ocean surfaces. A relatively high sampling density is used to ensure accuracy. The effects of the low and high portions of the spectrum on the emissivity are studied numerically. Monte Carlo simulation for ocean surfaces is also performed by exploiting the efficiency of the multilevel expansion method and the use of parallel computing techniques. The convergence of the results with respect to the sampling density is also illustrated 相似文献
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为更好地研究海面上方低空突防飞机的雷达散射特性,基于迭代物理光学法(AIPO)和等效电流法(MEC),提出了计算电大尺寸二维导体海面上方低飞目标的AIPO+MEC算法,应用AIPO计算海面与目标之间的相互作用,用MEC计算棱边绕射。通过计算海面上金属立方体的双站散射系数,与已有数值算法结果相比较,验证了算法的正确性。用PM谱粗糙面模拟实际海面,应用该算法计算了海面上方三种典型隐身飞机模型的后向散射系数,并与自由空间中飞机模型的散射系数和平面上方飞机模型的散射系数进行了比较。结果表明,由于海面散射以及海面与飞机之间的相互作用,后向散射系数增大,且下方为海面时的散射系数角度性分布的散射比下方为平面时更为平缓。这对现代战争中海面上方低空目标探测和雷达设计具有一定的理论指导意义。 相似文献
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Lin Zhou Leung Tsang Jandhyala V. Qin Li Chan C.H. 《Geoscience and Remote Sensing, IEEE Transactions on》2004,42(8):1739-1748
In the numerical Maxwell-equation model (NMM3D) of rough-surface scattering, we solve Maxwell equations in three dimensions to calculate emissivities for applications in passive microwave remote sensing of soil and ocean surfaces. The difficult cases for soil surfaces are with exponential correlation functions when the surfaces have fine-scale structures of large slopes. The difficulty for ocean surfaces is that because the emissivities are close to that of a flat surface, the emissivities have to be calculated accurately to correctly assess the rough-surface effects. In this paper, the accuracies of emissivity calculations are improved by using Rao-Wilton-Glisson basis functions. We further use sparse matrix canonical method to solve the matrix equation of Poggio-Miller-Chang-Harrington-Wu integral equations. Energy conservation checks are provided for the simulations. Comparisons are made with results from the pulse basis function. Numerical results are illustrated for soil and ocean surfaces respectively with exponential correlation function and ocean spectrum. The emissivities of soil are illustrated at both L- and C-bands and at multiple incidence angles for the same physical roughness parameters. The brightness temperatures for ocean surfaces are illustrated for cases with various wind speeds. We compare results with those from the sparse matrix methods. Comparisons are also made with experimental emissivity measurements of soil surfaces. Parallel computation is also implemented. Lookup tables of emissivities based on NMM3D are provided. 相似文献
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基于几何光学法(GO)、物理光学法(PO)、射线弹跳法(SBR)和等效电流法(MEC),提出了一种快速计算金属海面上电大尺寸目标电磁散射的解析算法。该算法考虑了阴影效应,运用GO/PO+SBR计算了目标与海面的镜面反射以及它们之间的多次相互作用,并运用MEC计算了目标的棱边绕射以改进计算结果。应用该算法计算了平板上方规则金属目标的双站雷达散射截面(RCS),并与传统矩量法(MoM)进行比较,验证了算法的有效性。最后,计算了PM(Pierson-Moskowitz)海浪谱的随机海洋粗糙面上舰船模型目标的散射特性,并对计算结果进行了分析,讨论了海洋面以及入射波参数对散射结果的影响。 相似文献
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给出了一种基于Gabor小波变换的机载合成孔径雷达(SAR)海面风向反演的新方法。该方法利用Gabor小波对SAR图像进行二次小波分解,并对小波系数作FFT变换来获取图像谱,其低波数谱连线的垂线方向就是海面风场的风向。利用该方法获得了SAR图像海面风向信息,并与àtrous算法反演结果、浮标测得的海面风向(真值)进行了比较。实验结果表明,采用该方法获得的机载SAR海面风向反演结果与海面浮标实测数据吻合,比àtrous算法有较大改进。 相似文献