用契合方法求平面SH波对半圆形突起地形的散射

采用“契合”的方法，给出了一个求解平面SH波对半圆形凸起地形散射的新方法。利用包括半圆形凸起上边界在内的一个圆域中预先构造的满足其上半部应力为零，下半部应力任意的级数解和其余的具体半圆形凹陷的半空间中的解答，通过在其结合面上完成“契合”的过程中分别决定出出圆域和半空间中的解答，给出了问题的最终结果。利用上述方法，问题的求解仍归结为对一组无穷代数方程组的求解。最后，给出了数值结果并对其进行了讨论。     

双翼金属圆柱体散射场的整体计算

本文利用keller的几何绕射理论（GTD）推求出双翼金属圆柱体散射场高频快收敛整体解，弥补了传统分离解（把系统分解为一个金属圆柱和两个金属半平面，分别求解再简单迭加）的不足之处，最后，给出了整体解和分离解的散射电场的模值数值计算结果。     

近地空间航天员训练视景真实感渲染技术研究

载人航天任务中,地面模拟训练是培养提升航天员操作技能的重要手段。视景系统是航天飞行训练模拟的重要组成部分,高逼真度的仿真场景对提升航天员训练效果有重要的意义。针对空间视景仿真场景调度和渲染的特殊性,提出并设计实现视景仿真软件的总体架构。对影响空间场景真实感的地球纹理数据库的生成和调度技术、大气散射仿真技术、场景光照实时渲染等关键技术进行研究,融合各种方法,在视景仿真系统中基于GPU实现。试验验证表明,实现算法准确,模型设计合理,已经应用于航天员的训练中。     

混合场积分方程在开放结构散射分析中的应用

针对复合开放闭合结构电磁散射问题的矩量法求解,通过修改混合场积分方程的建立方式,将混合场积分方程扩展应用到这类开放结构,大大提高了求解效率,数值算例证明了该方法的精度和效率。     

The lower ionosphere response to its disturbances by powerful radio waves

The paper presents data from some campaigns at Sura heating facility in 2011–1016. The experiments on probing of the artificial disturbed region of the lower ionosphere were carried out at two observation sites. One of them was located near Vasil’sursk 1 km from Sura facility (56.1°N; 46.1°E) and the other site was located at the Observatory (55.85°N; 48.8°E) of Kazan State University, 170 km to the East. Investigation of the features of the disturbed region of the lower ionosphere based on its diagnostics by the methods of the vertical sounding and oblique backscattering is the main goal of this paper. Ionosphere disturbance was fulfilled by the effect of the powerful radio wave of the ordinary or extraordinary polarization emitted by transmitters of the Sura facility with effective radiated power ERP = 50–120 MW at the frequency of 4.3, 4.7 and 5.6 MHz. Pumping waves were emitted with period from 30 s to 15 min. The disturbed region of the ionosphere in Vasil’sursk was probed by the vertical sounding technique using the partial reflexion radar at the frequency of 2.95 and 4.7 MHz. For the oblique sounding of the disturbed region the modified ionosonde Cyclon-M, operating at ten frequencies from 2.01 to 6.51 MHz was used at the Observatory site. On many heating sessions simultaneous variations of the probing partial reflection signals in Vasil’sursk and backscattered signals in Observatory were observed at the height at 40–100 km below the reflection height of the pumping wave. These observations were correlated with the pumping periods of the Sura facility. Possible mechanisms of the appearance of the disturbance in the lower ionosphere and its effect on the probing radio waves are discussed.     

天籁射电阵的空间碎片探测性能分析

提出以曲靖非相干散射雷达作为一种可能的发射源与天籁射电阵组成一套双基地雷达空间碎片探测系统，对该系统的空间碎片探测性能进行计算与仿真分析，包括可探测目标雷达散射截面积(RCS)、天籁射电阵对空间目标与碎片探测时间、探测效率等。分析表明，该系统具有探测直径10 cm以下级空间小碎片的潜力，并在最后提出了一种基于该系统的交叉波束的确定方法及对空间碎片定位的方法。     

Multiple Coulomb scattering method to reconstruct low-energy gamma–ray direction in the GAMMA-400 space-based gamma–ray telescope

The GAMMA-400 currently developing space-based gamma-ray telescope is designed to measure the gamma-ray fluxes in the energy range from ～20?MeV to several TeV in the highly elliptic orbit (without shadowing the telescope by the Earth) continuously for a long time. The physical characteristics of the GAMMA-400 gamma-ray telescope, especially the angular and energy resolutions (at 100-GeV gamma rays they are ～0.01° and ～1%, respectively), allow us to consider this space-based experiment as the next step in the development of extraterrestrial high-energy gamma-ray astronomy. In this paper, a method to improve the reconstruction accuracy of incident angle for low-energy gamma rays in the GAMMA-400 space-based gamma-ray telescope is presented. The special analysis of topology of pair-conversion events in thin layers of converter was performed. Applying the energy dependence of multiple Coulomb scattering for pair components, it is possible to estimate the energies for each particle, and to use these energies as weight in the angle reconstruction procedure. To identify the unique track in each projection the imaginary curvature method is applied. It allows us to obtain significantly better angular resolution in comparison with other methods applied in current space-based experiments. When using this method for 50-MeV gamma rays the GAMMA-400 gamma-ray telescope angular resolution is about 4°.     

时变海面复反射系数建模

基于二维时变海面模型和粗糙面电磁散射的低阶小斜率近似方法,研究了海面复反射系数的时变和统计特性.在电磁散射幅度基础上推导了粗糙面反射系数及其相干和非相干分量,相干分量理论计算公式与经验模型一致.仿真结果表明相干分量幅度与经验模型基本吻合,但相位中存在明显的起伏特性,这种起伏在经验公式中没有体现出来.引入Middleton相位差统计模型为反射系数时变特性建模,仿真数据统计与理论分布吻合较好,且概率密度函数的等高图可以很好地表征时变复反射系数间的相关特性.这种吻合性表明复反射系数在短时间尺度上满足高斯分布,但其幅度和频率被海浪长波调制.      

基于Pauli基分解的极化校准算法

极化校准是现代雷达精确获取目标极化散射特性的前提和基础。为解决某全极化雷达的校准问题,提出一种基于Pauli基分解的极化校准算法,给出了算法的正交条件和相关推导,可选择任意满足正交条件的三个目标做为定标体。对校准算法的误差来源和误差对校准结果的影响分别进行了理论分析和仿真分析。给出了不同条件下该校准算法和其它校准算法的仿真结果,以及某全极化雷达校准试验数据分析结果。结果表明：基于Pauli基分解的极化校准算法能有效消除天线的变极化效应,可更准确地校准目标的极化散射矩阵,并可应用于大型地基极化雷达、极化合成孔径雷达以及极化相控阵雷达等的极化校准。     

基于属性散射中心模型的SAR超分辨成像算法

基于属性散射中心模型,提出一种稳健而快速的SAR超分辨成像算法,在超分辨的同时能够考虑到目标的整体结构。首先利用改进的正交匹配追踪算法（OMP）对简化的属性散射中心模型进行参数估计,然后基于估计的模型参数在信号重构时进行二维频谱外推实现SAR超分辨成像。该算法具有较高的运算效率,相对于传统基于点散射模型超分辨算法,能够有效解决部件不连续的问题,并且初始指向角的利用可以取得良好的聚焦效果。仿真实验验证了该算法的优越性。