基于非线性器件特征的辐射源识别

为提高雷达辐射源的正确识别率以满足航空电子对抗需求,提出基于非线性器件特征的辐射源识别方法.在非线性失真分析的基础上,通过谱再生现象的观测,对非线性器件的功率级数系数进行了估计,由于不同的雷达系统设计和随机组装,因此这种特征对每一辐射源是唯一的.仿真结果表明,该特征提取方法在低信噪比环境下可以获得高的辐射源识别率,证实...     

Optimal satellite formation reconfiguration actuated by inter-satellite electromagnetic forces

The inter-satellite electromagnetic forces generated by the magnetic dipoles on neighboring satellites provide an attractive control actuation alternative for satellite formation flight due to the prominent advantages of no propellant consumption or plume contamination. However, the internal force nature as well as the inherent high nonlinearity and coupling of electromagnetic forces bring unique dynamic characteristics and challenges. This paper investigates the nonlinear translational dynamics, trajectory planning and control of formation reconfiguration actuated by inter-satellite electromagnetic forces. The nonlinear translational dynamic model is derived by utilizing analytical mechanics theory; and analysis on the dynamic characteristics is put forward. Optimal reconfiguration trajectories of electromagnetic force actuated formation are studied by applying optimal control theory and the Gauss pseudospectral method. Considering the high nonlinearity and uncertainty in the dynamic model, an inner-and-outer loop combined control strategy based on feedback linearization theory and adaptive terminal sliding mode control is proposed with finite-time convergence capability and good robust performance. Theoretical analysis and numerical simulation results are presented to validate the feasibility of the proposed translational model, reconfiguration trajectory optimization approach and control strategy.     

加权型中值定理

本文给出了Cauchy和Lagrange中值定量的一种推广形式：加权型中值定理。     

基于流固耦合航行体入水冲击数值模拟研究

针对航行体入水冲击过程中的流固耦合问题,利用任意拉格朗日 欧拉算法建立三维入水冲击数值仿真模型。首先,建立球体入水冲击数值模型,获取了入水过程中的冲击载荷和表面压力数据,通过与试验对比,探究网格密度、接触刚度耦合系数以及时间步长对仿真准确性的影响。结果发现,冲击区域网格密度和接触刚度耦合系数决定流固耦合接触刚度;冲击域的网状密度对冲击系数结果和入水速度变化有明显影响;耦合节点之间的接触刚度系数会影响局部压力峰值。最后,建立锥形头部圆柱体入水仿真模型,提出分段刚体计算截面载荷方法,研究不同速度下结构入水冲击加速度、速度、位移和截面载荷变化规律,与试验结果对比证明仿真准确性。     

基于Hankel矩阵填充的稀疏孔径ISAR成像

在稀疏孔径(SA)逆合成孔径雷达(ISAR)成像中,传统压缩感知(CS)方法使用稀疏信号处理来处理数据缺失下的成像问题。这类方法存在模型不匹配这一固有问题,在一定程度上会限制成像质量。提出了一种利用Hankel矩阵填充(HMC)的基于结构化稀疏ISAR成像方法。该方法是一种典型的无网格方法,可以有效地提高稀疏孔径ISAR成像性能。首先,建立ISAR稀疏孔径成像信号模型,根据每个距离单元的回波构造Hankel矩阵;其次,通过证明所构造Hankel矩阵的低秩性质,作为方位稀疏成像的先验信息约束;最后,通过逐步迭代求解基于增广拉格朗日乘子(ALM)的矩阵填充(MC)来实现重构方位维成像。提出的基于低秩约束的方法,可以避免过完备基的假设,有效地克服了CS方法的离网格效应。基于实测数据的实验分析,进一步验证了所提算法的有效性。     

考虑高耗时约束的全电推进卫星多学科优化

为提高卫星系统整体性能与优化设计效率，本文采用多学科设计优化（MDO）方法进行全电推进卫星总体参数优化。主要考虑轨道转移、位置保持、空间环境、供配电、结构及质量六个学科，以整星质量最小为优化目标，考虑轨道转移时间等约束条件，建立了全电推进卫星MDO模型。提出一种基于增广拉格朗日乘子法的高效全局优化方法（ALM-EGO）以快速求解卫星MDO问题。标准数值算例对比研究表明，对于处理高耗时约束优化问题，ALM-EGO方法在全局收敛性与优化效率方面具有一定的优势。最后，采用ALM-EGO求解全电推进卫星MDO问题，优化后的全电推进卫星设计方案满足各类工程设计约束，实现整星减重161.09 kg，从而验证了本文所建立模型的合理性和ALM-EGO方法的有效性。     

Motion equations of hemispherical resonator and analysis of frequency split caused by slight mass non-uniformity

The mass non-uniformity of hemispherical resonator is one of reasons for frequency split, and frequency split can cause gyroscope to drift. Therefore, it is of great significance to analyze the relationship between mass non-uniformity and frequency split, which can provide a theoretical basis for mass balance of imperfect resonator. The starting point of error mechanism analysis for gyroscope is the motion equations of resonator. Firstly, based on the Kirchhoff-Love hypothesis in the elastic thin shell theory, the geometric deformation equations of resonator are deduced. Secondly, the deformation energy equation of resonator is derived according to the vibration mode and relationship between the stress and strain of hemispherical thin shell. Thirdly, the kinetic energy equation of resonator is deduced by the Coriolis theorem. Finally, the motion equations of resonator are established by the Lagrange mechanics principle. The theoretical values of precession factor and natural frequency are calculated by the motion equations, which are substantially consistent with the ones by the finite element method and practical measurement, the errors are within a reasonable range. Simultaneously, the varying trend of natural frequency with respect to the geometrical and physical parameters of resonator by the motion equations is consistent with that by the finite element analysis. The above conclusions prove the correctness and rationality of motion equations. Similarly, the motion equations of resonator with mass non-uniformity are established by the same modeling method in case of ignoring the input angular rate and damping, and the state equations with respect to the velocity and displacement of vibration system are derived, then two natural frequencies are solved by the characteristic equation. It is concluded that one of reasons for frequency split is the 4th harmonic of mass non-uniformity, and thus much attention should be paid to minimizing the 4th harmonic of mass non-uniformity in the course of mass balancing for imperfect resonator.     

涡轮叶片外换热计算程序对比研究

对两种涡轮叶片外换热计算程序STAN 5和S1ICH的数值方法进行了比较.采用STAN5和S1ICH程序完成了VKI(Von Karman Institute)高压涡轮导叶和动叶叶栅的外传热系数计算,并将计算结果与试验数据进行了对比.结果表明,S1ICH预估的转捩位置、外传热系数的精度较高,同时S1ICH具有适应性广,收敛性好,准备初始参数方便的特点,满足工程设计计算的要求.      

The feasibility of using an L1 positioned dust cloud as a method of space-based geoengineering

In this paper a method of geoengineering is proposed involving clouds of dust placed in the vicinity of the L₁ point as an alternative to the use of thin film reflectors. The aim of this scheme is to reduce the manufacturing requirement for space-based geoengineering. It has been concluded that the mass requirement for a cloud placed at the classical L₁ point, to create an average solar insolation reduction of 1.7%, is 7.60 × 10¹⁰ kg yr⁻¹ whilst a cloud placed at a displaced equilibrium point created by the inclusion of the effect of solar radiation pressure is 1.87 × 10¹⁰ kg yr⁻¹. These mass ejection rates are considerably less than the mass required in other unprocessed dust cloud methods proposed and are comparable to thin film reflector geoengineering requirements. Importantly, unprocessed dust sourced in-situ is seen as an attractive scheme compared to highly engineered thin film reflectors. It is envisaged that the required mass of dust can be extracted from captured near Earth asteroids, whilst stabilised in the required position using the impulse provided by solar collectors or mass drivers used to eject material from the asteroid surface.