Method for denoising and reconstructing radar HRRP using modified sparse auto-encoder

A high resolution range profile (HRRP) is a summation vector of the sub-echoes of the target scattering points acquired by a wide-band radar. Generally, HRRPs obtained in a non-cooperative complex electromagnetic environment are contaminated by strong noise. Effective pre-processing of the HRRP data can greatly improve the accuracy of target recognition. In this paper, a denoising and reconstruction method for HRRP is proposed based on a Modified Sparse Auto-Encoder, which is a representative non-linear model. To better reconstruct the HRRP, a sparse constraint is added to the proposed model and the sparse coefficient is calculated based on the intrinsic dimension of HRRP. The denoising of the HRRP is performed by adding random noise to the input HRRP data during the training process and fine-tuning the weight matrix through singular-value decomposition. The results of simulations showed that the proposed method can both reconstruct the signal with fidelity and suppress noise effectively, significantly outperforming other methods, especially in low Signal-to-Noise Ratio conditions.     

航天器相对姿态跟踪的非线性前馈控制

针对航天器相对姿态跟踪过程中严重的非线性及控制器设计的复杂性,建立了基于修正罗德里格斯参数的航天器相对姿态运动学和动力学方程并根据Lyapunov直接法设计了非线性前馈控制律.设计的控制律不仅保证闭环系统稳定,还使得航天器相对姿态跟踪误差快速收敛到零点邻域内.通过在Matlab/Simulink环境下对航天器相对姿态跟踪进行数值仿真,验证了建立模型和设计控制律的有效性.     

Testing Modified Newtonian Dynamics with LISA Pathfinder

We suggest that LISA Pathfinder, a technology demonstrator for the future gravitational wave observatory LISA, could be used to carry out a direct experimental test of Modified Newtonian Dynamics (MOND). The LISA Pathfinder spacecraft is currently being built and the launch date is just a few years away. No modifications of the spacecraft are required, nor any interference with its nominal mission. The basic concept is to fly LISA Pathfinder through the region around the Sun-Earth saddle point, in an extended mission phase, once the original mission goals are achieved. We examine various strategies to reach the saddle point, and find that the preferred strategy, yielding relatively short transfer times of just over 1 year, probably involves a lunar fly-by. LISA Pathfinder will be able to probe the intermediate MOND regime, i.e. the transition between deep MOND and Newtonian gravity. We present robust estimates of the anomalous gravity gradients that LISA Pathfinder should be exposed to, based on MONDian effects as derived from the Tensor-Vector-Scalar (TeVeS) theory. The spacecraft speed and spatial scale of the MOND signal combine in a way that the spectral signature of the signal falls precisely into LISA Pathfinder’s measurement bandwidth. We find that if the gravity gradiometer on-board the spacecraft achieves its currently predicted sensitivity, these anomalous gradients could not just be detected, but measured in some detail.     

Interface flux reconstruction method based on optimized weight essentially non-oscillatory scheme

Aimed at the computational aeroacoustics multi-scale problem of complex configurations discretized with multi-size mesh, the flux reconstruction method based on modified Weight Essentially Non-Oscillatory (WENO) scheme is proposed at the interfaces of multi-block grids. With the idea of Dispersion-Relation-Preserving (DRP) scheme, different weight coefficients are obtained by optimization, so that it is in WENO schemes with various characteristics of dispersion and dissipation. On the basis, hybrid flux vector splitting method is utilized to intelligently judge the amplitude of the gap between grid interfaces. After the simulation and analysis of 1D convection equation with different initial conditions, modified WENO scheme is proved to be able to independently distinguish the gap amplitude and generate corresponding dissipation according to the grid resolution. Using the idea of flux reconstruction at grid interfaces, modified WENO scheme with increasing dissipation is applied at grid points, while DRP scheme with low dispersion and dissipation is applied at the inner part of grids. Moreover, Gauss impulse spread and periodic point sound source flow among three cylinders with multi-scale grids are carried out. The results show that the flux reconstruction method at grid interfaces is capable of dealing with Computational AeroAcoustics (CAA) multi-scale problems.     

RDX含量对改性双基推进剂动态力学性能的影响

利用动态热机械分析(DMA)研究了一组不同黑索今(RDX)含量的改性双基推进剂的低温动态力学性能。β松弛的峰温几乎不受固体填料加入的影响。认为RDX含量超过一定值时,在低温下将起到辅助增塑作用,β松弛tanδ峰值与"等效增塑剂"的含量有关。经拟合得到"等效增塑剂"的含量。从推进剂的动态模量主曲线获得了β松弛的粘弹系数Cg1,Cg2以及松弛过程(分子构象变化)的活化能Ea,以及"脆化参数"m,并用线性方程关联了"脆化参数"m与低温抗拉强度σm和延伸率εm。     

基于FIP WA的RCS快速计算

为改善基于矩量法(MOM)快速多极子(FMM)的稳定性,介绍了快速非均匀平面波算法(FIPWA).根据入射波及电场积分方程(EFIE),采用修正最陡下降路径(MSDP)进行数值积分和内插外推转换,建立了二雏FIPWA模型.该法基于格林函数谱域积分,其转移因子不含特殊函数而仅有初等函数,便于数值实现和稳定性控制,其多层形式复杂度与多层快速多极子(MLFMA)相当.算例表明:该算法与MOM吻合较好,且大幅节省计算时间及计算机内存.     

改性BMI／DPA和CTBN增韧环氧树脂的温度,力学性能及本构关系研究

研究了ＣＴＢＮ增韧环氧树脂和烯丙基双酚Ａ改性双马树脂（ＢＭＩ／ＤＰＡ）在不同温度和加载速率下的拉伸和压缩力学性能。对于ＣＴＢＮ 增韧环氧树脂,材料在动态拉伸情况下,随着应变率的增大,材料由韧变脆,模量升高,断裂伸长率下降;在压缩情况下,弹性模量和屈服应力均随着加载速率的增大而增大。对于改性双马树脂,在室温的动载压缩下,其模量Ｅ和屈服应力σｙ均基本上与ｌｎε呈直线关系增大,并给出了该树脂在不同加载速率下的压缩应力应变曲线。计算了两种材料的温度敏感度和加载速率敏感度以及温度和应变率对两种树脂材料屈服应力影响的本构关系。     

几种化合物在改性双基推进剂中降低燃速的作用

本文介绍了六种化合物在改性双基推进剂中的降燃速作用，这些化合物是黑索今（ＲＤＸ）、奥克托金（ＨＭＸ）、１，３，５－三氨基２，４，６－三硝基苯（ＴＡＴＢ）、硝酸铵、蔗糖入醋酸酯（ＳＯＡ）、草酸铵。讨论了它们对燃气发生剂降低燃速的贡献和机理，从实验数据的分析中得出了几点有用的结论。     

PDADN-RDX-CMDB推进剂催化燃烧特性研究

采用热分析、微热电偶技术、燃速测试、熄火表面的扫描电镜观测等实验方法，研究了不同类型的复合催化剂对PDADN－RDX－CMDB推进剂燃烧特性的影响。结果发现，邻苯二甲酸铅／雷索辛酸铜／炭黑与雷索辛酸铅铜／炭黑两类复合催化剂可较好地改善PDADN－RDX－CMDB推进剂的燃烧特性，明显降低其压强指数且同时提高燃速，基于实现现象的观测结果分析，提出了“气泡－凝取相反应”理论，解释了该类推进剂在中枢 压区发生的“超速燃烧”现象。     

碳纤维增强双马来酰亚胺树脂基复合材料体系冲击后压缩强度研究

探讨了树脂基体、碳纤维增强体以及树脂基体 纤维的界面等对双马来酰亚胺 (简称双马 )树脂基复合材料冲击后压缩强度 (CAI)值的影响 ,指出降低树脂基体的交联密度和产生微观两相结构是提高碳纤维 /双马复合材料CAI值的两个典型方法。合适的树脂含量有利于保持复合材料体系较高的CAI值 ,采用高强高韧性的碳纤维可明显提高复合材料体系的CAI值。为获得较高的CAI值 ,保持合适的树脂基体 纤维界面性能也是必要的