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.     

基于滑模控制的剖面跟踪制导律

针对高超声速飞行器滑翔段的高精度制导问题，考虑复杂多约束条件以及干扰和不确定因素的影响，设计了一种基于全局积分滑模控制的剖面跟踪制导方法。首先，将多重约束转化为阻力加速度-速度（D-V）平面内的再入走廊；然后，以终端精度和总吸热量为性能指标，采用分段函数的形式优化设计出一条标准D-V剖面；再基于简化的动力学模型，推导得到关于阻力加速度微分和速度的二阶非线性模型；最后，基于滑模控制理论，设计全局积分滑模面和指数趋近律，获得控制量幅值大小，并结合侧向方位误差走廊确定控制量符号，从而实现对标准剖面的有效跟踪。采用CAV-H滑翔再入模型进行数值仿真，分析验证了提出的基于滑模控制的剖面跟踪制导律具有较好的跟踪性能和精度。     

基于改进A~*算法的进离场航线网络3D规划

为提高终端空域航线设计的自动化水平,对进离场航线进行了研究。针对独立航线规划,提出角度扩展航路点搜索方法,提高算法运行效率。选取水平剖面经济性最优为目标函数,垂直剖面满足最优爬升/下降剖面,实现3D航线网络规划。实例结果表明,在保证航线安全性、经济性的同时,算法运行稳定,效率明显提高。     

On Stabilizing Role of Parallel Inhomogeneous Flow on Low-frequency Space Fluctuations

A fundamental reality throughout the space plasma is the existence of magnetic field-aligned flows. It is usually believed that the spatial transverse shear in the parallel flow destabilizes many low frequency oscillations and this may be the origin of low frequency oscillations in the ionosphere (V. V. Gavrishchaka et al., 1998, Phys. Rev. Lett., 80, 728 and Phys. Rev. Lett.: 2000, 85, 4285). Here we show that this notion of destabilizing influence of the shear in the parallel flow can be changed altogether if one takes the effect of the flow curvature (second spatial derivative) into account. The transverse curvature in the parallel flow can overcome the destabilizing influence of the shear and can render the low frequency modes stable. It is shown that unlike flow shear the effect of flow curvature is sign- and mode-dependent. This revised version was published online in August 2006 with corrections to the Cover Date.     

双齿气体循环泵基本几何理论和容积计算

以数学几何理论为基础,通过坐标变换和包络条件推导了阴阳转子的基本型线方程,建立了双齿气体循环泵的数学模型。研究了阴阳转子相互啮合时啮合点位置随阴转子转角的变化关系。采用了线积分的计算方法推导出工作容积的基元面积随转角的变化关系,可简化工作容积的计算难度。结果表明:在转角为0和π的时候,阴阳转子会形成一个封闭的无效区域导致了工作腔的基元面积随转角变化过程中的突升和突降。在吸气结束时,由于吸气腔相较于排气腔多了一个与吸气口相连的部分导致了基元面积的突降。这些基本几何理论的建立可为双齿气体循环泵的应用打下一定的理论基础。     

Optimal multi-site selection for a PV-based lunar settlement based on a novel method to estimate sun illumination profiles

Recently, space organizations have considered the Moon to host lunar bases. Such bases require power and energy to function. However, the efficient and safe use of the energy resources on the Moon is a huge challenge. Space photovoltaic (PV) power systems are appealing technologies due to their maturity and high solar energy availability at some locations on the Moon. The effectiveness of these PV systems depends on their selenographic location, which might necessitate the deployment of energy storage technologies to cover the base’s energy demand. Some analysts have proposed the installation of PV modules on kilometers-tall towers near the lunar poles to harvest more solar energy and limit the need for energy storage systems (ESSs). Alternatively, this paper proposes to harvest the energy from multiple sites in the lunar South Pole region using a novel technique to compute the Sun illumination profile and the LOLA topographic databases to compute the terrain elevations. The proposed algorithm seeks the most optimal configuration of sites and tower heights to minimize the longest night period and total distance between the sites. This study assesses groups of 1 to 6 sites assuming the use of towers having heights of 10, 100, and 500 [m]. The time horizon for the analysis is one Axial Precession Cycle, which is approximately 18.6 years. According to the results, a system of two sites with a separation of 42.05 [km] and towers of 500 [m] height has a maximum darkness period of only 3 [h] while another solution proposes a system of three sites with towers of 10 [m] that removes the need of EES (solar eclipse periods by the Earth are not considered). The proposed technique is suitable for engineering applications, such as base planning and operation management.     

一种大负荷低压涡轮叶型的气动性能

基于Lantry-Menter转捩模型,分别对Zweifel升力系数为1.2的一种大负荷低压涡轮叶型在定常来流不同湍流度、雷诺数条件下,上游非定常、周期性尾迹作用下的流动进行了数值模拟.计算结果表明,定常来流低雷诺数条件下,湍流度对该大负荷叶型的气动性能影响较大;上游非定常、周期性尾迹对叶型吸力面分离泡的抑制作用可进一步减小低雷诺数条件下的叶型损失.计算结果揭示了该大负荷叶型在低压涡轮内部真实流动环境中的表面流动及损失特征,对国内现行低压涡轮设计有着较好的启示.      

Usage of pre-flight data in short rendezvous mission of Soyuz-TMA spacecrafts

The paper describes the reduction of the vehicle autonomous flight duration before docking to the ISS. The Russian Soyuz-TMA spacecraft dock to the ISS two days after launch. Due to the limited volume inside Soyuz-TMA the reduction of time until docking to the ISS is very important, since the long stay of the cosmonauts in the limited volume adds to the strain of the space flight. In the previous papers of the authors it was shown that the existing capabilities of Soyuz-TMA, the ISS and the ground control loop make it possible to transfer to the five-orbit rendezvous profile. However, the analysis of the cosmonauts' schedule on the launch day shows that its duration is at the allowable limit and that is why it is necessary to find a way to further reduce the flight duration of Soyuz-TMA before docking to less than five orbits. In a traditional rendezvous profile, the calculation of rendezvous burns begins only after determination of the actual vehicle insertion orbit. The paper describes an approach in which the first two rendezvous burns are performed as soon as the spacecraft reaches the reference orbit and the values of the burns are calculated prior to the launch based on the pre-flight data for the nominal insertion. This approach decreases the duration of the rendezvous by one orbit. The demonstration flight of a Progress vehicle using the proposed profile was implemented on August 1, 2012 and completely confirmed the correctness of the imbedded principles. The paper considers the possible improvements of the proposed approach and recovery from the contingencies.     

对信息检索系统应用技术的数学表示模型的分析

页面表示、用户兴趣模型、页面链接排序是信息检索系统中的关键技术,分析相应的数学模型,并例举在一个智能搜索引擎中的应用,通过动态的更新用户兴趣模型和由此而引起的WEB页面更新,有效地适应用户兴趣的变化。     

脉冲星导航试验卫星科学观测数据分析

脉冲星导航试验卫星是我国发射的一颗专用试验卫星.经过4个多月的在轨观测,该卫星已成功获取了大量观测数据.介绍利用该卫星搭载的掠入射聚焦型X射线探测器在近4个月中对PSR B0531+21获得的观测数据第一批处理结果.本文详细阐述掠入射聚焦型X射线探测器的观测模式,给出脉冲星观测数据的处理方法以及脉冲星参数的拟合过程,利用基于第一手观测数据的脉冲星精化参数验证掠入射聚焦型探测器在轨工作性能,得以回答使用国产X射线探测器是否能够“看得见”脉冲星问题.