SSPS-OMEGA超大型球形聚光器结构拓扑构型与设计

为同时兼顾千米量级尺度空间太阳能电站聚光系统的在轨发射安装难度、光学收集效率、稳定性及结构工艺等多方面的因素,提出采用基于球面正多面体的经纬线划分法模块化构建球形聚光器。该方法不仅可实现基础划分单元分布均匀、规格种类少,降低在轨构建与运载发射难度。而且只要合理控制弧高等分数和基础划分单元的口径就可以同时保证聚光系统的光学收集效率。理论与仿真结果显示,当弧高等分数为24时,该划分法共有25种基础单元件,整个球面被分成5762块。并且此时模块化构建的实际球形聚光器的光学收集效率与理想球面相比基本保持不变,解决了太阳能电站聚光系统设计中存在的关键问题。     

考虑侧窗约束的模型预测静态规划末制导方法

针对红外导引头侧窗探测模式下,非对称视场约束造成末制导阶段目标易丢失的问题,提出一种考虑侧窗约束的模型预测静态规划末制导方法。首先,基于体视线坐标系建立三维相对运动模型,得到不依赖于“小攻角”假设的准确模型。在处理无过程约束问题的模型预测静态规划方法基础上,引入松弛变量与虚拟控制量,设计出考虑侧窗视场约束的末制导算法。为了进一步降低末制导算法对初始猜测轨迹的依赖性,提高适应性与计算效率,提出逐步增加约束条件的计算策略。仿真结果表明,该方法在末制导过程中满足侧窗约束,相比于凸优化方法,优化变量减少,计算速度更快;相比于基于障碍李雅普诺夫函数的末制导律,能够满足侧窗约束,同时能适应不同的初始条件。     

海洋定位卫星性能分析

编队卫星是重要的空间设施,为保证编队卫星在空间复杂环境中的工作效率,需对编队卫星的工作原理、状态进行分析。以三星编队的海洋定位卫星为例,由于该编队卫星工作状态常受到星间基线、目标源位置、卫星高度等多种因素的制约,易造成定位模糊等问题。在评价海洋定位卫星性能方面,传统的方法主要着眼于定位精度,而忽略了定位迭代解算时间这一指标,而在特定的场景下(海上搜救、抢险救灾),较短的解算时间可以迅速找出目标源的概略位置。通过分析海洋定位卫星的时差测量定位原理,对定位误差精度进行了分析,提出水平精度因子(HDOP)和最小二乘迭代结合的评价方法,分析了影响卫星性能的因素,包括目标源相对几何位置、卫星高度及卫星几何构型等方面的影响。仿真结果表明:本文的设计可以提高卫星的定位效果,为定位卫星的参数设定提供参考。     

碳纤维前驱体的研究进展北大核心CSCD

综述了可用于制备碳纤维的各类改性聚丙烯腈前驱体以及完全可替代型前驱体的最新研究进展,包括各种新型前驱体的制备以及碳化后的纤维结构与性能等,并介绍了其潜在应用领域,对各类前驱体发展目前面临的问题进行了总结,拟为制备高性能、低成本碳纤维前驱体进一步发展提供参考。     

基于摄影测量技术的航天发动机装配过程几何参数测量方法研究

当前我国航天发动机装配过程几何参数的测量方法为专业人员操作激光跟踪仪或全站仪逐点位进行测量,此类方法存在测量效率低的缺点。针对此问题,提出了一种高效的基于摄影测量技术的航天发动机装配过程几何参数测量方法,对该测量方法的测量原理进行了介绍,详细说明了这一方法各测量环节实现的测量目的,最后通过实测数据计算工业数字摄影测量技术在此类应用中的系统准确度,证明了该测量方法的可行性。     

非恒定增压式微尺度拉瓦尔喷管流动特性

针对微尺度喷流在航天器运动状态切换时出现的非恒定增压变化,采用直接模拟蒙特卡洛(DSMC)方法对阶跃式增压和线性式增压两种模式下的微尺度拉瓦尔喷管流场进行了模拟,并对其变化过程中的流动特性进行了对比分析。结果显示：阶跃式增压会导致流动特性出现较大幅值的峰谷式波动,而线性式增压下的流动特性则呈现出线性变化的特点;黏性力对微尺度喷流的非恒定增压变化产生了重要的黏滞作用,在喉部扩张段至出口的流场中尤为明显;在设定的条件下,阶跃式增压过程中喷流产生的总冲量较线性式增压高59.5%,质量流量高74.7%,单位工质提供的冲量低约8.6%,波动性也高于线性式模型,阶跃式增压适用于系统需要较大推力改变运动状态且推进剂充足的情况,而线性式增压在系统精确微调或需要推进剂产生更高效能时具有明显的优势。     

Effects of yaw-roll coupling ratio on lateral-directional aerodynamic characteristics

Experimental investigation of large amplitude yaw-roll coupled oscillations was conducted in a low-speed wind tunnel using an aircraft configuration model. A special test rig was designed and constructed to provide different coupled motions from low to high angles of attack.A parameter ‘‘coupling ratio" was introduced to indicate the extent of yaw-roll coupling. At each pitch angle, seven coupling ratios were designed to study the yaw-roll coupling effects on the lateraldirectional aerodynamic characteristics systematically. At high angles of attack, the damping characteristics of yawing and rolling moments drastically varied with coupling ratios. In the coupled motions with the rotation taking place about the wind axis, the lateral-directional aerodynamic moments exhibited unsteady characteristics and were different from the ‘‘quasi-steady" results of the rotary balance tests. The calculated results of the traditional aerodynamic derivative method were also compared with the experimental data. At low and very high angles of attack, the aerodynamic derivative method was applicative. However, within a wide range of angles of attack, the calculated results of aerodynamic derivative method were inconsistent with the experimental data, due to the drastic changes of damping characteristics of lateral-directional aerodynamic moments with yaw-roll coupling ratios.     

Mean energy of response to galactic cosmic ray spectrum: IMP 8 and Climax neutron monitor

Solar modulations of galactic cosmic ray (GCR) intensity contain a wealth of information about their transport in the heliosphere. To extract this information from the data one studies the dependence of the observed modulations on the mean energy of response of detectors providing data for the analyses. There is a great deal of confusion about the detector energy response to GCR spectrum in the literature. We present a preliminary report on the computations of the mean energy of response for the Climax neutron monitor (CL/NM) and IMP 8 cosmic ray nuclear composition instrument to GCR protons for 1973–1998, covering the solar cycles 21 and 22. We find that for penetrating proton channel on IMP 8 the mean energy changes by a factor of over two whereas for the neutron monitor the change is only 21%. However, the corresponding change for the computed modulation function is a factor of about 3.5.     

Remote upgrading of a space-borne instrument

The main purposes of experiment “Obstanovka” (“Environment” in Russian) consisting of several instruments are to measure a set of electromagnetic and plasma phenomena characterizing the space weather conditions, and to evaluate how such a big and highly energy consuming body as the International Space Station disturbs the surrounding plasma, and how the station itself is charged due to the operation of so many instruments, solar batteries, life supporting devices, etc. Two identical Langmuir electrostatic probes are included in the experiment “Obstanovka”. In this paper the Langmuir probes for “Obstanovka” experiment are described, including the choice of geometry (spherical or cylindrical), a more reliable method for the sweep voltage generation, an adaptive algorithm for the probe’s operation. Special attention is paid to the possibility for remote upgrading of the instrument from the ground using the standard communication channels.