Analysis and control of the compaction force in the composite prepreg tape winding process for rocket motor nozzles

In the process of composite prepreg tape winding, the compaction force could influence the quality of winding products. According to the analysis and experiments, during the winding process of a rocket motor nozzle aft exit cone with a winding angle, there would be an error between the deposition speed of tape layers and the feeding speed of the compaction roller, which could influence the compaction force. Both a lack of compaction and overcompaction related to the feed-ing of the compaction roller could result in defects of winding nozzles. Thus, a flexible winding sys-tem has been developed for rocket motor nozzle winding. In the system, feeding of the compaction roller could be adjusted in real time to achieve an invariable compaction force. According to exper-iments, the force deformation model of the winding tape is a time-varying system. Thus, a forgetting factor recursive least square based parameter estimation proportional-integral-differential (PID) controller has been developed, which could estimate the time-varying parameter and control the compaction force by adjusting the feeding of the compaction roller during the winding process. According to the experimental results, a winding nozzle with fewer voids and a smooth surface could be wounded by the invariable compaction force in the flexible winding system.     

结构系统可靠性及可靠性灵敏度分析的改进子集模拟法

在再生自适应子集模拟(RASS)法的基础上,提出了一种改进的再生自适应子集模拟(MRASS)法以用于结构系统的可靠性及可靠性灵敏度分析。MRASS法继承了RASS法中马尔可夫链再生、延迟拒绝、自适应马尔可夫过程及分量各自采样等优点,并改进了自适应采样过程。MRASS法通过对产生的样本点的接受率与最佳接受率进行比较,有针对性地寻找合适的建议分布方差,提高了抽样的效率。工程算例的数值结果表明:MRASS法相比于RASS法及传统的子集模拟(SS)法,在处理具有高维随机变量、小失效概率及高度非线性特点的结构系统时,有更好的适应性、稳健性及精度。     

三维编织体复合材料空间几何结构的计算机模拟

针对四步方形编织结构,从三维编织工艺和实际的编织过程出发,提出一种单元几何模型,并通过计算机图形建模建立织物的空间几何数学模型,解决了三维编织复合材料内部编织结构分析困难的问题。该模型以携纱器循环一周返回到起始位置所形成的纱线编织结构作为单元,系统分析编织过程中纱线的空间运动规律,保证纤维束的连续性和材料整体结构的完整性。对每根纱线,选取它在编织体各个区域内合适的控制点,过这些控制点拟合成三次样条曲线,以此模拟纱线的空间结构中心线,从而能够方便直观地观察到各纱线具体走向。最后得到纱线和编织体的结构,从而便于下一步进行编织体复合材料力学性能的有限元分析。     

无隙锥形旋流器燃烧室中流场分叉现象成因的探讨

本文以实验为依据, 结合分析和推理, 对在无隙锥形旋流器燃烧室中发生的流场分叉现象的成因进行了初步探讨。      

High energy radiation from the direction of the galactic black hole Sgr A

X-ray observations indicate that the Galactic black hole Sgr A^∗ is inactive now, however, we suggest that Sgr A^∗ can become active when a captured star is tidally disrupted and matter is accreted into the black hole. Consequently the Galactic black hole could be a powerful source of relativistic protons with a characteristic energy ∼10⁵² erg per capture. The diffuse GeV and TeV γ-rays emitted in the direction of the Galactic Center (GC) are the direct consequences of p–p collisions of such relativistic protons ejected by very recent capture events occurred ?10⁵ yr ago. On the other hand, the extended electron-positron annihilation line emission observed from GC is a phenomenon related to a large population of thermalized positrons, which are produced, cooled down and accumulated through hundreds of past capture events during a period of ∼10⁷ yr. In addition to explaining GeV, TeV and 511 keV annihilation emissions we also estimate the photon flux of several MeV resulting from in-flight annihilation process.     

在MATLAB中模拟平稳随机过程

叙述了平稳随机过程理论的基本定义,以及运用实谱分解方法模拟平稳随机过程的原理.全面分析了在微型计算机上使用MATLAB软件模拟平稳随机过程的注意事项,包括:信号源的选取,仿真算法和相应参数的设置,由于功率谱密度的不同定义而需要进行相应的调整等3个方面.结合大气紊流和航空母舰在海上的随机运动的2个实例,给出了在MATLAB中模拟类似过程的方法,并对结果进行了检验.分析表明在MATLAB中能够较好地模拟平稳随机过程.      

Interstellar hydrogen bonding

This paper reports the first extensive study of the existence and effects of interstellar hydrogen bonding. The reactions that occur on the surface of the interstellar dust grains are the dominant processes by which interstellar molecules are formed. Water molecules constitute about 70% of the interstellar ice. These water molecules serve as the platform for hydrogen bonding. High level quantum chemical simulations for the hydrogen bond interaction between 20 interstellar molecules (known and possible) and water are carried out using different ab-intio methods. It is evident that if the formation of these species is mainly governed by the ice phase reactions, there is a direct correlation between the binding energies of these complexes and the gas phase abundances of these interstellar molecules. Interstellar hydrogen bonding may cause lower gas abundance of the complex organic molecules (COMs) at the low temperature. From these results, ketenes whose less stable isomers that are more strongly bonded to the surface of the interstellar dust grains have been observed are proposed as suitable candidates for astronomical observations.     

非线性动力Alfven波的演化

本文讨论了非线性动力Alfven波在1＞＞β＞＞me／mi条件下形成孤子解的限制条件，表明只有亚Alfven速度才能形成压缩型孤子．由动力Alfven波孤子和湍流产生的极大纵向电子速度不会超过本底电子热速度，但由此产生的纵向电场在小尺度范围可以很强，这可能对太阳风的能量传输与粒子加速产生一定影响．     

一种新型水溶性芯模的制备和性能

概述了金属模具不易脱模的形状复杂的复合材料结构件成型中遇到的工艺技术难题,着重对水溶性芯模的制备工艺特点和性能进行了研究,并将所制得的水溶性芯模成功的用于树脂基复合材料结构件的制造中。结果表明,水溶性芯模的各项性能满足复杂异型复合材料结构件制造的要求。     

基于HMDP的无人机三维路径规划

路径规划是UAV(Unmanned Aerial Vehicle)自主飞行的重要保障.初步建立了基于MDP(Markov Decision Processes)的全局路径规划模型,把UAV的路径规划看作是给定环境模型和奖惩原则的情况下,寻求最优策略的问题;为解决算法时空开销大、UAV航向改变频繁的缺点,提出一种基于状态聚类方法的HMDP(Hierarchical Markov Decision Processes)模型,并将其拓展到三维规划中.仿真实验证明:这种简单的规划模型可以有效解决UAV的三维全局路径规划问题,为其在实际飞行中的局部规划奠定了基础.