连续型和非连续型蜂窝芯材的共振吸声结构性能研究

以芳纶纸蜂窝、内嵌树脂隔板和微穿孔面板为原料,制备了连续和非连续双自由度共振吸声结构,对两种共振吸声结构的力学性能和吸声系数进行对比研究。结果表明：连续蜂窝芯材所制备共振吸声结构的压缩和拉伸性能高于非连续型共振吸声结构,其中非稳定型压缩强度和拉伸强度高19%,稳定型压缩强度高32%,稳定型压缩模量高43%,剪切性能基本相当;两层蜂窝芯材容易出现孔格错位（非连续型共振吸声结构）,引起错位区域的微孔堵塞,使该结构的共振吸收峰与理论值出现较大差异。     

星图匹配制导中的关键技术

为了提高新一代弹道导弹的快速、机动反击能力和射击精度，采用星光，惯性组合制导足最佳的选择。本论文给出了基于双星敏感器的、星图匹配制导系统的关键技术。提出了根据弹道设计导航星表．极大地简化了弹载星表；提出了一种适用于星光制导的凸多边形箅法，合理地减少了匹配的星对角距数目。这两项技术保证了星图匹配制导技术的实用性。提出了一种分离初始定位、定向误差及平台漂移误差方法。采用凸多边形的星图识别算法可同时获得多颗星的瞬时位置，结合恒星在像平面的位置可解算导弹在赤道惯性系和发射点惯性系的三轴姿态，最后，给出了导弹初始定位、定向误差的数学表达式。仿真结果表明了该方法的有效性。     

基于CMOS APS的星敏感器光学系统参数确定

基于CMOS APS图象传感器的星敏感器是适应航天技术的发展而产生的新一代姿态敏感器。确定光斑形状和大小、光学系统有效通光孔径、视场和焦距等参数是进行星敏感器光学设计的前提。本文基于选定的CMOS APS图象传感器分别对这些参数进行了分析和计算。确定光斑形状和大小的依据是，减小由于探测器像元对光斑能量分布的采样导致点扩散函数变形，从而引起的利用亚像元技术求星像中心的计算误差。光学系统的有效通光孔径与星敏感器所能探测到的极限星等有关，通过从目标辐射特性直到探测器响应的能量计算可以确定孔径的大小。确定视场和焦距首先要满足星敏感器实现全天自主星图识别所需的导航星捕获概率，其次要考虑与之相关的误差。     

铅化合物在双基推进剂燃烧过程的作用机理

本文提出了铅化合物催化双基推进剂燃烧的反应历程。充分说明这类化合物是最终通过提高燃烧表面处嘶嘶区温度梯度提高燃速的。本文还提出了“铅化合物有通过增加燃烧表面上碳质物量增加燃速的一面,还有通过减少碳质物抑制燃速增加的一面”这一新的论点及抑制碳质物增加的反应并阐明了压力对这种抑制能力的影响。最后根据本文提出的作用机理及传热原理圆满解释了超速、平平和/或麦撒效应。     

单星-星光制导方案

从原理上论述星跟踪器捷联安装的单星－星光制导原理，推导利用星光信息来修正导弹团初始定位定向误差引起落点偏差的数据处理方法、公式，对两种主要的误差源进行了数学仿真计算，结合仿真试验分析了单星方案的可行性。     

捷联星光制导仿真方法研究

捷联星光制导方案是把星跟踪器安装在平台基座上，利用星跟踪器和平台框架角的测量信息解算出因初始定位定向误差引起导弹的落点偏差，由末助推控制系统完成弹道修正。有关捷联星光制导方案的地面仿真原理、方法、组成，选星及大气修正计算原则、地球旋转影响在本文中作了论述，并给出仿真原理框图、硬件设备组成和功能、接口要求以及系统工作程序框图。     

浅谈内部控制制度的建立和实施

内部控制制度是现代管理工作的一个重要组成部分。本文指出了要实现内部控制制度的目标，应建立和实施管理控制和会计控制。     

Modeling Pulsar Wind Nebulae

In the last few years, new observations by CHANDRA and XMM have shown that Pulsar Wind Nebulae present complex but similar inner features, with the presence of axisymmetric rings and jets, which are generally referred to as a jet-torus structure. Due to the rapid growth in accuracy and robustness of numerical schemes for relativistic fluid-dynamics, it is now possible to model the flow and magnetic structure of the relativistic plasma responsible for the emission. Recent results have clarified how the jet and rings are formed, suggesting that the morphology is strongly related to the wind properties, so that, in principle, it is possible to infer the conditions in the unshocked wind from the nebular emission. I will review here the current status in the modeling of Pulsar Wind Nebulae, and, in particular, how numerical simulations have increased our understanding of the flow structure, observed emission, polarization and spectral properties. I will also point to possible future developments of the present models.     

Kink-like mode of a double gradient instability in a compressible plasma current sheet

A linear MHD instability of the electric current sheet, characterized by a small normal magnetic field component, varying along the sheet, is investigated. The tangential magnetic field component is modeled by a hyperbolic function, describing Harris-like variations of the field across the sheet. For this problem, which is formulated in a 3D domain, the conventional compressible ideal MHD equations are applied. By assuming Fourier harmonics along the electric current, the linearized 3D equations are reduced to 2D ones. A finite difference numerical scheme is applied to examine the time evolution of small initial perturbations of the plasma parameters. This work is an extended numerical study of the so called “double gradient instability”, – a possible candidate for the explanation of flapping oscillations in the magnetotail current sheet, which has been analyzed previously in the framework of a simplified analytical approach for an incompressible plasma. The dispersion curve is obtained for the kink-like mode of the instability. It is shown that this curve demonstrates a quantitative agreement with the previous analytical result. The development of the instability is investigated also for various enhanced values of the normal magnetic field component. It is found that the characteristic values of the growth rate of the instability shows a linear dependence on the square root of the parameter, which scales uniformly the normal component of the magnetic field in the current sheet.     

分级时效工艺对1420Al—Li合金组织与性能的影响

研究了分级时效工艺对1420Al-Li合金组织与性能的影响，试验结果表明：经70℃／12h＋120℃／4－10h工艺分级时效处理可使1420Al-Li合金的综合力学性能得到显著的提高；分级时效工艺使1420Al-Li合金析出的δ‘相粒子分布均匀、尺寸细小。