On the effect of considering more realistic particle shape and mass parameters in MMOD risk assessments

One of the primary mission risks tracked in the development of all spacecraft is that due to micro-meteoroids and orbital debris (MMOD). Both types of particles, especially those larger than 0.1 mm in diameter, contain sufficient kinetic energy due to their combined mass and velocities to cause serious damage to crew members and spacecraft. The process used to assess MMOD risk consists of three elements: environment, damage prediction, and damage tolerance. Orbital debris risk assessments for the Orion vehicle, as well as the Shuttle, Space Station and other satellites use ballistic limit equations (BLEs) that have been developed using high speed impact test data and results from numerical simulations that have used spherical projectiles. However, spheres are not expected to be a common shape for orbital debris; rather, orbital debris fragments might be better represented by other regular or irregular solids. In this paper we examine the general construction of NASA’s current orbital debris (OD) model, explore the potential variations in orbital debris mass and shape that are possible when using particle characteristic length to define particle size (instead of assuming spherical particles), and, considering specifically the Orion vehicle, perform an orbital debris risk sensitivity study taking into account variations in particle mass and shape as noted above. While the results of the work performed for this study are preliminary, they do show that continuing to use aluminum spheres in spacecraft risk assessments could result in an over-design of its MMOD protection systems. In such a case, the spacecraft could be heavier than needed, could cost more than needed, and could cost more to put into orbit than needed. The results obtained in this study also show the need to incorporate effects of mass and shape in mission risk assessment prior to first flight of any spacecraft as well as the need to continue to develop/refine BLEs so that they more accurately reflect the shape and material density variations inherent to the actual debris environment.     

自由段弹道扰动引力计算的球谐函数极点变换

为提高弹道导弹自由段扰动引力赋值速度,提出了自由段扰动引力计算的球谐函数极点变换一般方法。重点针对轨道动量矩与天球交点为极点及主动段关机点为极点两种情况,推导了考虑侧向偏差和地球旋转修正的扰动引力计算的球谐函数极点变换模型。仿真分析表明:从落点偏差来看,前者扰动引力计算相对误差为1.89%,后者为6.07%,满足诸元和制导精度要求。     

弹道相机水平投影交会测量法的改进及精度分析

介绍弹道相机数据处理的水平投影交会测量法,提出了加权平均水平投影交会测量法,并分析了两种方法的交会精度,得出加权平均水平投影法可显著提高交会精度的结论。     

倒立摆系统的建模与积分滑模控制

在研究了倒立摆系统动力学模型的基础上,提出了一种积分滑模变结构的控制方法。通过设计积分性质的非线性滑模面,可以减少系统静差,提高控制精度,系统鲁棒性能获得了很好的保存。仿真证明,该方法能够在较短时间内实现系统的稳定,提高系统的控制精度,使倒立摆系统具有更高的稳定性和鲁棒性。     

小型弹体转动惯量的测定

阐述了对称式三线摆的结构原理及该摆微角与大角摆动周期的计算方法 ,利用此摆可以测量构件的转动惯量。当 RL <130 、φ0 <6 0°时 ,该装置的测量准确度优于 1%。     

一种基于多点测距信息的复合制导方法

分析探讨了一种用于提高弹道式导弹对目标命中精度的复合制导方案，提出了通过进行多点测距，利用状态转移矩阵方法，来估计导弹落点偏差和末修级起控点飞行状态参数，然后再按照需要的速度进行末修级导引控制的复合制导方案，并通过仿真计算分析论证了该方法的可行性。     

单/双轴预拉载荷对碳纤维复合材料高速冲击性能的影响研究

针对发动机工作时受预载荷的叶片受到外物冲击的情况,设计一种面内单轴及双轴预加载装置,开展单轴与双轴不同大小预拉载荷下碳纤维/环氧树脂复合材料（T700/TDE-86）的高速冲击试验,探究预拉载荷对复合材料抗冲击性能的影响,并结合超声C扫描分析预拉载荷对损伤面积的影响。结果表明：面内初始载荷对复合材料层合板抗冲击性能和分层损伤面积有显著影响;预拉载荷会提高靶板的抗弯刚度,减少靶板吸收的能量,减小弹道极限,且在双轴预拉情况下更明显;弹体击穿靶板后分层损伤面积几乎不变,而预拉载荷会减小分层损伤面积,且在双轴预拉情况下更明显。     

基于层次评估理论的弹道导弹末段突防制导律研究

针对弹道导弹末段突防问题,应用层次性能评估体系,对弹道导弹末段典型突防制导律进行对比分析.并通过对弹道导弹制导精度、弹道导弹最大过载、弹道飞行时间和反导导弹脱靶量以及它们的均值、均方差的重要性和需求性分析,合理设置评估体系的指标及其权值,应用随机仿真分析方法,对比仿真经典比例导引、修正比例导引和变结构比例导引三种突防制导律的性能.仿真结果证明,层次评估理论可以用于弹道导弹末段突防制导律的评估及优选.     

再入体激波层和近尾流热辐射实验研究

本文介绍了在弹道靶设备上对再入速度下模型的热辐射进行的实验研究工作。铝、高硅氧和聚碳酸酯三种材料的模型在速度为4.5～6.0(km/s),压力为600—8000Pa条件下做了实验,在258nm—1100nm光谱范围内完成了九个波段的辐射测量,给出了三种材料模型的辐射光谱分布曲线。结果表明辐射量除了受环境条件影响外,还强烈地依赖于模型材料;由烧蚀产物引起的辐射通量主要在可见光和近红外区(465nm以上)。估算了烧蚀产物引起的辐射加热率,对头部和近尾流辐射通量做了比较。     

基于推力加速度模板的主动段弹道跟踪方法

对弹道导弹的主动段跟踪是导弹防御中重要的环节。针对此问题提出了一种基于推力加速度模板的主动段跟踪算法，该算法需要主动段推力加速度信息支持。给出了一种简捷的推力加速度模板构建方法。利用近常速运动模型描述了导弹运动特性，解决了对导弹发射时间的估计问题和模板概率的递推计算问题，并将该方法应用到空间预警系统中，通过仿真验证了该方法具有较好的识别效果，位置和速度估计误差都接近于CRLB限。