吉林陨石（H5）的冲击压缩线及其意义

在二级轻气炮动高压装置上运用电探针技术测量了具有H群球粒陨石典型代表性的吉林陨石冲击压缩线。当冲击压力>～70GPa时,吉林陨石发生相变,其高压相零压密度为4.425g/cm~3,硅酸盐部分高压相零压密度为4.068g/cm~3。吉林陨石冲击压缩性质的研究结果与地球形成的星子堆积模型(IAB铁陨石+H群球粒陨石)一致。此外,根据陨石或其类似物的冲击压缩线,用阻抗匹配原理计算了主要类型陨石中重要冲击特征形成的最小碰撞速度,揭示了陨石冲击效应形成的动力学条件与空间环境。     

4116航天润滑油摩擦特性的影响因素

采用球盘试验机测定了4116航天润滑油在不同工况下的摩擦因数,尤其成功实现了高低温环境下的测试.应用正交试验设计方法,研究了滚动速度、滑动速度、最大工作压力和入口油温4个因素对润滑油摩擦特性的影响,并绘出各因素对摩擦因数的影响曲线.研究结果表明:滑动速度和滚动速度对摩擦因数有显著影响,入口油温和最大工作压力对摩擦因数影响不显著.摩擦因数随着滑动速度的增加而增加,但是增加的幅度随滑动速度的增加而逐渐减小;随着滚动速度的增加,摩擦因数迅速减小,当滚速高于20m/s时趋于稳定;入口油温低于0℃时,其对摩擦因数有较大影响;随最大工作压力的增加摩擦因数缓慢增加.      

空间伸展机构接触碰撞的动力学分析

本文以子结构离散的柔性多体系统动力学为基础，引入与碰撞有关的约束条件导出了描述碰撞过程的柔性多体系统的动力学方程。通过仿真计算可得到空间伸展机构撞击阶段的时间，构件在碰撞阶段的动力学响应；并从与约束方程相关的Ｌａｇｒａｎｇｅ乘子获得撞击力的变化规律。从而可较全面地描述空间伸展机构整个接触碰撞动力学过程。本文以伸展机构的两个构件碰撞过程的仿真为例详细介绍各种建模方法与计算方法。     

Whipple防护屏弹道极限参数试验

在中国空气动力研究与发展中心FD-18A超高速碰撞靶上进行了Whipple防护屏的超高速撞击试验。弹丸为LY12铝球,撞击速度为4.5km/s,撞击角为0°。通过固定弹丸速度、变弹丸直径、寻找弹丸临界直径的办法获得了该Whipple防护屏在试验条件下的弹道极限参数。试验结果表明速度为4.5km/s时的弹丸临界直径为0.35cm,大于用Christiansen方程预测的0.27cm。     

不同增强体C/C复合材料韧性研究

研究了编织C/C复合材料、针刺C/C复合材料和毡基C/C复合材料室温、高温的断裂韧性,以及3种不同增强体C/C复合材料的冲击韧性。研究发现,C/C复合材料的高温断裂韧性高于室温,其中针刺C/C复合材料的断裂韧性值最高。编织C/C复合材料的抗冲击性能表现出强烈的各向异性,针刺C/C复合材料抗冲击性能优于毡基C/C复合材料。     

基于双量程推力传感器的精确测力技术

针对双量程推力传感器在使用中测试精度低的问题,结合传感器固有特性,开展了传感器动态特性分析及误差补偿方法的研究。通过有限元分析和力锤冲击试验,结合结构分析获得了双量程力传感器等效二自由度和三自由度动力学模型。利用近似求积数值法对冲击力试验输出信号进行补偿,获得了接近标准信号的测试结果,对该补偿方法进行了有效性验证。结果显示:本方法对发动机试验的推力信号进行了补偿,推动了单室双推力发动机推力的精确测量,为双推力发动机的推力测试提供了有效途径。     

空投舱体着陆冲击仿真与分析

针对空投物资方式中物资的安全着陆问题,采用舱体结构对空投救生装备进行缓冲保护.本文在对舱体空投问题进行了力学分析的基础上,采用显式非线性动力学分析有限元软件ANSYS/LS-DYNA对空投舱体着陆冲击进行模拟计算,根据仿真计算所得的舱体在冲击过程中的动态响应,来确定舱体结构设计方案的可行性,体现了设计的先进性.     

Extraterrestrial environmental impact assessments – A foreseeable prerequisite for wise decisions regarding outer space exploration,research and development

Although existing international instruments such as the Outer Space Treaty and Moon Agreement generally express sentiments for minimizing missions' extraterrestrial environmental impacts, they tend to be limited in scope, vague and generally unenforceable. There is no formal structure for assessing how and to what extent we affect those environments, no opportunity for public participation, no uniform protocol for documenting and registering the effects of our actions and no requirement to mitigate adverse impacts or take them into consideration in the decision-making process. Except for precautions limiting forward biological contamination and issues related to Earth satellites, environmental impact analysis, when done at all, remains focused on how missions affect the Earth and near-Earth environments, not how our actions affect the Moon, Mars, Europa, comets and other potential destinations. Extraterrestrial environmental impacts are potentially counterproductive to future space exploration, exploitation and scientific investigations. Clear, consistent and effective international protocols guiding a process for assessing such impacts are warranted. While instruments such as the US National Environmental Policy Act provide legally tested and efficient regulatory models that can guide impact assessment here on Earth, statutory legal frameworks may not work as well in the international environment of outer space. A proposal for industry-driven standards and an environmental code of conduct based, in part, on best management practices are offered for consideration.     

注装梯恩梯(TNT)装药冲击Hugoniot参数的实验测定

本文利用一级轻气炮实验技术，对注装梯恩梯药进行了高应变率下的动态冲击实验，对实验方法进行了改进，设计了一种新型的轻气炮延伸炮管。根据实验数据结果，得到了注装ＴＮＴ装药的冲击Ｈｕｇｏｎｉｏｔ参数。     

Comparison of fragments created by low- and hyper-velocity impacts

This paper summarizes two new satellite impact experiments. The objective of the experiments was to investigate the outcome of low- and hyper-velocity impacts on two identical target satellites. The first experiment was performed at a low-velocity of 1.5 km/s using a 40-g aluminum alloy sphere. The second experiment was performed at a hyper-velocity of 4.4 km/s using a 4-g aluminum alloy sphere. The target satellites were 15 cm × 15 cm × 15 cm in size and 800 g in mass. The ratios of impact energy to target mass for the two experiments were approximately the same. The target satellites were completely fragmented in both experiments, although there were some differences in the characteristics of the fragments. The projectile of the low-velocity impact experiment was partially fragmented while the projectile of the hyper-velocity impact experiment was completely fragmented beyond recognition. To date, approximately 1500 fragments from each impact experiment have been collected for detailed analysis. Each piece has been weighed, measured, and analyzed based on the analytic method used in the NASA Standard Breakup Model (2000 revision). These fragments account for about 95% of the target mass for both impact experiments. Preliminary analysis results will be presented in this paper.