Z-pins增强陶瓷基复合材料层间Ⅰ型开裂性能预测

基于Z-pins增强陶瓷基复合材料层间Ⅰ型断裂韧性的试验结果、Z-pins增强机理,提出了Z-pins拔出的单线性软化模型.重点考虑了Z-pins直径范围内拔出位移的不一致性,在简单双悬臂梁（DCB）理论的基础上,获得了Z-pins增强陶瓷基复合材料层间Ⅰ型开裂性能的分析预测模型,预测结果与试验结果吻合较好.在此基础上,采用预测模型获得了不同Z-pins直径、裂纹长度下的裂尖能量释放率,并与理想弹簧元法进行了比较.结果表明:当裂尖靠近Z-pins时,随着Z-pins直径增大,两种方法所得的裂尖能释放率的差异逐渐增大,但总体来说差异的量级很小;随着裂纹长度的增加,裂尖逐渐远离Z-pins,两种方法所得的裂尖能释放率的存在较大的差异,不能忽略Z-pins直径范围内拔出位移不一的影响.      

陶瓷基复合材料基体裂纹偏转能量释放率研究

采用虚裂纹闭合技术(VCCT)计算了基体裂纹在界面处不同传播路径的能量释放率,并结合基于能量释放率的裂纹偏转准则对陶瓷基复合材料基体裂纹偏转进行了研究.计算了弹性错配参数α和β、基体裂纹扩展长度a、基体裂纹相对扩展长度ad/ap对裂纹偏转的影响,并将VCCT计算结果与积分法的计算结果进行比较.结果表明:VCCT能够准确计算基体裂纹扩展时的能量释放率,计算结果可为研究陶瓷基复合材料失效机制提供一定参考.      

多种材料人工脱粘应力场分析

采有网格自动生成技术，给出了考虑多种材料结构的人工脱粘层前缘附近推进剂／衬层界面较为合理的疏密平滑过渡的计算网格，对整个药柱尤其是对头部人工脱粘前缘附近进行了详细的有限元计算，得出了与实际情况接近的有限元诸模型析应力，应变场，此外，还考虑不同模量绝热层（人工脱粘层）和衬层对人工脱粘层前缘附近推进剂／衬层界面应力的影响。     

基于实时数据库技术的空间环境 模拟器数据管理平台

针对现有空间环境模拟器试验数据统一管理和试验设备集中监控的难题,文章提出了一种基于实时数据库技术的试验数据管理平台,首次在国内系统级空间环境模拟器研制中引入实时数据库概念,并成功应用于KM7空间环境模拟器中。该数据管理平台将KM7设备各分系统的关键数据信息进行分散采集,统一存储和调用,并通过网络发布。     

新型柔索式杆束结构压紧释放装置

针对空间机械臂、空间可展开天线等空间机构在收拢状态的杆束结构压紧与释放问题,提出一种基于柔性索捆绑压紧与热刀释放的新型压紧释放装置。建立了柔索式压紧释放装置锁紧状态的力学模型,分析了静态压紧和考虑惯性载荷情况下的绳索预紧力变化情况,得到了满足可靠压紧的绳索预紧力设计值。基于质量和刚度等效,设计了机械臂杆束结构力学等效件,并进行了正弦与随机振动力学试验。试验结果验证了所设计的柔索式杆束结构压紧释放装置的可行性,并可以推广到具有复杂包络的杆束结构压紧释放中。     

空间模拟碎片释放装置技术方案

为配合空间碎片主动清除技术的演示验证试验,提出了一种空间模拟碎片释放装置的技术方案:由模拟碎片及分离解锁装置组成。模拟碎片不具备任何合作特征,最初通过压紧杆与分离解锁装置相连,释放时由火工切割器切断压紧杆,模拟碎片在压缩弹簧的驱动下与分离解锁装置分离。最后,通过静载、模态、运动特性分析及分离解锁试验验证了该释放装置设计的正确性。     

提高航班签派或放行中的天气评估能力

在实际航班运行中,导致返航备降的各类原因里,天气因素占首位,因此,为保证航班安全、正常地运行,飞行签派员务必在航班签派或放行中做好天气的评估工作。     

Mathematical description of the NaK model for MASTER-2005

The release of NaK droplets has been modeled for the new version of the European Meteoroid and Space Debris Terrestrial Environment Reference model MASTER-2005. Previously published versions of the model have been revised. The parameters of the model are introduced and discussed. NaK droplets consist of eutectic sodium–potassium alloy and have been released during RORSAT reactor core ejections. They contributed to the space debris environment in the centimeter and millimeter size regime. Sixteen nuclear powered RORSATs launched between 1980 and 1988 activated a reactor core ejection system in Sufficiently High Orbits (SHO), mostly between 900 and 950 km altitude. The core ejection caused an opening of the primary coolant circuit. The liquid coolant has been released into space during these core ejections. The outflow is considered as a discrete event for each of the sixteen core ejections in total. The NaK coolant has been forming droplets up to a diameter of 5.5 cm. NaK releases are restricted to a very narrow region near 65° inclination. This paper gives the parameters of the NaK release model as it is implemented in MASTER-2005. The quantitative values of all model parameters including characteristic diameter and uniformity parameter are presented. The ratio of the characteristic droplet size to the orifice diameter is discussed. It is estimated that altogether 128 kg of NaK-78 (8 kg per RORSAT) was released on orbit. Simulation runs show that there are still 45,000 droplets with a total mass of 97 kg in orbit at the reference epoch 1 May 2005, whereas the smallest droplet has a diameter of 5 mm. Results of orbit propagation simulation runs are presented in terms of spatial density.     

牵制缓释放过程中火箭动力响应特性分析

为研究运载火箭在牵制缓释放过程中的结构动力响应特性,将牵制缓释放发射过程依次分为静态竖立、点火牵制和缓释放三个阶段进行计算。运用MSC.Patran有限元程序的场功能来实现上一阶段的全部计算结果场向下一阶段初始条件场的传递,运用MSC.Nastran有限元程序的非线性弹簧单元的非线性位移载荷函数功能来模拟运载火箭缓释放过程中的缓释力,实现运载火箭牵制缓释放过程结构动力响应的数值计算,并对比分析运载火箭几种常用发射释放方式的结构动力响应特性。结果表明:采用牵制缓释放系统可有效减小运载火箭释放时所受冲击载荷,减小运载火箭全箭结构动力响应。     

Simulation and analysis of chemical release in the ionosphere

Ionospheric inhomogeneous plasma produced by single point chemical release has simple space-time structure, and cannot impact radio wave frequencies higher than Very High Frequency (VHF) band. In order to produce more complicated ionospheric plasma perturbation structure and trigger instabilities phenomena, multiple-point chemical release scheme is presented in this paper. The effects of chemical release on low latitude ionospheric plasma are estimated by linear instability growth rate theory that high growth rate represents high irregularities, ionospheric scintillation occurrence probability and high scintillation intension in scintillation duration. The amplitude scintillations and the phase scintillations of 150?MHz, 400?MHz, and 1000?MHz are calculated based on the theory of multiple phase screen (MPS), when they propagate through the disturbed area.