PIP工艺对2D高硅氧/甲基硅树脂复合材料结构与性能的影响

研究了不同浸渍工艺对2D高硅氧织物增强甲基硅树脂复合材料结构与性能的影响。结果表明,复合材料的密度及抗氧化性随着浸渍循环次数和热裂解温度的增加而增加;当热裂解温度不高于400℃时,复合材料仍具有较好的假塑性;但当热裂解温度高于400℃时,复合材料表现为典型的脆性断裂。当浸渍过程中热裂解温度为400℃、循环次数为2次时,500℃热处理20 m in的复合材料的室温弯曲强度最高,为49.8 MPa,比未处理的提高了150%。     

CM2程控稳流电源电流稳定性的自动化测试

文章将零磁通电流互感器技术应用到了大电流稳定性测试中,从而解决了CM2航天器磁环境模拟设备中的程控稳流电源输出电流稳定性测试的难题,稳定性指标高达10-5/8h。文章简述了零磁通电流互感器技术的基本原理,介绍了采用零磁通电流互感器技术对CM2程控稳流电源电流稳定性进行自动测试的方法,分析了影响大电流稳定性现场自动测试的因素并提出了相应解决方案。     

基于拟平均根数之差的航天器相对导航UKF滤波算法

针对星载雷达数据(距离及其变率、角度及其变率),推导了以相对拟平均根数为状态变量的星间相对导航UKF滤波算法.建立了包含J2一阶长期项摄动的状态转移方程.推导了无奇点的相对拟平均根数与相对位置速度之间的转换矩阵,并分析了坐标变换中被忽略的二阶项的影响,对转换矩阵的精度进行了有效补偿.提出以相对位置速度为直接观测量,设计了具有自调整功能的测量误差协方差阵,避免了建立观测方程时状态量对直接观测量的繁琐偏导计算.仿真结果证明了该算法的有效性.     

基于有限时间H2性能指标的导弹机动突防策略设计

针对导弹机动突防策略设计中存在的对主要性能指标缺乏综合评价手段的问题,基于有限时间H2性能指标,给出系统性能分析与设计的准则,综合考虑脱靶量和机动消耗的能量,设计了脱靶量/能量最优的机动形式。考虑拦截器制导律信息存在不确定性,提出了有限时间鲁棒H2性能分析方法与有限时间鲁棒H2保性能控制准则,设计了在拦截器制导律信息存在不确定性时的保性能机动。结果表明,突防导弹在拦截末段的大幅度机动最为有效,能够以较小的能量代价换取较大的拦截脱靶量。
     

弹性体运载火箭建模及控制器设计

考虑运载火箭飞行过程中的弹性振动特性,对运载火箭进行全量动力学建模以及控制器设计。首先将运载火箭考虑为一维梁模型并建立全量动力学模型,分别引入自适应滤波姿态控制算法和H_2范数鲁棒增益调度控制算法设计控制器。仿真结果表明:在考虑舵机非线性情况下两种控制方法均能够满足精度要求,在具有较大外部扰动情况下,鲁棒增益调度控制算法相较于自适应滤波算法具有较强的鲁棒性。     

基于微观图像及内聚力模型的复合材料裂纹扩展模拟

为研究材料微观结构及晶界强度对材料力学性能的影响,在晶界处引入内聚力单元模型,模拟晶间破坏过程。以ZrB_2-SiC复合材料为研究对象,将其扫描的微观结构图片进行矢量化处理,并导入ABAQUS有限元软件中建立模型,同时在其晶界处,设置内聚力单元模拟晶界破坏过程。通过改变Zr B2与Si C相界面强度,得到了晶界及材料不均匀对材料应力分布及裂纹扩展的影响。结果表明,由于晶界的存在,材料内部出现应力分布不均匀现象并产生应力集中。随着晶界强度的改变,裂纹起始位置及扩展方向发生改变,且裂纹沿低强度的界面进行扩展。随着ZrB_2-SiC界面强度增大,材料的强度提高,拉伸模量不变。     

Effects of in-track maneuver on Sun illumination conditions of near-circular low Earth orbits

By developing approximate analytical models considering the J₂ perturbation, the effects of an in-track maneuver on the orbital Sun illumination conditions of near-circular low Earth orbits are analyzed. First, two approximate models for the variations in orbital sunshine angles are developed, one for variations at a given time and the other for variations at a given argument of latitude. Next, two approximate models for variations in orbital arc in Earth shadow are developed, one considers the small eccentricity and the other uses the zero eccentricity. Finally, the developed approximate models are applied to analyzing the Sun illumination conditions of a typical in-track maneuver mission on a near-circular low Earth orbit. From the results obtained, three major conclusions can be drawn. First, the variations in orbital sunshine angles at a given time may reach tens of degrees when the drifting time reaches hundreds of orbital periods, and the approximate model for that situation cannot effectively approach the numerical results. Second, the variations in orbital sunshine angles for any given argument of latitude are only a couple of degrees even when the drifting time reaches 500 orbital periods, and the approximation model developed can effectively approach the numerical results. Third, for variations in orbital arc in Earth shadow, the approximate model considering the small eccentricity has simple expressions and can effectively approach the numerical results; in contrast, the approximate model using the zero eccentricity has relatively worse precision.     

Evolution of periodic orbits near the Lagrangian point L2

A study of the evolution of the periodic and the quasi-periodic orbits near the Lagrangian point L₂, which is located to the right of the smaller primary on the line joining the primaries and whose distance from the more massive primary is greater than the distance between the primaries, in the framework of restricted three-body problem for the Sun–Jupiter, Earth–Moon (relatively large mass ratio) and Saturn–Titan (relatively small mass ratio) systems is made. Two families of periodic orbits around the smaller primary are identified using the Poincaré surface of section method – family I (initially elliptical, gradually becomes egg-shaped with the increase in the Jacobi constant C and elongated towards the more massive primary) and family II (initially egg-shaped orbits elongated towards L₂ and gradually becomes elliptical with the increase in C). The family I in the Sun–Jupiter and Saturn–Titan systems contains two separatrix caused by third-order and fourth-order resonances, while the Earth–Moon system has only one separatrix which is caused by third-order resonances. Also in the Sun–Jupiter and the Saturn–Titan systems, family I merge with family II, around Jacobian constant 3.0393 and 3.0163, respectively, while in the Earth–Moon system, family II evolves separately from two different branches. The two branches merge at C = 3.184515. In the Earth–Moon system, the family II contains a separatrix due to third-order resonances which is absent in the other two systems.     

基于I~2C总线的CPU温度监控系统

随着高性能、高功耗器件在嵌入式领域中广泛应用,温度监控已成为高可靠嵌入式领域研究的热点,采用ADI公司的测温电路ADT7461设计了面向高性能PowerPC处理器的温度监控系统。介绍了ADT7461芯片的功能原理,描述了整个硬件电路的结构。在软件部分阐述了I2C总线协议以及基于I2C总线协议实现的ADT7461寄存器读/写基本操作,针对应用中会面临的实际问题给出了具体解决方法。设计方法对于同类温度监控系统设计有一定的参考意义。     

Comparison of peak characteristics of F2 ionospheric layer over Tehran region at a low solar activity period with IRI-2001 and IRI-2007 models predictions

In the present work values of peak electron density (NmF2) and height of F2 ionospheric layer (hmF2) over Tehran region at a low solar activity period are compared with the predictions of the International Reference Ionosphere models (IRI-2001 and IRI-2007). Data measured by a digital ionosonde at the ionospheric station of the Institute of Geophysics, University of Tehran from July 2006 to June 2007 are used to perform the calculations. Formulations proposed by  and  are utilized to calculate the hmF2. The International Union of Radio Science (URSI) and International Radio Consultative Committee (CCIR) options are employed to run the IRI-2001 and IRI-2007 models. Results show that both IRI-2007 and IRI-2001 can successfully predict the NmF2 and hmF2 over Tehran region. In addition, the study shows that predictions of IRI-2007 model with CCIR coefficient has closer values to the observations. Furthermore, it is found that the monthly average of the percentage deviation between the IRI models predictions and the values of hmF2 and NmF2 parameters are less than 10% and 21%, respectively.