航空装备修理工厂质量竞争力评价体系研究

目前,国内缺少一套科学、系统的适用于飞机、发动机和导弹等航空装备修理工厂的质量竞争力评价体系。运用系统工程理论和过程分析方法,从质量体系能力、质量支持能力、质量运行能力和质量绩效能力四个方面构建涵盖19项二级、60项三级指标的质量竞争力评价指标体系;提出一种基于G1专家组合多重相关赋权的评价方法,全面综合决策者或专家意愿,形成一套标准化的权重系数集;依据评价准则,采用专家打分、模糊评价的方式对航空装备修理工厂质量竞争力进行评价,并作进一步分析。结果表明:该指标体系合理,评价方法可行,对航空装备修理工厂提高自身质量竞争力具有一定的指导和借鉴意义。     

基于DBN的不均衡样本驱动民航发动机故障诊断

在结合深度置信网络(DBN)、采样与集成技术的基础上,提出了基于不均衡样本驱动的民航发动机故障诊断模型。该模型通过分析民航发动机历史飞行数据,利用DBN提取性能参数中的内部特征,利用采样技术将不均衡样本均衡化,采用集成技术进行故障分类。将该模型应用到CFM56-7B系列发动机历史飞行数据,实验结果表明:与常用故障诊断方法相比,该模型的准确率高达0.996,AUC值高达0.948,可以有效处理民航发动机样本高维、不均衡问题。      

基于L_1自适应的超低空空投抗侧风控制律设计

针对超低空空投过程中侧风干扰与装备投放过程相耦合,影响载机飞行安全和空投任务的完成等问题,提出了基于L_1自适应的控制律设计方法。利用最优控制对系统线性部分做状态反馈并确定匹配参考模型,在此基础上,考虑系统的匹配和非匹配不确定性,设计L_1自适应控制器实现姿态保持,结合外环PID侧向轨迹控制器实现对航迹的稳定和保持。仿真结果表明,控制器具有优良的控制性能,对复杂侧风干扰和系统非线性不确定性具有很强的鲁棒性,且在高自适应增益下能有效抑制输入信号高频抖振。     

扩散连接界面缺陷对Ti-6Al-4V合金力学性能的影响

研究了φ4mm与φ2mm的扩散连接界面缺陷对Ti-6Al-4V合金力学性能的影响。当拉伸载荷方向与缺陷平面平行时,材料的强度与塑性与无缺陷材料相当,这是由于此类缺陷对样品受力截面的面积几乎没有影响。含有φ4mm缺陷试样的拉压疲劳寿命展现出很大的分散性,界面缺陷并未成为裂纹萌生的唯一位置。从表面起裂的样品均处于高寿命区域,而绝大部分从缺陷处起裂的样品均落于低寿命区域。有限元分析表明,当缺陷位于中心位置时其引起的应力集中较小,应力分布梯度较小;缺陷位于边缘位置时,应力集中效应增大。     

不同冶炼工艺对1Cr18Ni10Ti钢夹杂物的影响

通过试验研究了1Cr18Ni10Ti不锈钢的4种冶炼工艺:真空感应+电渣重熔、真空感应(陶瓷过滤器)、真空感应(陶瓷过滤器)+电渣重熔、真空感应+真空自耗,得到钢锭中夹杂物的种类、大小以及数量的变化.对比试验结果可知,采用真空感应(陶瓷过滤器)冶炼工艺与真空感应+真空自耗之后的钢锭的夹杂物水平相当,D类夹杂物数量最少,大颗粒夹杂物占比也最小.     

Balloon altitude studies of southern hemisphere hard X-ray sources by the Imperial College-University of Tasmania-INPE collaboration

Hard X-ray balloon altitude measurements with a 1600 cm² phoswich array are described. Data from observations on Sco X-1, GX1+4, GX5−1, Nova Oph. 1977, SMC X-1, SS433, IC 4329A and MR 2251-178 are presented. The role of Comptonisation in X-ray production for Sco X-1 and GX1+4 is discussed.     

Orbital phase spectroscopy of four high mass X-ray binary pulsars to study the stellar wind of the companion

Our work focuses on a comprehensive orbital phase-dependent spectroscopy of the four High Mass X-ray Binary Pulsars (HMXBPs) 4U 1538-52, GX 301-2, OAO 1657-415 and Vela X-1. We hereby report the measurements of the variation of the absorption column density and iron-line flux along with other spectral parameters over the binary orbit for the above-mentioned HMXBPs in elliptical orbits, as observed with the Rossi X-ray Timing Explorer (RXTE) and the BeppoSAX satellites. A spherically symmetric wind profile was used as a model to compare the observed column density variations. Out of the four pulsars, only in 4U 1538-52, we find the model having a reasonable corroboration with the observations, whereas in the remaining three the stellar wind seems to be clumpy and a smooth symmetric stellar wind model appears to be quite inadequate in explaining the data. Moreover, in GX 301-2, neither the presence of a disk nor a gas stream from the companion was validated. Furthermore, the spectral results obtained in the case of OAO 1657-415 and Vela X-1 were more or less similar to that of GX 301-2.     

A Revisit of the Phobos Events

The magnetic field disturbances detected by the Phobos-2 spacecraft in 1989 have been suggested to be caused by a ring of dust and/or gas emitted from the Martian moon, Phobos. The physical nature of these ``Phobos events' is examined using results from related investigations over the last twenty years. It is concluded that there is no clear evidence at present to support the association of magnetic field disturbances in the solar wind with Phobos. The situation will be further clarified taking advantage of the multi-spacecraft observations of the Yinghuo-1(YH-1), Mars Express and MAVEN missions beginning in 2012. It is expected that many novel features of solar wind interaction with Phobos (and possibly also Deimos) itself will also be revealed.      

New results and questions of lunar exploration from SELENE,Chang’E-1, Chandrayaan-1 and LRO/LCROSS

The moon has longstanding questions such as lunar environments, origin, formation and evolution, magnetization of crustal rocks, internal structure and possible life. The recent lunar missions, e.g., SELenological and ENgineering Explorer “KAGUYA” (SELENE), Chang’E-1, Chandrayaan-1, and Lunar Reconnaissance Orbiter/Lunar CRater Observation and Sensing Satellite (LRO/LCROSS), have provided new opportunities to explore and understand these issues. In this paper, we reviewed and presented the results and findings in the fields of lunar gravity, magnetic field, atmosphere, surface geomorphology and compositional variations, volcano, craters, internal structure, water and life science from new lunar exploration missions. In addition, the new objectives and scientific questions on lunar explorations in near future are presented and discussed.     

中俄联合火星电离层星-星掩星探测

中俄联合火星星-星掩星探测是人类首次在火星空间环境进行此类的联合试验。用于探测火星电离层的星-星掩星技术较以前星地间的探测技术相比,有可接收高信噪比信号,反演精度高,可探测火星上太阳天顶角大于43°,或者小于138°的区域电离层等优点。本文介绍了中俄联合火星星-星掩星探测方案、基本原理,给出了主要技术指标、地面模拟测试结果。