吸热型碳氢燃料RP-3替代模型研究

利用广义对应态法则对吸热型碳氢燃料RP-3的5种替代模型的密度、黏度、导热系数和比定压热容进行了数值计算.计算温度变化范围为300~800K,压力变化范围为3~6MPa.结果表明:不同替代模型均能定性重现RP-3在拟临界温度附近的物性急剧变化;由53%正十一烷,18%正丁基环己烷,29%1,3,5-三甲基苯组成的3组分替代模型在预测RP-3物性上表现最优,相对于实验数据,300~700K内密度相对误差均小于0.08;替代模型的相对分子质量越大,预测的拟临界温度越高,对拟临界温度下物性值的影响无显著规律.      

Nb/Nb5Si3微叠层材料及其制备技术

Nb/Nb5Si3合金是未来最具潜力的超高温结构材料,实现该材料的结构微叠层化是一种新颖的材料设计思路和制备方法.Nb/Nb5Si3微叠层材料是将Nb和Nb5Si3按一定的层间距及层厚比以ABABAB型交互重叠结构形成的多层材料,其几种典型的制备技术包括热压、等离子喷涂、磁控溅射和电子束物理气相沉积(EB-PVD).其中EB-PVD是一种最适合工程应用的Nb/Nb5Si3微叠层材料制备方法,结构和功能复合、纳米化叠层、高韧化工艺是EB-PVD技术制备Nb/Nb5Si3微叠层材料的发展方向.     

飞机维修大纲中的任务转移风险评估方法

以波音737NG飞机维修大纲为例,对其依据MSG—3决断逻辑制定的维修大纲中的任务转移风险进行模糊综合评价。使用模糊理论、层次分析法、熵权法和转移修正因子计算维修大纲中任务转移的风险概率值。结果表明,该值符合FAA和EASA的安全标准,方法可行。     

高性能纤维增强树脂基复合材料3D打印及其应用探索

纤维增强树脂基复合材料具有优异的力学性能,能够实现轻质、高性能结构的制造,但传统的成型工艺过程复杂、成本高,难以实现纤维回收利用,限制了纤维增强树脂基复合材料的广泛应用.3D打印技术是一种新兴的零件成形工艺,将3D打印技术应用于纤维增强树脂基复合材料的制造,为实现复合材料低成本、绿色制造提供了可能性.综述了纤维增强树脂基复合材料3D打印技术研究的发展现状,提出了一种高性能连续纤维增强热塑性复合材料3D打印工艺及其回收再制造策略.     

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.     

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.     

基于PERT网络的航空弹药保障人员优化配置

针对航空弹药保障效率和可靠性要求高的问题,在分析保障流程的计划评审技术（PERT,Program Evaluation and Review Technique）网络图中各工序对任务完工影响程度的基础上,提取了工序关键度指标和重要度指标以及各方案下的按期完工概率,建立了保障人员配置方案评价指标体系,表示为评价函数形式.以基于蒙特卡洛方法的PERT网络仿真为核心,选择在遗传算法进化寻优框架下构建优化模型,该方法不仅得到了最优的保障人员配置方案,而且评估了需要注重的关键工序.算例实验证实了其有效性与实用性.      

高精度UT1-UTC差分预报方法研究

针对卫星导航所需的高精度地球定向参数(EOP)中的UT1-UTC预报问题,提出了基于双差分LS+AR的UT1-UTC参数预报方法。对UT1-UTC观测数据进行跳秒检测、固体地球带谐潮汐项改正,然后对改正后的UT1-UTC数据进行双差分处理,增强数据平稳性;采用最小二乘拟合(LS)与自回归(AR)分析方法对差分处理后的数据进行分析与预报;对预报结果进行逆差分处理与潮汐项改正外推、跳秒恢复,获取高精度的UT1-UTC预报值。通过与国际EOP_PCC预报结果对比表明,UT1-UTC短期预报精度与EOP_PCC较优的预报精度相当,其中1天UT1-UTC预报精度优于0.03ms,优于EOP_PCC预报结果。介绍了北京航天飞行控制中心的UT1-UTC每日例行预报情况。     

A 3NM-64_He added to LARC for Solar Extreme Event studies during solar cycle 24

The Antarctic Laboratory for Cosmic Rays (LARC, acronym for Laboratorio Antartico per i Raggi Cosmici or Laboratorio Antártico para Rayos Cósmicos) operates on King George Island (South Shetlands). Since January 1991 a standard 6NM-64 detector has been recording continuous cosmic ray measurements and several Ground-Level Enhancements have been registered. Here we describe the different phases performed in Italy for the realization of a 3NM-64_³He detector, which started its measurements during the Italian XXII Antarctic Summer Campaign. Data recorded during solar activity cycle 24 will furnish an useful research tool for the next Solar Extreme Events.     

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.