太阳能飞机翼肋结构拓扑优化设计

太阳能飞机翼肋结构轻薄且数量众多,其结构形式的合理性对于结构减重、机翼刚度设计等具有重要意义。基于现有太阳能飞机翼肋的结构形式,提出一种翼肋拓扑优化设计方法:首先,应用双向渐进结构优化法(BESO),以单元应力为判断指标,对太阳能飞机典型翼肋进行结构拓扑优化;其次,基于拓扑优化结果对翼肋进行结构细节设计;最后,通过有限元计算,验证翼肋的结构强度、刚度和静稳定性。通过本文方法,能够得到太阳能飞机翼肋更为合理的结构布局。     

机载蒸发循环系统结构的稳健性研究

机载蒸发循环系统结构的疲劳寿命易受外界和内部环境的影响,导致无法满足设计要求。采用随机有限元法,参照设计变量和随机变量的变异性,建立机载蒸发循环系统结构疲劳寿命稳健性优化的数学模型;通过引入权因子α,将稳健性优化问题转化为结构疲劳寿命均值和标准差的双目标优化问题。结果表明:合理设置疲劳寿命均值和标准差的权因子,可有效降低设计变量和随机变量对变异的敏感性,进而提高机载蒸发循环系统结构疲劳寿命的稳健性。     

民用飞机不同商载配置对机身着陆载荷的影响分析

重量分布和重心位置是影响起落架和机体地面载荷的重要因素,其中商载是影响全机重心、惯量的最活跃因素。飞机实际运营中,有无穷多种商载分布及装载方案。为了确保机身载荷分析时,不遗漏严重设计情况,同时能大大减少载荷人员的工作量,本文对不同商载配置下的机身着陆载荷进行了研究分析,分析结果表明最大商载情况将构成机身垂直剪力和垂直弯矩的严重情况。因此,在进行机身载荷分析时,必须考虑最大商载情况,而最大燃油情况可以不必考虑。这一结论为今后有针对性的开展民机机身载荷分析提供了数据支持。     

TC18钛合金疲劳断裂过程声发射信号特征分析

声发射技术通过实时监测结构服役过程中发出的声发射信号,判断结构是否出现损伤,是一种重要的在线监测损伤的技术。为了明确TC18钛合金在疲劳试验中产生微裂纹、裂纹扩展及断裂等过程中声发射信号的特性,设计TC18钛合金试验件,进行其疲劳试验并全程采集声发射信号;采用参数分析方法,得到声发射信号在时域、频域方面的参数特征。结果表明:在裂纹萌生及扩展阶段,声发射信号幅值为40~65dB,低于相同条件下铝合金的信号幅值;在200~280kHz频段上,裂纹萌生阶段与后续过程的能量分布存在较大差异。结合上述研究结果,给出TC18钛合金试验件声发射监测的参考原则。     

Magnetar descendants in HMXBs?

We investigate the relation between the pulse and orbital periods in high-mass X-ray binaries (HMXBs), in order to find the candidates of magnetar descendants in HMXBs. We suggest that magnetar descendants can be found among the HMXBs with relatively shorter orbital periods and longer pulse periods.     

Orbital evolution studies of two HMXB pulsars

High mass X-ray binary (HMXB) pulsars are of two types, persistent and transient. 4U1538−52 is a persistent HMXB whose orbit was previously measured to be circular but the RXTE observations revealed an eccentric orbit. We observed this system with RXTE-PCA in August 2003 and our timing analysis supports the eccentric orbit of the system. However, we do not find any evidence for orbital evolution.

Rotational and tidal interactions between the stars of a closed binary system result in apsidal motion which can be measured in systems with eccentric orbit. 4U0115+63 is a Be-transient HMXB whose eccentric orbit was well-determined during its 1978 outburst. We report preliminary results from analysis of data obtained during the 1999 outburst of this source with the RXTE-PCA.     

Keck observations of ROSAT ultra-luminous X-ray source candidates

We present results of optical follow-up observations of candidate ultra-luminous X-ray sources (ULXs). Using Keck optical spectroscopy, 17 of the candidates from the Colbert and Ptak [Colbert, E.J.M., Ptak, A.F. A catalog of candidate intermediate-luminosity X-ray objects. ApJS 143, 25–45, 2002] catalog have been identified; this is one of the largest sets of optical identifications of such objects thus far. Fifteen are background active galactic nuclei (AGN); two are foreground stars in our Galaxy. These findings are consistent with background and foreground object expectations, as derived from log N–log S relations. Also, the results are briefly discussed in terms of the spiral-galaxy/ULX connection.     

分布式计算机技术在飞机非标测控设备中的应用和实现

在研究、分析和总结分布式计算机技术与系统实现的基础上，以苏-27战斗机火控雷达天线部件性能测控系统研制过程为例，详细论述了分布式计算机测控系统的实现模式，介绍了一种先进合理的非标测控设备设计解决方案和快捷、低成本的系统实用集成方案。     

太阳能飞行器能源昼夜闭环仿真分析

以能量为核心，建立太阳能飞行器的获能模型；通过对太阳能飞行器飞行剖面特点的分析，设计飞行过程中各个阶段的飞行方案，并建立相应的耗能模型；考虑目前储能电池技术水平，根据产能和耗能模型，建立储能模型，完成了能源闭环模型的设计；参照Zephyr 7太阳能无人机的结构参数对论文建立的模型进行了仿真分析，获取了飞行过程中能量变化规律，同时对飞行姿态进行优化。结果表明：通过对太阳能飞行器昼夜飞行高度的不同设置以及飞行姿态角的优化，太阳能飞行器可以实现跨昼夜持久飞行。     

Cosmology and GUTs: The matter of the universe

To illustrate the interaction of Grand Unified Theories (GUTs), supersymmetry (SUSY), and cosmology, a worked example is carried out. This example is the dark matter problem, or “What is the dominant matter of the Universe?” It is shown that if GUTs are assumed then the primordial perturbations are probably adiabatic, if inflation is assumed then Ω = 1 and GUTs first name is probably SUSY. If Ω = 1, big bang nucleosynthesis tells us that the bulk of the matter is non-baryonic. SUSY-GUTs gives us some possible candidate inos to which massive neutrinos, axion or planetary mass black holes can be added. These candidates can be classified hot (or warm) or cold types of dark matter. It is shown that hot gives Ω = 1 and naturally gives large scale structure but does not give small scale structure or galaxy formation times, whereas cold gives small scale structure and formation times but cannot easily yield Ω = 1. It is concluded that either a hybrid of both hot and cold or non-random phases for the perturbations may be needed.