TC11/TC17钛合金线性摩擦焊接头组织与性能

针对航空发动机钛合金整体叶盘的典型材料TC11和TC17开展对异种钛合金线性摩擦焊的研究,其中包括飞边形貌、接头组织及拉伸性能等.研究结果表明:TC11/TC17异种钛合金线性摩擦焊沿振动方向的飞边较长;焊接接头明显分为3个区域:母材、热机械影响区和焊缝区,其中TC11母材为双态组织、TC17母材为网篮组织、热机械影响区的组织沿着受力方向被拉长,焊缝发生了动态再结晶,组织为等轴晶.拉伸测试结果表明:接头的抗拉强度及屈服强度能达到与TC11等强,拉伸试样均断在TC11母材一侧,随着测试温度提高,强度呈线性下降趋势;而断面收缩率均超过TC17母材,随着测试温度提高,变化不明显.     

ARTEMIS Mission Design

The ARTEMIS mission takes two of the five THEMIS spacecraft beyond their prime mission objectives and reuses them to study the Moon and the lunar space environment. Although the spacecraft and fuel resources were tailored to space observations from Earth orbit, sufficient fuel margins, spacecraft capability, and operational flexibility were present that with a circuitous, ballistic, constrained-thrust trajectory, new scientific information could be gleaned from the instruments near the Moon and in lunar orbit. We discuss the challenges of ARTEMIS trajectory design and describe its current implementation to address both heliophysics and planetary science objectives. In particular, we explain the challenges imposed by the constraints of the orbiting hardware and describe the trajectory solutions found in prolonged ballistic flight paths that include multiple lunar approaches, lunar flybys, low-energy trajectory segments, lunar Lissajous orbits, and low-lunar-periapse orbits. We conclude with a discussion of the risks that we took to enable the development and implementation of ARTEMIS.     

影响某型燃机转子轴向力关键因素分析

燃气轮机转子的轴向力是燃机总体设计的重要指标之一。为了研究影响轴向力的因素,针对某型燃机,通过建立轴向力仿真平台,计算不同装机状态燃机的轴向力载荷,并结合大量整机试车与轴向力实测数据,分析影响该载荷的关键因素。研究与实测表明：运行工况、涡轮导向器喉道面积、封严结构等均构成影响轴向力的关键因素;调整封严直径、喉道面积可以大范围地调整转子轴向力,调整封严间隙值能对轴向力进行微小的调整。     

采用多级优化技术进行复合材料结构可靠性优化设计

在可靠性基础上将结构体系可靠性优化设计方法发展至复合材料结构,并采有多级优化技术提出了复合材料结构可靠性优化设计方法。系统级优化以结构总重最小为目标函数,以满足结构体系可靠性指标要求为约束条件;元件级优化以元件可靠度最大为目标函数,以层板或元件重量在一次迭代中保持不变为约束条件,从而导出了相应的优化准则和迭代式。算例表明该方法的效率高、收敛性好,能推广应用于大型复合材料结构。     

退火温度对Al-Mg 合金拉伸性能和显微组织的影响

通过硬度、拉伸性能测试和金相组织观察,研究了不同退火温度对含和不合Sc的Al-Mg合金组织和性能的影响.结果表明:添加Sc明显提高了Al-Mg合金的强度,抑制了合金形变组织的再结晶,高温退火后1570合金中仍弥散分布的Al3( Sc,Zr)粒子质点造成其较高的再结晶温度及拉伸性能.     

具有纳米结构的 VO_2 相变薄膜

采用无机溶胶－凝胶法制备ＶＯ２相变薄膜，该薄膜相变时的电阻（率）突变可达４～５个数量级。并用ＸＲＤ，ＤＳＣ和ＴＧＡ法研究了制膜过程中干凝胶膜的层状非晶纳米结构。通过适当的非晶晶化过程及随后Ｖ２Ｏ５→ＶＯ２转变的真空热处理，可获得带有空洞（ｖｏｉｄ）结构的低密度纳米薄膜，从而使电阻（率）突变特性异常优异     

Algol, Beta Lyrae, and W Serpentis: Some new results for three well studied eclipsing binaries

The properties of the eclipsing binaries Algol, Beta Lyrae, and W Serpentis are discussed and new results are presented. The physical properties of the components of Algol are now well determined. High resolution spectroscopy of the H-alpha feature by Richards et al. and by Gillet et al. and spectroscopy of the ultraviolet resonance lines with the International Ultraviolet Explorer satellite reveal hot gas around the BBV primary. Gas flows also have been detected apparently originating from the low mass, cooler secondary component and flowing toward the hotter star through the Lagrangian L1 point. Analysis of 6 years of multi-bandpass photoelectric photometry of Beta Lyrae indicates that systematic changes in light curves occur with a characteristic period of -275 ± 25 days. These changes may arise from pulsations of the B8II star or from changes in the geometry of the disk component. Hitherto unpublished u, v, b, y, and H-alpha index light curves of W Ser are presented and discussed. W Ser is a very complex binary system that undergoes complicated, large changes in its light curves. The physical properties of W Ser are only poorly known, but it probably contains one component at its Roche surface, rapidly transfering matter to a component which is embedded in a thick, opaque disk. In several respects, W Ser resembles an upscale version of a cataclysmic variable binary system.     

Atomic and molecular hydrogen in interstellar space

This paper reviews the present state of knowledge of the abundances and physical state of interstellar atomic and molecular hydrogen. Much new data in this area have been obtained in recent rocket observations. There have also been new developments as a result of ground-based infrared and 21-cm observations, and theoretical research.Rocket observations of the Lyman- interstellar absorption line of atomic hydrogen indicate that, in many directions in the sky, atomic hydrogen is up to a factor of 10 less abundant than previously indicated by 21-cm emission measurements. In the direction of the Orion Nebula, most of the absorbing gas appears to be concentrated in the near vicinity of the nebula and to have a temperature considerably lower than the average of 100 K obtained from 21-cm emission measurements. Molecular hydrogen appears essentially absent from the general interstellar medium, as confirmed by theoretical studies of photodissociation processes. However, ground-based infrared and 21-cm studies indicate that the hydrogen in dark dust clouds is mostly molecular.     

液体火箭发动机故障特性动态模拟

以某大型泵压式供应系统液体火箭发动机为研究对象, 建立了液体火箭发动机非线性动态数学模型。针对已发生过或可能出现的故障形式, 以阶跃形式输入, 进行了故障状态下动态特性模拟。数值方法用四阶定步长龙格-库塔方法发展而成的自适应变步长龙格-库塔法。计算结果表明, 所建模型较精确合理, 数值方法满足故障模拟的要求。该工作为故障模式提取、监控参数优化选择、基于模型的故障检测与诊断等发动机健康监控问题的研究奠定了基础。      

GPS based onboard and onground orbit operations for small satellites

In extension to common applications such as groundtrack displays and antenna steering, the SGP4 orbit model is proposed for operational orbit determination in small satellite missions. SGP4 is an analytical orbit model for Low-Earth orbiting satellites that is widely used for the propagation of NORAD twoline elements. Twoline elements may hence be generated completely independent of NORAD. Their use as exclusive source of orbital information simplifies the operations concept and reduces mission costs through the extensive use of existing low-cost mission support software. Due to small computer resource requirements of 8–10kByte, the SGP4 model may also be applied for onboard orbit computations making use of e.g. a 80186 processor, thus ensuring full compatibility of ground-based and onboard operations. The proposed approach is particularly suited in combination with a space-borne GPS receiver, were the C/A-code navigation solutions are treated as measurements that are adjusted in a least-squares sense using the SGP4 model. As consequence, inherent drawbacks of the pure navigation solutions such as data gaps and scatter as well as limited velocity accuracy are avoided, while the operational navigation activities are kept at a minimum. The feasibility of the concept is illustrated based on real GPS navigation data from the TOPEX/Poseidon and the MIR space station with an inherent data quality of 50–100 m. It is shown that 3 hours of data within a 4 day period are sufficient to keep the position error within 4 km, that is considered sufficient for most applications.