空间相机中与大口径透镜有关的结构设计分析

某空间相机镜头在光学设计时，因透过率、吸收率等原因，为了满足光学系统要求，经过各方面平衡后，其中有一片透镜比正常径厚比设计的偏薄些。在镜头总体结构设计时，单独对该镜片及与之相配的结构件进行了有限元分析和实验检测，发现不同的结构形式对镜片面形影响不同。为了解决这一问题，在实验中进行了探讨，以保证整个相机系统满足空间相机的实用要求。     

氨电弧喷射推力器实验和数值研究

为了证实氨电弧喷射推力器良好的工作性能，对其进行了系统的实验和数值研究。在实验研究中建立了高真空实验系统、先进的小推力测量系统和恒定电流控制系统，在数值研究中采用二阶精度无波动、无自由参数的耗散差分格式(NND格式)数值求解耦合电磁源项的扩展N-S方程组。通过实验获得了不同结构尺寸的推力器不同工作条件下的工作性能，通过数值模拟给出了推力器的流场结构，预计了其推力、比冲和推进效率。研究结果表明，氨电弧喷射推力器工作性能良好，能够担负一定的空间应用任务。     

The Brazilian scientific microsatellite SACI-1

The National Space Research Institute (INPE) is developing the first Brazilian Scientific Microsatellite (SACI-1) based on the vanguard technology and on the experience acquired through projects developed by Brazilian Space Program. The SACI-1 is a 750km polar orbit satellite. The spacecraft will combine spin stabilization with geomagnetic control and has a total mass of 60 kg. The overall dimensions are 640×470×470 mm. The SACI-1 satellite shall be launched together with CBERS (China-Brazil Earth Resource Satellite). Its platform is being designed for multiple mission applications. The Brazilian Academy of Sciences has selected four scientific payloads that characterize the mission. The scientific experiments are: ORCAS (Solar and Anomalous Cosmic Rays Observation in the Magnetosphere), PLASMEX (Study of Plasma Bubbles), FOTSAT (Airglow Photometer), and MAGNEX (Geomagnetic Experiment).     

The population of massive stars in R136 from HST/FOC UV observations

New ultraviolet (1300 A, 3400 A),HST FOC observations have been used to derive the UV color-magnitude diagram (CMD) of R136, with the main scientific goal of studying the upper end of the stellar mass function at ultraviolet wavelengths where the color degeneracy encountered in visual CMDs is less severe. The CMD has been compared to a set of theoretical isochrones, which have been computed using the latest generation of evolutionary models and model atmospheres for early type stars. Wolf-Rayet stars are included. Comparison of theTheoretical andobserved CMD suggests that there are no stars brighter than M₁₃₀–11. We use the observed main sequence turn-off and the known spectroscopic properties of the stellar population to derive constraints on the most probable age of R136. The presence of WNL stars and the lack of red supergiants suggests a most likely age of 3±1 Myr. A theoretical isochrone of 3±1 Myr is consistent with the observed stellar content of R136 if the most massive stars have initial masses around 50 M.Bases on Observations with the NASA/ESA Hubble Space Telescope, obtained at the STScI, which is operated by AURA, Inc., under NASA contract NAS5-26555.Astrophysics Division, Space Science Department, ESA     

Experimental Aspects of Mid-Frequency Pulsations (f≈10–100 mHz) in the Southern Polar Cap

We review the results obtained in the frequency range of Pc3 (22-100 mHz) and Pc4 (7-22 mHz) pulsations at Italian Antarctic stations in the southern polar cap (“Mario Zucchelli”, at Terra Nova Bay, TNB, 80^˚.S; “Concordia”, the Italian/French base at Dome C, DMC, 89^˚.S). The absence of a midnight enhancement in the pulsation power suggests a negligible substorm influence at extreme latitudes, while the sharp noon enhancement, which appears only at TNB, is determined by the closer proximity of the station to cusp related phenomena. The relationship between the frequency of the band-limited signals and the interplanetary magnetic field strength, the cone angle influence, and the higher correlation of the Pc3 power with the solar wind speed in the morning hours suggest a global scenario in which upstream waves would be mainly responsible for the mid-frequency activity in the polar cap. However, the polarization pattern is odd with respect to the predictions for tailward propagating modes.     

航空发动机用新材料——16Cr3NiWMoVNbE齿轮钢

综合介绍了新型齿轮钢--16Cr3NiWMoVNbE钢的性能、热工艺及其在航空发动机上的应用.该钢具有淬透性高、晶粒长大倾向低等优异的综合性能,其使用温度可达350℃.该钢的研制成功,满足了我国新一代航空发动机对齿轮材料的需求.     

涡切片图象立体重建

 <正> 1.引言 激光片光技术和流体中微粒的光散射效率逐步提高;从烟雾、水汽到激发诱导荧光使流动可视化程度不断开拓。许多研究工作需要通过观察切片照片获得对复杂流动整体结构的理解。因此,将系列二维切片照片重建成立体图象是十分有意义的。 近年来这方面比较典型的工作有Jimener的平面混合层和Agui and Hesselink的共轴喷流重建,分别在平面型和封闭柱面型的不同气流混合界面研究涡系的生成和发展。用涡迹切片重建的三维图象能清楚地显示涡的内部结构,对提供合理的流动假说和计算模型有重要意义。     

“T”型尾翼飞机的深失速特性研究

应用时间历程法讨论了“Ｔ”型尾翼飞机的深失速开环特性，分析了气动力矩特性和升降舵操纵规律对深失速改出特性的影响。建立了深失速闭环特性计算数学模型，分析了驾驶员数学模型参数变化对深失速特性的影响。研究结果表明，气动力矩特性，升降舵操纵规律和驾驶员模型参数的变化对“Ｔ”型尾翼飞机的深失速改出特性有显著的影响。     

SBS改性再生型木塑复合材料及其耐水性能

为了充分利用城市固体废弃物中的各项资源，本项工作将固体废弃物中的高密度聚乙烯（HDPE）回收后与废弃的木纤维、苯乙烯-丁二烯-苯乙烯（SBS）进行复合，成功地制备出SBS／再生型木塑复合材料，并进行了力学性能测试和水煮试验。结果表明，SBS的加入使木塑复合材料的冲击韧性得到显著改善，同时，复合材料的弯曲强度和弯曲模量没有明显的影响，表明SBS可以作为木塑复合材料的增韧剂。SBS／木塑复合材料经过8周、60℃的水煮后，复合材料的吸水率和厚度膨胀率均有所增加，弯曲模量和冲击韧性分别平均下降14．4％、10．8％。水煮试验初期复合材料的弯曲强度逐渐降低，然后又逐渐增大，第8周后弯曲强度增加的幅度约10％。木塑复合材料的冲击破坏模式以界面脱粘为主，而加入SBS后，复合材料的破坏以纤维断裂和基体断裂为主。     

Evaluating a multiple-hypothesis multitarget tracking algorithm

The performance evaluation of multiple-hypothesis, multitarget tracking algorithm is presented. We are primarily interested in target-detection/track-initiation capabilities as measures of performance. Through Monte Carlo simulations, a multiple-hypothesis tracking algorithm was evaluated in terms of 1) probability of establishing a track from target returns and 2) false track density. A radar was chosen as the sensor, and a general multiple-hypothesis, multitarget tracking algorithm was used in the Monte Carlo simulations. The simulation results predict the probability of establishing a track from returns of a target as well as the false track density per scan volume per unit time. The effects of the target radar cross section and the radar power, measured through the mean signal-to-noise ratio (SNR) were studied, as were the effects of detection threshold and track quality threshold. Computational requirements were also investigated