战术导弹大迎角高M数绕流特性分析

某战术导弹高马赫数大迎角蒸汽屏流动显示和测力试验先后在中国空气动力研究与发展中心0.6m跨超声速风洞中进行,本文给出了M数为0.8、2.0、4.0,模型迎角为20°、30°、40°时的部分结果.结果表明:模型在大迎角下出现十分复杂的涡系图像;随着M数或迎角的增加,涡的尺寸及其离弹身的高度都增大;当模型状态对称时,流动图像基本上是对称的,而当模型状态不对称时,流动图像也不对称.测力结果与流动显示图像结果具有较好的一致性.     

基于实时交易系统中间件的设计与实现

实时交易系统是一种基于客户 /服务器模式的应用系统。随着人们对实时交易系统的可扩展性和性能的需求 ,两层客户 /服务器模式难以满足系统要求。中间件技术的产生和发展给两层客户 /服务器模式注入了新的活力     

抗氧化处理对3D C/C复合材料性能的影响

研究了采用化学气相反应法制备的SiC抗氧化涂层对3D整体编织C／C复合材料的密度、力学性能以及微观结构的影响。结果表明，3D C／C复合材料经抗氧化处理后，其密度、开孔率以及力学性能均有不同程度的提高。由SEM微观结构可以看出，其力学性能提高是由于气态Si渗入到材料基体内部，并与内部的C反应生成SiC，在一定程度上弥合了材料中的缺陷所致。     

微量碳化硅纤维/环氧树脂复合吸波材料研究

研究微量碳化硅纤维／环氧树脂复合吸波材料不同排布的吸波性能。结果表明：碳化硅纤维吸波性能与纤维的排布间距和纤维含量密切相关；正交排布试样的吸波效果总体上优于平行排布试样；间距为4mm、纤维含量为1600根／束时的正交排布方式获得大于8GHz、-10dB以下的反射衰减。     

不同组织状态TC4合金靶材损伤行为的研究

采用直径为4mm的CoCr15钢珠作为弹丸对两种不同组织状态的TCA合金进行撞击试验，撞击速度为1．5km／s；观察撞击后不同厚度靶材的宏观损伤及微观损伤行为。结果表明：靶材的组织状态对靶材的宏观损伤行为有很大的影响；时效处理态的组织具有更高的绝热剪切敏感性，在中厚靶发生了绝热冲塞；退火态中厚靶的背面则发生了凸起。各种靶材的微观损伤形式基本相同，在弹坑附近出现了大量的绝热剪切带；微孔洞在绝热剪切带内形核、长大并连结成为裂纹。     

模压工艺制备短纤维增强C/C复合材料的研究

以模压工艺为主线，综述了短纤维增强C／C复合材料的制备、工艺特点及其组织和性能；介绍了国内外不连续纤维增强C／C复合材料性能的研究现状；提出了发展我国短纤维增强C／C复合材料急需解决的技术难题。     

航空发动机滑油系统稳态压力模型研究

以某型发动机滑油系统为研究对象,深入分析了系统的工作原理和部件结构特点。综合应用流体力学,工程热力学理论以及数值计算和实验的方法,建立了滑油系统主要部件的数学模型和管路压力损失的计算模型;在此基础上,依据发动机滑油系统良好状态下采集的数据,建立了滑油系统的稳态压力数学模型,为判断滑油系统性能衰退和故障提供参考依据。      

The Time-of-Flight Energy,Angle, Mass Spectrograph (Teams) Experiment for Fast

The Time-of-flight Energy Angle Mass Spectrograph (TEAMS) is being flown on the FAST Small Explorer mission to measure the 3-dimensional distribution function of the major ion species present in the lower magnetosphere. The instrument is similar to time-of-flight plasma analyzer systems that have been designed and planned for flight as CODIF (COmposition and DIstribution Function analyzer) on the four European Space Agency Cluster-II spacecraft and, as ESIC (Equator-S Ion Composition instrument) on Equator-S. This instrument allows the 3-dimensional distribution functions of individual ion species to be determined within spin period (2.5 s). Two-dimensional distributions are measured in 80 ms. These capabilities are crucial for the study of selective energization processes in the auroral regions of the magnetosphere. The design, operational characteristics, and test and calibration results for this instrument are presented. The sensor consists of a toroidal top-hat electrostatic analyzer with instantaneous acceptance of ions over 360° in polar angle. After post-acceleration of the incoming ions by up to 25 kV, a time-of-flight mass spectrograph discriminates the individual species. It has been demonstrated through calibration that the instrument can easily separate H⁺, He²⁺, He⁺, O⁺ and, for energies after post-acceleration of > 20 keV, even O₂ ⁺ molecules. On-board mass discrimination and the internal accumulation of several distinct data quantities combined with the spacecraft's flexible telemetry formatting allow for instrument data rates from 7.8 kb s^–1 to 315 kb s^–1 to be telemetered to ground through the FAST centralized Instrument Data Processor.     

Ion Acoustic Waves in the Heliosphere

Observations of ion acoustic waves in the solar wind during the first and second orbit of the Ulysses spacecraft are presented. The observations show variations of the wave activity with the heliolatitude and with the phase of the solar cycle. The interrelationships between the wave intensity and the electron heat flux and the ratio of electron to proton temperature, T _e/T _p, are examined. This revised version was published online in August 2006 with corrections to the Cover Date.     

The FAST Satellite Fields Instrument

We describe the electric field sensors and electric and magnetic field signal processing on the FAST (Fast Auroral SnapshoT) satellite. The FAST satellite was designed to make high time resolution observations of particles and electromagnetic fields in the auroral zone to study small-scale plasma interactions in the auroral acceleration region. The DC and AC electric fields are measured with three-axis dipole antennas with 56 m, 8 m, and 5 m baselines. A three-axis flux-gate magnetometer measures the DC magnetic field and a three-axis search coil measures the AC magnetic field. A central signal processing system receives all signals from the electric and magnetic field sensors. Spectral coverage is from DC to 4 MHz. There are several types of processed data. Survey data are continuous over the auroral zone and have full-orbit coverage for fluxgate magnetometer data. Burst data include a few minutes of a selected region of the auroral zone at the highest time resolution. A subset of the burst data, high speed burst memory data, are waveform data at 2×10⁶ sample s^–1. Electric field and magnetic field data are primarily waveforms and power spectral density as a function of frequency and time. There are also various types of focused data processing, including cross-spectral analysis, fine-frequency plasma wave tracking, high-frequency polarity measurement, and wave-particle correlations.