湿热对单向复合材料层合板Ⅱ型分层特性的影响

利用横向裂纹拉伸试验模型（Transverse Crack Tension-tension Test）,在3种湿热环境（室温、85℃和85℃/95%RH）条件下,对2种单向碳纤维增强树脂基复合材料（T300/QY8911和HTA/6376）层合板的Ⅱ型分层特性进行了试验研究。结果表明湿热环境导致复合材料层间断裂韧性降低,引起Ⅱ型应变能释放率门槛值显着下降,裂纹扩展速率大大提高,温度的影响较湿度更为明显。利用电镜（SEM）对试样分层表面进行了检测,湿度对断面特征无明显的影响。     

Voyager 2 Solar Wind Observations in the Outer Heliosphere

We discuss the solar wind parameters measured in the distant heliosphere from the Voyager 2 spacecraft. Periodic variations in the speed of the wind observed at roughly the solar rotation period may correspond to interaction regions between slower and faster streams of wind. Since the interplanetary magnetic field is enhanced in such regions, they are important for the study of modulation of cosmic rays. Unfortunately, direct observation of the enhanced magnetic field from Voyager 2 has been made difficult by spacecraft-associated noise since 1989.     

The Low Metallicity Tail of the Halo Metallicity Distribution Function

Ongoing spectroscopy and photometry of stars selected in the HK objective-prism/interference-filter survey of Beers and colleagues has resulted in the identification of many hundreds of additional stars in the halo (and possibly the thick disk) of the Galaxy with abundances [Fe/H] -2.0. A new calibration of the technique for estimation of metal abundance based on a CaII K index as a function of broadband B - V color is applied to obtain metallicities for stars observed with the SSO 2.3m and INT 2.5m telescopes. This new data is combined with other samples of extremely metal-deficient stars (Ryan and Norris, 1991a; Beers et al., 1992; Carney et al., 1994) to form a large database of objects of low metallicity. The combined sample is examined and compared with expectations derived from a Simple Model of Galactic chemical evolution. There appears to be a statistically-significant deficit of stars more metal-weak than [Fe/H] = -3.0. An abundance of [Fe/H] -4.0 can be taken as the low-metallicity limit for presently-observable stars in the Galaxy.     

CVD铱涂层／铼基复合喷管研究进展

介绍了高温抗氧化铱涂层／铼基复合喷管的化学气相沉积制备工艺,并就铱,铼的有关性能,ＣＶＤ铱／铼复合中元素的扩散,铱／铼合金的氧化行为及寿命预测等理论研究作了评述。     

战斗机敏捷性管理系统

阐述了设计敏捷性管理系统的必要性,介绍了传统大迎角限制器,分析了其存在的不足,在基础上,介绍了国外关于敏捷性管理 研究情况,包括敏捷性管理系统的基本概念,管理模式,设计中应注意的问题,分析结果表明,敏捷性管理系统有助于提高飞机的作战效能并可减轻驾驶员的负担。     

弹性梁碰撞阻尼识别的新方法

首先将连续碰撞系统离散成包括任意个模态的状态方程,然后基于Hertz定理和能量平衡原理,证明弹性碰撞阻尼取决于碰撞冲量和最大碰撞力,提出了确定弹性梁碰撞阻尼的新方法,解决了碰撞阻尼识别中的关键问题。最后由两个弹性梁的碰撞实验检验了其正确和有效性。     

不均匀进气对压缩系统稳定性影响的逐级动态响应模型研究

发展了一种分析进口畸变对多级轴流压气机影响的逐级动态响应模型。采用动态压缩系统模型和动态加载技术,建立了一种压缩系统气动稳定性分析的新方法。应用新的模拟方法对一８级跨声多级压气机进行了详细的数值分析。结果表明,所发展的逐级动态响应模型更合理和可靠。基于流动阻塞,给出了一种更为迅速的压缩系统失稳识别方法。     

Experiments in Adaptive Estimation of Unknown Binary Waveforms

A special-purpose adaptive machine is described which carries out estimation in real time of an unknown binary waveform which is perturbed with additive Gaussian noise. Unknown waveforms of over 103 samples in duration can be recovered. The unknown waveforms are of unknown epoch and can reappear at either random or periodic time intervals. The observed signal is received at moderate or low signal-to-noise ratios so that a single observation of the received data (even if one knew the precise signal arrival time) is not sufficient to provide a good estimate of the signal waveshape. Experimental results are described which show transient behavior waveform estimate. The transient behavior is expressed as the number of errors in the current estimate of the signal plotted vs. time. In a noisy environment, each ``learning' transient is a random time function. These learning transients are shown for several different signal-to-noise ratios and indicate the threshold noise levels for various types of initial states of the machine memory.     

Output of a Balanced Frequency Discriminator Driven by a Sine Wave and Gaussian Noise

The output of a realizable balanced frequency discriminator is calculated for an input consisting of a sine wave plus Gaussian noise. Explicit autocorrelation and power spectra are found for one practical embodiment of the discriminator for various input carrier-to-noise ratios, with the carrier tuned to center frequency and also off-center. The formulas also permit the calculation of the output for the case of a spectrum of noise slowly swept through the discriminator. Although qualitatively similar to results previously obtained with an ideal discriminator, substantial differences are also found. Measurements are made that closely verified the theoretical results. No limiting is assumed.