发动机试车和数据采集自动化的双微机系统

本文介绍一个双微机对话型实现航空发动机试车和采集数据自动化的微机系统。两台微机分别完成发动机工作状态的控制、显示和发动机试车数据的采集,打印,重要物理参数的监控,应急处理等。两台微机间的相互通讯,可使发动机的状态控制和数据的采集按预定程序交替或同步进行,从而实现自动化的目的。本文对系统的软、硬件结构作了详细的介绍,在目前国内通用试车台的基础上,硬件的改装工作量很小,实现很方便。手动和自动控制间的切换迅速而可靠。本系统在发动机试车台上进行了试验,并通过了航空工业部部级鉴定。     

进口为均匀剪切流的二元亚音扩压器

本文在主流为均匀流的二元亚音扩压器流动计算方法的基础上,发展了一种进口为均匀剪切流的二元亚音扩压器流动特性计算方法。为验证本方法,计算了三种实例,并和试验测定结果进行了比较,二者符合情况良好。     

柔性夹具设计方法与技术

针对ＦＭＳ中夹具设计、制造、组装准备系统自动化程度低的现状,重点分析了柔性夹具设计依据、特点、设计方法,可为其它ＦＭＳ柔性夹具的设计提供参考依据。     

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.     

一种简单的中远程空-空导弹中制导律研究

基于奇异摄动方法,提出了中远程空－空导弹由爬升段控制、巡航段控制和交接段最小能量控制３部分构成的次优中制导律。根据工程实际要求,给出了简单的、易于实现的中制导律执行算法。结果表明,该制导律较好地满足了中制导段的要求。     

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.