提高形状记忆合金丝工作频率的一种方法

研究了提高形状记忆合金（SMA）工作频率的物理方法--研制细丝。给出了拉拔细丝的工艺流程,从理论上分析了在不同的加热和冷却过程中丝径与响应速度的关系,对2种丝径的SMA丝进行了性能对比测试。同时测定了2种丝径的SMA的响应速度。结果表明,丝径的减小对丝的相变性能,如最大恢复应变、最大恢复应力等影响不大,但可显着提高其动作频率。     

涡扇发动机气路故障定量诊断的BP网络研究

为了克服ＢＰ算法收敛速度慢的问题,提出了一种基于混合学习规则的ＢＰ算法,并采用模归一化方法,成功地定量组织了故障的学习样本,建立了能够定量分析发动机气路部件故障的人工神经网络（ＢＰＮ）。通过分析测量系统随机误差的影响和实际试车数据的效验结果,表明该网络具有较强的推广能力及适应性,能基本满足故障定量诊断的要求,并具有较好的工程实用性。     

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.     

三组元喷嘴雾化特性的试验研究

三组元喷嘴是气氢／液氧／煤油火箭发动机的重要部件,对４ 种类型的三组元喷嘴进行了雾化特性试验, 研究了喷嘴的雾化特性随各组元喷注压降的变化规律, 分析了喷嘴结构对雾化性能的影响, 比较了相同工况下单喷嘴和三喷嘴的雾化性能, 进行了三组元工况和双组元工况下的雾化特性试验, 试验结果表明同轴离心内混式喷嘴的雾化性能较好。所得结论对三组元喷嘴和气液同轴式喷嘴的优化设计有重要的参考价值     

Soho Observations of Density Fluctuations in Coronal Holes

In recent UVCS/SOHO White Light Channel (WLC) observations we found quasi-periodic variations in the polarized brightness (pB) in the polar coronal holes at heliocentric distances of 1.9 to 2.45 solar radii. The motivation for the observation is the 2.5D MHD model of solar wind acceleration by nonlinear waves, that predicts compressive fluctuations in coronal holes. In February 1998 we performed new observations using the UVCS/WLC in the coronal hole and obtained additional data. The new data corroborate our earlier findings with higher statistical significance. The new longer observations show that the power spectrum peaks in the 10–12 minute range. These timescales agree with EIT observations of brightness fluctuations in polar plumes. We performed preliminary LASCO/C2 observations in an effort to further establish the coronal origin of the fluctuations. This revised version was published online in June 2006 with corrections to the Cover Date.     

推力矢量飞机的起飞性能研究

简述推力矢量技术的作用,建立了带三轴推力矢量飞机的起飞滑跑段运动方程,通过数值仿真探讨了推力矢量的偏转大小对起飞性能的影响,对不同推力矢量偏转下飞机起飞性能的仿真计算结果进行了分析。仿真结果表明,采用直接力控制可以明显提高飞机的起飞性能。     

Radio observations of Venus and the interpretations

The radio observations of Venus are reviewed and compared with theoretical microwave spectra computed for a variety of models of the Venusian environment. The models considered are (a) a CO₂-N₂ atmosphere, (b) an atmosphere of dust (the aeolosphere model), and (c) a cloud model with various loss mechanisms in the cloud. The effect of polarization on the surface emissivity has been included in all the computations. It is shown how the radio observations place limits upon the acceptable models, for example, the density and size of dust particles required in the aeolosphere model. It is shown how some models place severe restrictions on radar observations at short centimeter wavelengths, thereby emphasizing the importance of such experiments. These same models show that the Mariner II observations can not be interpreted in terms of surface phenomena and provide a new interpretation for the microwave phase effect.This work was supported in part by the U.S. Army, Navy and Air Force under Contract DA36-039-AMC-03200(E); and in part by the National Aeronautics and Space Administration (Grants NsG-250-62 and NsG-419).