金属水反应水冲压发动机系统性能估算

使用金属／水反应燃料是推进水下超高速航行器的最佳途径，分析了单次注水和二次注水的铝／水反应燃料水冲压发动机系统，得出了燃料质量配比、燃烧室温度、燃烧室压强、系统有效推力、效率等关键技术性能指标。指出了二次注水系统的优越性并提出了一种二次注水系统的实施方案。分析结论与实际系统性能指标相吻合，证明了分析的正确性，可以为系统研究提供参考。     

原位反应合成Nb掺杂Al2O3/TiAl复合材料的显微结构分析

利用Al-Ti-TiO2体系原位反应合成了Nb掺杂Al2O3／TiAl复合材料。借助XRD和SEM研究了Nb掺杂Al2O3／TiAl的显微结构以及Nb引入量对复合材料显微结构的影响。结果表明，复合材料由TiAl、Ti3Al、Al2O3、Nb和NbAl3相构成，细小Al2O3颗粒分布于基体晶粒交界处，存在一定的团聚；Nb元素引入量的高低，可调节产物中TiAl和Ti3Al的相对含量，随Nb含量的增大，TiAl含量逐渐减少，Ti3Al则逐渐增大；同时，基体晶粒和Al2O3颗粒均有所细化，且分布逐渐均匀，材料的均匀性得到改善。     

高超声速平头圆柱绕流化学反应流场的DSMC/EPSM混合算法研究

本文发展了平衡粒子模拟方法(EPSM)，建立了与高温气体化学反应动力学理论相匹配的EPSM耦合模型，并通过混合参数进行流区的自动识别，将EPSM方法与蒙特卡罗直接模拟方法(DSMC)结合，构造了可模拟化学反应流动的DSMC／EPSM混合算法。应用该算法对汲及化学反应的轴对称情况下高超声速平头圆柱绕流流场进行模拟，将结果与DSMC方法的结果进行比较，验证了新算法对求解化学反应流动的可行性。将混合算法的计算效率与DSMC方法的计算效率进行比较，发现混合算法能够大大提高计算效率。     

金属零件的一种快速成型制造方法

金属零件的快速制造是快速成型技术的最终目标之一,也是当今快速成型领域的一大研究热点。本文在介绍快速成型技术的一个重要分支－选区激光烧结的基础上,提出了一种基于小功率激光快速成型系统的金属零件成型工艺。这种方法首先烧结金属与有机粘结剂的混合粉末,生成“绿件”,而后除粘、熔渗金属,最终得到致密的金属件。最后,文中给出了加工实例,并对这种工艺的影响因素进行了详细的分析与讨论。     

电励磁双凸极无刷直流发电机电压纹波分析

在电励磁双凸极无刷直流发电机结构参数一定,电阻性负载的条件下,考虑到铁芯材料的非线性饱和特性,在二维有限元非线性分析的基础上,通过仿真定量地分析解释了励磁磁场不同时,12/8电励磁双凸极发电机相电压波形在120~180°变化的原因及变化规律,并分析了励磁磁场强弱及电枢反应对发电机输出直流电压纹波的影响及其非线性变化规律,经过实验验证了分析结果的正确性。分析所得结论为电机性能的优化设计提供了理论依据,并对励磁控制的优化具有指导作用。同时,对双凸极电动机控制方式的选择具有指导意义。     

TiB_2粉料的合成与纯化研究

基于SHS还原反应合成TiB2 混合粉料 ,研究了酸洗条件对TiB2 纯度的影响。实验结果表明 ,TiO2 B2 O3 Mg三元系统的化学反应由两部分组成 ,第一部分由金属Mg还原出B和Ti单体 ,第二部分由两种单体化合反应生成TiB2 。TiB2 粉料的纯度主要取决于酸洗条件。提高盐酸浓度、增加酸过量和延长酸洗时间可以提高TiB2 粉料的纯度 ,而升高酸洗温度还可以大大加快酸洗速度     

基于SVR选择性集成的机场噪声预测模型研究

机场噪声预测对机场规划设计、航班计划制定以及机场噪声控制具有十分重要的作用。针对机场周围各个监测点上的单飞行事件进行噪声预测。由于机场噪声数据的复杂性,用单一的SVR方法对其预测往往得出局部优化结果,不能达到理想的预测效果,针对这一问题,提出一种基于SVR选择性集成的机场噪声预测方法,通过Adaboost方法对机场噪声数据进行采样训练得到多个SVR预测模型,并结合一种排序方法对预测模型进行选择集成得到最终机场噪声预测值,取得了较好的预测效果。     

CLVD 法制备C/C复合材料工艺探索研究

研究了采用化学液气相沉积法制备C／C复合材料的工艺过程，分析了不同预制件、温度、浸泡时间等工艺参数对致密速度、效果的影响，并总结出了一套快速高效的致密方法。     

The Primordial Helium-4 Abundance from Observations of a Large Sample of Blue Compact Dwarf Galaxies

We use a sample of 45 low-metallicity H II regions in blue compact dwarf (BCD) galaxies to determine the primordial helium abundance YP with a precision better than 5%. We have carefully investigated the physical effects which may make the He I line intensities deviate from their recombination values such as collisional and fluorescent enhancements, underlying He I stellar absorption and absorption by Galactic interstellar Na I. By extrapolating the Y vs. O/H and Y vs. N/H linear regressions to O/H = N/H = 0, we obtain YP = 0.244±0.002 and 0.245±0.001, respectively, higher than previous determinations (YP = 0.230 - 0.234). Part of the difference comes from the fact that previous investigators have not taken into account underlying He I stellar absorption, especially in the NW component of the BCD I Zw 18 which, because of its extremely low metallicity plays a key role in the determination of YP. We derive a slope dY/dZ = 2.3±1.0, considerably smaller than those derived before. With this smaller slope and taking into account the errors, chemical evolution models with an outflow of well-mixed material can be built for star-forming dwarf galaxies which satisfy all the observational constraints. Our YP gives _bh ₅₀ ² = 0.058±0.007,f consistent with the lower limit set by dynamical measurements and X-ray observations of clusters of galaxies. It is also consistent, within the framework of standard big bang nucleosynthesis theory, with measurements of primordial 7Li in galactic halo stars and with the D/H abundance measured in absorption systems toward quasars by Burles and Tytler (1997).     

Development process of muzzle flows including a gun-launched missile

Numerical investigations on the launch process of a gun-launched missile from the muzzle of a cannon to the free-flight stage have been performed in this paper. The dynamic overlapped grids approach are applied to dealing with the problems of a moving gun-launched missile. The high-resolution upwind scheme(AUSMPW+) and the detailed reaction kinetics model are adopted to solve the chemical non-equilibrium Euler equations for dynamic grids. The development process and flow field structure of muzzle flows including a gun-launched missile are discussed in detail.This present numerical study confirms that complicated transient phenomena exist in the shortly launching stages when the gun-launched missile moves from the muzzle of a cannon to the freeflight stage. The propellant gas flows, the initial environmental ambient air flows and the moving missile mutually couple and interact. A complete structure of flow field is formed at the launching stages, including the blast wave, base shock, reflected shock, incident shock, shear layer, primary vortex ring and triple point.