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     

光学太阳反射器的性能评价试验规范

航天器在地面待发射期间和空间实际飞行过程中，热控元件光学太阳反射器要遇到各种地面和空间环境，为了航天器的可靠和长寿命，必须对所制备的ＯＳＲ涂层进行各种地面和空间环境试验并对其各项性能检验与考核，该文就这一系列试验的目的和规范进行了讨论。     

卫星优化热设计方法

试图把最优化技术应用于卫星工程的热设计中,提出一种优化热设计的方法,并以14个节点模型作为实例进行了计算分析,采用Hooke-Jeeves 的直接搜索法得到了满意的结果。初步编制的计算机程序,可作为卫星热设计方案计算的基础。     

微重力场中对流—辐射—传质系统的地面模拟技术

研究了微重力条件下对流－辐射－传质稳态系统的地面相似模拟技术，进一步发 温度－材料综合保护技术。通过采取补偿热流，调整壁面热流密度分布的方法，保持了原型与尺寸适当缩小后的模型的Ｎｕ数，Ｓｈ数，材料，温度，湿度不变，从而实现模型与原型流动，换热和传质相似。     

防静电白色热控涂层的空间环境性能试验

通过在氧化锌晶格中掺入重金属离子，得到具有防静电功能的白色颜料，再以丙烯酸树脂为粘合剂制备出空间飞行器外表面用的ACR－1防静电白色热控涂层；研究了空间环境效应（包括紫外辐照，电子和质子辐照）对该热控涂层太阳吸收率的影响并与有机硅白色热控涂层进行了比较，地面模拟空间环境试验研究结果证明，ACR－1防静电白色热控涂层具有良好的空间稳定性。     

多层隔热材料的性能研究

本文从多层隔热材料的实际应用条件出发,研究了它们在几种层密度下的隔热性能,特别包括了在层密度较高情况下的性能。为了改善多层隔热材料的隔热性能,采用了间隔几层隔离层的组合形式。压缩负荷对层密度、隔热性能的影响也进行了初步的研究。     

Numerical simulations of water spray on flame deflector during the four-engine rocket launching

This paper aims to study on the cooling effect with two types of water spray nozzle on the flame deflector during the four-engine launch vehicle take-off. To accurately simulate the two-phase flow of the rocket gas with multispecies and the water spray, the three-dimensional compressible Navier-Stokes equations, discrete ordinates methods and realizable k-Ɛ turbulence model are used to establish the rocket supersonic plumes impact model. The Eulerian dispersed phase (EDP) model was used to simulate the water spray into the exhaust gas. The accuracy and effectiveness of the gas-liquid flow model are verified by a good agreement between simulation results and experimental data. On this basis, a series of numerical simulation studies under different water injection position are performed. The results show that the high temperature regions, along the axis of engines on the deflector plate, have no significant temperature decreasing effect by water spray from the nozzles mounted on the apex of the deflector, and the high temperature converts a large quantity of water into vapor near the plume boundary, which would decrease the flow conductivity. With the cooling spray nozzle fixed directly to the deflector plate, the temperature decrease effect is obvious and the effect of thermal shock on deflector plate induced by exhaust plume is reduced, so that it can prevent the flame deflector from thermal ablation. The study results provide indepth information and engineering guidance for designing the water spray systems and increasing the safety of the launch process.     

Prediction of shock-layer ultraviolet radiation for hypersonic vehicles in near space

A systemic and validated model was developed to predict ultraviolet spectra features from the shock layer of near-space hypersonic vehicles in the ‘‘solar blind" band region. Computational procedures were performed with 7-species thermal non-equilibrium fluid mechanics, finite rate chemistry, and radiation calculations. The thermal non-equilibrium flow field was calculated with a two-temperature model by the finite volume technique and verified against the bow-shock ultra-violet(BSUV) flight experiments. The absorption coefficient of the mixture gases was evaluated with a line-by-line method and validated through laboratory shock tube measurements. Using the line of sight(LOS) method, radiation was calculated from three BSUV flights at altitudes of 38,53.5 and 71 km. The investigation focused on the level and structure of ultraviolet spectra radiated from a NO band system in wavelengths of 200–400 nm. Results predicted by the current model show qualitative spatial agreement with the measured data. At a velocity of 3.5 km/s(about Mach11), the peak absolute intensity at an altitude of 38 km is two orders of magnitude higher than that at 53.5 km. Under the same flight conditions, the spectra structures have quite a similar distribution at different viewing angles. The present computational model performs well in the prediction of the ultraviolet spectra emitted from the shock layer and will contribute to the investigation and analysis of radiative features of hypersonic vehicles in near space.