高精度盘式永磁电机温度分析与研究

以高精度无槽盘式永磁电机为研究对象,建立了电机三维电磁仿真模型。详细分析了该电机反电动势和转矩特性,避免由高次谐波引起的定、转子及永磁体涡流损耗,有效改善了电机的热性能,为进一步研究打下基础。建立了三维温度场仿真模型,分析了热源分布和传热过程,计算了电机在自然散热条件下温度的稳态分布。最后通过电机温升试验,验证了理论分析的正确性与合理性。     

制导炸弹偏航通道变结构控制研究

针对制导炸弹偏航通道存在对象参数摄动与外界干扰问题,设计自适应变结构控制器,并进行分析与改进（特别是分析了对象参数摄动后系统的稳态误差）,通过理论推导保证系统稳定性以及良好的动态响应品质与静态响应品质;最后通过仿真验证了该方法的可行性。     

用于微小型GNC系统的电气单元集成一体化及信息快速处理技术

微小型导航、制导与控制（MGNC）集成一体化电气单元需要采集和处理的数据量较多,且算法复杂,本文采用流水线与高速串行总线技术,实现了集成一体化电气单元电路的多路、实时、同步采样。并对GNC软件中组合导航算法的Kalman滤波器进行了降维处理,车载导航试验表明该设计方法可有效提高组合导航软件的实时性与智能性,为最终提高GNC软件运行速度和效率创造了条件。     

考虑陀螺效应的转子动力学相似准则

针对考虑陀螺力矩的转子系统缩尺相似模型与原型是否满足动力学相似的问题,采用量纲分析法推导了考虑陀螺力矩的转子-简单支撑系统相似准则,得到了模型与原型各物理量相似比.通过求解不同相似比下Jeffcott转子系统临界转速的解析解,和利用有限元软件ANSYS对某转子系统临界转速和振型相似性进行了数值模拟,验证了所推导的考虑陀螺力矩转子系统相似准则的正确性.研究表明:考虑陀螺力矩、简单支撑和Rayleigh比例阻尼的转子系统,在相似转速下缩尺模型与原型的固有频率具有相似性,并且临界转速相似.      

Modelling of galactic Carbon in an asymmetrical heliosphere: Effects of asymmetrical modulation conditions

Observations of galactic cosmic rays (GCRs) from the two Voyager spacecraft inside the heliosheath indicate significant differences between them, suggesting that in addition to a possible global asymmetry in the north–south dimensions (meridional plane) of the heliosphere, it is also possible that different modulation (turbulence) conditions could exist between the two hemispheres of the heliosphere. We focus on illustrating the effects on GCR Carbon of asymmetrical modulation conditions combined with a heliosheath thickness that has a significant dependence on heliolatitude. To reflect different modulation conditions between the two heliospheric hemispheres in our numerical model, the enhancement of both polar and radial perpendicular diffusion off the ecliptic plane is assumed to differ from heliographic pole to pole. The computed radial GCR intensities at polar angles of 55° (approximating the Voyager 1 direction) and 125° (approximating the Voyager 2 direction) are compared at different energies and for both particle drift cycles. This is done in the context of illustrating how different values of the enhancement of both polar and radial perpendicular diffusion between the two hemispheres contribute to causing differences in radial intensities during solar minimum and moderate maximum conditions. We find that in the A > 0 cycle these differences between 55° and 125° change both quantitatively and qualitatively for the assumed asymmetrical modulation condition as reflected by polar diffusion, while in the A < 0 cycle, minute quantitative differences are obtained. However, when both polar and radial perpendicular diffusion have significant latitude dependences, major differences in radial intensities between the two polar angles are obtained in both polarity cycles. Furthermore, significant differences in radial intensity gradients obtained in the heliosheath at lower energies may suggest that the solar wind turbulence at and beyond the solar wind termination shock must have a larger latitudinal dependence.     

A new global version of M(3000)F2 prediction model based on artificial neural networks

A new version of global empirical model for the ionospheric propagation factor, M(3000)F2 prediction is presented. Artificial neural network (ANN) technique was employed by considering the relevant geophysical input parameters which are known to influence the M(3000)F2 parameter. This new version is an update to the previous neural network based M(3000)F2 global model developed by Oyeyemi et al. (2007), and aims to address the inadequacy of the International Reference Ionosphere (IRI) M(3000)F2 model (the International Radio Consultative Committee (CCIR) M(3000)F2 model). The M(3000)F2 has been found to be relatively inaccurate in representing the diurnal structure of the low latitude region and the equatorial ionosphere. In particular, the existing hmF2 IRI model is unable to reproduce the sharp post-sunset drop in M(3000)F2 values, which correspond to a sharp post-sunset peak in the peak height of the F2 layer, hmF2. Data from 80 ionospheric stations globally, including a good number of stations in the low latitude region were considered for this work. M(3000)F2 hourly values from 1987 to 2008, spanning all periods of low and high solar activity were used for model development and verification process. The ability of the new model to predict the M(3000)F2 parameter especially in the low latitude and equatorial regions, which is known to be problematic for the existing IRI model is demonstrated.     

环模设备研制用玻璃钢的放气性能研究

文章介绍了在环模设备研制中采用玻璃钢材料制作真空容器的发展需求,为满足设计要求,对玻璃钢复合材料的放气性能进行研究。文中阐述了材料的放气机理和不同测试方法,以及对材料样品的放气性能的测试过程,并获得了重要数据。这项研究工作为真空系统设计提供了参考依据,也为非金属材料环模设备研制提供了思路。     

旋成体零攻角纵向大扰动势流的AF-2迭代及其并行算法

 <正> 1.引言 为提高跨音速差分计算效率,人们在计算格式的设计、改进方面做了大量的工作,并取得了可喜的成就。并行计算机的出现和发展,使我们有可能进一步提高计算效率。第9期阂赛金等:旋成体零攻角纵向大扰动势流的人F一2迭代及其并行算法A弓n因为并行处理机具有处理数据能力强、计算效益高的特点,但这种机器必须结合具体问题和机器特点加以考虑才能发挥其优势。目前,利用我国设计的“YH一1”(“银河一1”)亿次并行处理机,开展跨音速差分计算的并行算法研究具有理论和运用上的重要意义     

超临界压力下航空煤油在并联管中流量分配特性

研究了超临界压力下国产航空煤油RP-3在竖直并联U型管中的流量分配特性,分析了工质温度、系统压力以及加热热流密度不对称性对流量分配特性的影响规律.其中实验段内、外径分别为1.8mm和2.2mm, 实验中质量流量保持为4g/s,系统压力变化范围为3~5MPa,热流密度变化范围为q=60~240kW/m2. 实验结果表明:较低系统压力下,等热流密度加热至管路油温达到拟临界温度附近时会诱发支管流量的较大变化,从而导致并联管系统各支路流量的重新分配;加热不均对支路流量的影响非常显著;另外,提高系统压力可以有效抑制并联管系统中各支路流量分配失衡,增强系统的稳定性.      

Rocket berthing to an asteroid: Design problems

The results of research in a process of a probe rocket berthing to an asteroid are presented. Control laws were obtained as solutions of three problems, namely berthing considering transient processes in a rocket engine, fastest berthing with regard to fuel consumption and berthing in a scheduled time considering fuel consumption. A program trajectory obtained at solving of the first problem is suitable for mathematical modeling of berthing with the feedback control law and stabilization of angular motion. The solutions of the problems are reduced to simple formulas for controlling parameters calculation in the corresponding structures of control laws. The results can be applied in designing promising space vehicles intended for berthing to other space objects.