大规模定制设计的产品簇匹配研究

采用基于规则与基于实例相结合的推理方法，给出典型的基于实例推理的专家系统解决问题的一般过程，本文重点研究大规模定制设计的产品簇匹配问题，实施二级匹配策略，先采用规则推理的方法对产品簇大类属性进行匹配，缩小匹配范围，后采用基于实例推理的方法对产品簇小类具体属性进行定量精确匹配，优化了设计手段，效果良好。     

Relationships between energetic storm particle events and interplanetary shocks driven by full and partial halo coronal mass ejections

We have analysed energetic storm particle (ESP) events in 116 interplanetary (IP) shocks driven by front-side full and partial halo coronal mass ejections (CMEs) with speeds $>$400 km s^?1during the years 1996–2015. We investigated the occurrence and relationships of ESP events with several parameters describing the IP shocks, and the associated CMEs, type II radio bursts, and solar energetic particle (SEP) events. Most of the shocks (57 %) were associated with an ESP event at proton energies $>$1 MeV.The shock transit speeds from the Sun to 1 AU of the shocks associated with an ESP event were significantly greater than those of the shocks without an ESP event, and best distinguished these two groups of shocks from each other. The occurrence and maximum intensity of the ESP events also had the strongest dependence on the shock transit speed compared to the other parameters investigated. The correlation coefficient between ESP peak intensities and shock transit speeds was highest (0.73 $\pm$ 0.04) at 6.2 MeV. Weaker dependences were found on the shock speed at 1 AU, Alfvénic and magnetosonic Mach numbers, shock compression ratio, and CME speed. On average all these parameters were significantly different for shocks capable to accelerate ESPs compared to shocks not associated with ESPs, while the differences in the shock normal angle and in the width and longitude of the CMEs were insignificant.The CME-driven shocks producing energetic decametric–hectometric (DH) type II radio bursts and high-intensity SEP events proved to produce also more frequently ESP events with larger particle flux enhancements than other shocks. Together with the shock transit speed, the characteristics of solar DH type II radio bursts and SEP events play an important role in the occurrence and maximum intensity of ESP events at 1 AU.     

基于产品平台技术的大规模定制质量保证研究

明确提出了针对大规模定制生产模式特点的质量保证体系的实现是一项系统工程,其实现方法主要包括:以顾客满意为中心,凝练顾客需求来构建产品平台;基于产品平台,重组产品过程;加强敏捷供应链管理,稳定产品平台质量;持续改进产品平台,推动最终产品质量提高等.体系实施研究的实践表明:基于产品平台技术的大规模定制质量保证可以帮助企业增强满足顾客群体与个体质量要求的能力,最终达到持续提升顾客满意的目的.      

风力机防冰热载荷计算

采用一种新的基于压力和剪切力的溢流水流量计算方法进行部件表面防冰热载荷数值模拟。求解雷诺平均N-S方程,嵌入k-ωSST湍流模型获得空气流场;欧拉法求解水滴质量和动量守恒方程,获得部件周围水滴速度分布和表面水滴撞击特性;基于传统的Messinger控制容积思想,分析控制体的各项热流,建立质量守恒和能量守恒方程,引入溢流水质量流量计算方程,封闭控制方程,求解方程组获得表面所需的防冰热载荷。采用本文提出的新的流量计算方法获得了NACA0012翼型表面的结冰冰形,并与试验数据进行对比,说明了流量计算方法的正确性。计算分析了不同条件下表面的防冰热载荷分布,结果表明,工作风速和液态水含量的变化既影响了防冰热载荷大小,也影响了溢流范围,而工作温度仅影响防冰热载荷,水滴平均容积直径仅影响溢流范围。     

基于ALE的降落伞充气过程数值仿真

采用任意拉格朗日-欧拉法(Arbitrary Lagrange Euler method,ALEM)流固耦合方法模拟某模型伞在低速气流作用下充气展开过程。计算获得了充气过程中伞衣应力、流场速度矢量、压力以及伞衣半径变化等结果。与试验对比,开伞过程相同,同样出现了伞衣顶部塌陷、抖动等现象。通过对数值结果的分析解释了伞衣抖动以及风洞试验中伞底拍动产生巨大噪声的原因,同时预测开伞过程中的危险截面。     

基于分布质量轴模型的尾传动轴系临界转速分析

以直升机尾斜轴为研究对象,推导了传动轴的分布质量传递矩阵,模型中考虑了弯矩、横向位移、剪切变形、转动惯量、陀螺力矩和轴向力等 因素的综合影响。建立了膜片联轴器和弹性支承的传递矩阵。给出了尾传动轴系临界转速的计算方法。以三支点水平轴系为分析对象,将本文传递矩阵法计算的结果与有限元法计算的结果进行了对比分析,以检验本文传递矩阵法的有效性。本文传递矩阵法相对于有限元法的最大计算误差为4.1%,表明本文传递矩阵法的计算精度较高,同时本文传递矩阵法的计算速 度更快,便于设计人员进行尾传动轴系临界转速的影响因素分析。     

An empirical model to predict the 1-AU arrival of interplanetary shocks

We extend the empirical coronal mass ejection (CME) arrival model of Gopalswamy et al. [Gopalswamy, N. et al. Predicting the 1-AU arrival times of coronal mass ejections, J. Geophys. Res. 106, 29207, 2001] to predict the 1-AU arrival of interplanetary (IP) shocks. A set of 29 IP shocks and the associated magnetic clouds observed by the Wind spacecraft are used for this study. The primary input to this empirical shock arrival model is the initial speed of white-light CMEs obtained using coronagraphs. We use the gas dynamic piston–shock relationship to derive the ESA model which provides a simple means of obtaining the 1-AU speed and arrival times of interplanetary shocks using CME speeds.     

面向未知目标的柔性关节空间机器人滑模控制

针对载荷捕获的空间机器人控制问题,同时考虑机械臂关节柔性和非合作目标质量未知等因素影响,提出一种基于目标质量观测器的滑模变结构控制方法.首先,针对空间非合作目标质量未知问题,设计基于改进的最小二乘迭代算法实现对非合作目标质量在线辨识.进而,采用拉格朗日方法和动量矩守恒原理,建立漂浮基座柔性关节空间机器人动力学模型;针对...     

High resolution spectroscopy of X-ray emission from high mass X-ray binaries

This article briefly reviews first the progress of spectroscopy in X-ray astronomy from proportional counters, a major instrument in early phase of X-ray astronomy, to gas scintillation proportional counters, X-ray CCD cameras, transmission and reflection gratings, and finally to X-ray micro-calorimeters. As a typical example of spectral features observed from high mass X-ray binaries (HMXBs), the spectra observed from Vela X-1 with Chandra grating spectrometers are then presented and compared with computer simulations for high mass binary systems.