Trajectory control strategy of cathodes in blisk electrochemical machining

A turbine blisk, which combines blades and a disk together, is one of the most important components of an aero engine. In the process of blisk electrochemical machining (ECM), the sheet cathode, which is usually used as a tool electrode, has a complicated structure. In addition to that, the channel between the adjacent blades is narrow and twisted, so interference is apt to happen when the sheet cathode feeds into the channel. Therefore, it is important to choose suitable trajectory control strategy. In this paper, a new trajectory control strategy of the sheet cathode is presented and corresponding simulation analysis is conducted on the basis of an actual blisk model. The simulation results demonstrate that the sheet cathode can feed into the channel by a spatial line trajectory without interference. Moreover, the verification experiments are carried out according to the simulation. The experimental results show that the cathode can move into the channel without interference. It is verified that the new trajectory control strategy is correct and can be used in the blisk ECM process successfully.     

绳系卫星实施安全捕获的能量最优控制

考虑系绳质量、系统质心变化及状态、控制约束,基于Lagrange方程给出了圆轨道条件下空间绳系网捕系统三维动力学模型.推导得到了零相对速度条件下的安全捕获末端条件,研究了面内安全捕获策略下的非线性能量最优控制问题.为保证方法的适用性,基于Legendre伪谱法将连续时间最优控制问题离散为标准的非线性动态规划问题.最后在...     

静叶吸气对某轴流压气机裕度影响的研究

运用Numeca CFD对某大弯度叶栅和某轴流压气机流动进行数值模拟,为减小由于边界层分离而带来的损失,拓宽稳定工作范围,提出叶片吸力面表面开缝抽气方案.综合研究开缝位置、开缝长度、及吸气量大小对流动分离结构和裕度的影响.结果表明通过静子叶片上边界层抽气引出分离区域的低能量气流,可以明显的改善气动性能,分离得到很好的抑制,稳定工作裕度得到了提高.      

国际商务中的跨文化交际意识

跨文化交际(Intev-clllture Communication)是指不同文化背景的个人之间的交际,即不同文化背景的人之间所发生的相互作用.随着社会经济的发展,拥有不同文化背景的人们之间的合作越来越频繁.增强跨文化理解、克服文化冲突、加强文化传播和合作已经变得十分重要.本文分析了跨文化交际冲突的表现、产生这些冲突的原因并提出了具体对策.     

混配型吸热碳氢燃料热裂解及催化裂解

为提高吸热型碳氢燃料的吸热能效，将辅助燃料Y按不同比例与碳氢燃料混合，配制成新的混配型YNNJ—150燃料，利用连续流吸热型碳氢燃料裂解微型反应色谱评价装置，考察了它的热裂解转化率和低碳烯烃的选择性，并在HZSM—5分子筛上进行了催化裂解评价。结果表明混配型YNNJ—150燃料不仅降低了裂解温度，同时提高了燃料裂解的低碳烯烃的选择性，增加了燃料的吸热能力，且混合辅助燃料Y的比例为15％时的混配燃料YcNNJ—150的效果最好。混配型燃料可成为今后研究的一个重要方向。     

大跨悬挑屋盖风压分布风洞试验分析

通过大跨悬挑曲面屋盖刚性模型风洞试验,分析各风向角风压系数均值等值线图及跨中区域时体型系数以确定最不利风向角,研究跨中迎风边缘及顺风测点功率谱及相干特性,最后针对跨中不同位置测点风压概率分布密度特性探讨峰值因子合理取值。     

直升机旋翼回波特性建模

给出了雷达半主动寻体制的直升机旋翼回波模型,分析了直升机旋翼回波的时频特性,以旋翼真实参数对模型进行了仿真,并研究了直升机旋翼回波在时域上的调制效应及频域分布特点。结果表明：理论模型所得结果与外场实验的导引头跟踪直升机实验数据吻合。     

大气层内拦截弹脉冲发动机消耗量离线计算

采用姿控式直接侧向力/气动力复合控制方式可以显著提高大气层内拦截弹的机动能力,但由于产生侧向推力的脉冲发动机数量有限,必须考虑减少使用数量的问题.除了最优化脉冲发动机点火分配逻辑之外,充分利用气动力也是一种可能的方案.本文基于弹体运动的线性化模型,探讨了在给定攻角响应时间的情况下,最大限度地利用气动力能否节省脉冲发动机点火数目,并对攻角响应所需用的脉冲发动机数量做了离线计算,给出了计算公式.     

PAMELA observational capabilities of Jovian electrons

PAMELA is a satellite-borne experiment that has been launched on June 15th, 2006. It is designed to make long duration measurements of cosmic radiation over an extended energy range. Specifically, PAMELA is able to measure the cosmic ray antiproton and positron spectra over the largest energy range ever achieved and will search for antinuclei with unprecedented sensitivity. Furthermore, it will measure the light nuclear component of cosmic rays and investigate phenomena connected with solar and earth physics. The apparatus consists of: a time of flight system, a magnetic spectrometer, an electromagnetic imaging calorimeter, a shower tail catcher scintillator, a neutron detector and an anticoincidence system. In this work a study of the PAMELA capabilities to detect electrons is presented. The Jovian magnetosphere is a powerful accelerator of electrons up to several tens of MeV as observed at first by Pioneer 10 spacecraft (1973). The propagation of Jovian electrons to Earth is affected by modulation due to Corotating Interaction Regions (CIR). Their flux at Earth is, moreover, modulated because every 13 months Earth and Jupiter are aligned along the average direction of the Parker spiral of the Interplanetary Magnetic Field.PAMELA will be able to measure the high energy tail of the Jovian electrons in the energy range from 50 up to 130 MeV. Moreover, it will be possible to extract the Jovian component reaccelerated at the solar wind termination shock (above 130 MeV up to 2 GeV) from the galactic flux.