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.     

谈飞机结构装配工艺中几个细节问题的完善

基于飞机生产过程中长期固存的问题进行要点采摘,对于操作者在生产过程中的认识误区、原因分析做出比较详尽的叙述,对于完善设计和改良产品质量能够提供一定的帮助.     

直升机/粒子分离器一体化流场特性: 第一部分 前进比的影响

针对典型布局条件下直升机/粒子分离器的一体化流动特性进行了仿真研究.利用相关试验数据对仿真方法的有效性进行了检验,将整体式粒子分离器安装至类“阿帕奇”直升机外型上,形成了一种典型直升机/粒子分离器布局方案,并分析了其在不同前进比下的一体化流场特性.结果表明:较高前进比下,在粒子分离器进口上游的齿轮箱外罩上出现了复杂的三维流动分离,使得粒子分离器在较不均匀的进口来流条件下工作.与独立粒子分离器状态相比,一体化条件下粒子分离器主流出口、扫气流出口的总压损失均有所加大,增幅分别为1%和8%.      

Relationship Between Substorm Auroras and Processes in the Near-Earth Magnetotail

Although the auroral substorm has been long regarded as a manifestation of the magnetospheric substorm, a direct relation of active auroras to certain magnetospheric processes is still debatable. To investigate the relationship, we combine the data of the UV imager onboard the Polar satellite with plasma and magnetic field measurements by the Geotail spacecraft. The poleward edge of the auroral bulge, as determined from the images obtained at the LHBL passband, is found to be conjugated with the region where the oppositely directed fast plasma flows observed in the near-Earth plasma sheet during substorms are generated. We conclude that the auroras forming the bulge are due to the near-Earth reconnection process. This implies that the magnetic flux through the auroral bulge is equal to the flux dissipated in the magnetotail during the substorm. Comparison of the magnetic flux through the auroral bulge with the magnetic flux accumulated in the tail lobe during the growth phase shows that these parameters have the comparable values. This is a clear evidence of the loading–unloading scheme of substorm development. It is shown that the area of the auroral bulge developing during substorm is proportional to the total (magnetic plus plasma) pressure decrease in the magnetotail. These findings stress the importance of auroral bulge observations for monitoring of substorm intensity in terms of the magnetic flux and energy dissipation.     

Properties of Interplanetary Coronal Mass Ejections

Interplanetary coronal mass ejections (ICMEs) originating from closed field regions on the Sun are the most energetic phenomenon in the heliosphere. They cause intense geomagnetic storms and drive fast mode shocks that accelerate charged particles. ICMEs are the interplanetary manifestations of CMEs typically remote-sensed by coronagraphs. This paper summarizes the observational properties of ICMEs with reference to the ordinary solar wind and the progenitor CMEs.     

基于量子行为鸽群优化的无人机紧密编队控制

随着军事、民用需求的提高和相关领域的技术推动,无人机编队协同作业已成为当今人们逐渐关注的焦点。无人机紧密编队是指无人机间侧向距离在1~2倍翼展内的编队,因其可有效改善编队中无人机的气动性能而备受瞩目。基于无人机紧密编队条件下的气动耦合效应,建立三维空间下的状态空间方程描述双机相对运动,并推导了紧密编队条件下的双机最优编队构型,在此构型下将人工势场法和编队控制相结合作为控制系统中的间接控制环,并针对基本鸽群优化算法的寻优缺陷利用量子行为规则对其进行改进,将改进后的鸽群优化算法和无人机控制量结合作为控制系统中的直接控制环,最后通过仿真对比验证了此控制系统对于紧密编队控制的有效性。     

双流制窄轨电力机车用异步牵引电机设计

将牵引电机应用于双流制窄轨电力机车时,由于窄轨机车轨距小,所以牵引电机安装空间异常狭小,比一般牵引电机在安装空间、电机结构、电磁负荷等方面的要求更加苛刻。针对窄轨双流制电力机车的运用特点和特殊要求进行了分析,提出了牵引电机的设计要求和关键技术难点,并对关键技术难点给出了相应的分析和解决措施。对该牵引电机的制造过程及电机试验测试情况进行了论述。试验结果表明,该牵引电机达到了设计预期,完全能满足设计要求。     

Variations of the magnetic fields in large solar flares

We present preliminary results from high resolution observations obtained with the Michelson Doppler Imager (MDI) instrument on the SOHO of two large solar flares of 14 July 2000 and 24 November 2000. We show that rapid variations of the line-of-sight magnetic field occured on a time scale of a few minutes during the flare explosions. The reversibility/irreversibility of the magnetic field of both active regions is a very good tool for understanding how the magnetic energy is released in these flares. The observed sharp increase of the magnetic energy density at the time of maximum of the solar flare could involve an unknown component which deposited supplementary energy into the system. This revised version was published online in August 2006 with corrections to the Cover Date.     

15-5PH沉淀硬化不锈钢磁粉检测磁痕分析

针对航空15-5PH马氏体沉淀硬化不锈钢在磁粉检测过程中发现的条状、片状和长直磁痕显示进行了总结。分析了不同磁痕显示的特点及微观组织情况,最终确定了磁痕的性质。结合不同热处理状态下的磁特性分析,确立了纯洁度磁粉检测的工艺流程以及磁痕判别方法。研究发现沉淀硬化不锈钢在磁粉检测过程中磁痕显示主要是由铁素体和组织不均匀造成的。研究结论为航空制造过程中沉淀硬化不锈钢的磁粉检测的磁痕判定以及规范的制定提供依据,确保磁粉检测工作的顺利进行。     

复合材料构件热压罐成型温度场研究

在热压罐固化工艺的热历程中,复合材料零件表面温度场分布的合理与否将直接决定产品的固化质量.以工字型零件和T型加筋壁板两种复合材料零件为研究对象,使用EC-3×8M和SCH-5.5×21M两种型号热压罐,同时选择炉温偶和零件偶两种控温方式对零件进行固化.通过分析温度场测试结果发现,控温方式、设备加热方式、升降温速率、热电偶的摆放位置、固化压力等因素均对零件的温度场有影响.