结构参数对圆转矩形喷管换热的影响

为了解结构参数对圆转矩形内喷管再生冷却换热的影响，设计了多个圆转矩形喷管，考虑了三种结构参数：转方位置、出口高宽比和出口圆角大小的影响。采用有限体积法求解三维可压缩的N-S方程对其内部流动和换热进行了数值模拟。湍流模型采用标准的k-ε双方程模型，壁面附近的流动和传热采用壁面函数法处理，速度与压力的耦合采用SIMPLE算法求解。结果表明：在型面一阶导数连续的情况下，转方位置对圆转矩形内喷管的换热影响不大；出口高宽比对圆转矩形内喷管的换热影响较大，出口高宽比不能太小，否则影响内喷管流场和换热；出口圆角大小影响内喷管周向上的温度分布，圆角太小造成周向温度分布不均匀。     

高速铁路隧道初始压缩波一维流动模型的数值分析方法

基于隧道内空气流通截面是时间和距离的二元函数条件与一维流动理论,提出了高速列车驶入设有缓冲结构隧道端口时产生初始压缩波的数值分析方法。一维流动理论采用考虑摩擦、传热以及空气质交换等因素的一维可压缩非定常不等熵流动模型。数值分析方法采用广义黎曼变量特征线法。与国外有关未设缓冲结构、开孔型与未开孔型缓冲结构的隧道端口三种情况的现车试验结果进行了比较,表明本文所建方法正确、合理,能够模拟计算多种类型缓冲结构条件下的压缩波波动规律。     

异种金属材料磁脉冲焊接技术

通过对磁脉冲焊接技术结合机理的阐述,采用5A03Al-5A06Al、1050Al-AZ31Mg异种金属材料进行焊接试验.对所得的焊接接头进行气密性试验和剥离试验,检测其结合质量;结合光学显微镜,对比分析Al-Al、Al-Mg焊接接头的微观形貌特点;并采用SEM/EDS分析界面附近的元素分布;最后通过硬度试验,检测接头界...     

连续旋转爆震波细致结构及自持机理

基于化学非平衡流解耦方法和详细化学反应机理,在0.1mm的网格尺度下对连续旋转爆震波内流场和爆震波平掠惰性气体界面的传播过程进行了数值模拟。详细分析了连续旋转爆震波的空间结构,由于在出口侧无几何约束,受一系列稀疏波的影响,旋转爆震波强度受到不同程度的削弱,形状也发生了相应的变化。爆震波平掠惰性气体界面时的流场分布与连续旋转爆震波结构极为类似,对比研究了波前可燃气体层高度对爆震波结构和传播过程的影响,当爆震波高度较小时,其抵御惰性气体侧稀疏波衰减的能力弱,波阵面严重变形,爆震波解耦。若爆震波要稳定自持传播,其必须要达到一定的临界高度来抵御稀疏波的影响。     

旋转固体火箭发动机内弹道理论与实验研究

本文系统地总结了我们在旋转固体火箭发动机内弹道理论与实验研究方面的某些成果，其中包括含铝丁羟推进剂的试片实验和装药发动机实验以及燃速敏感性预示和内弹道预示，得出了一些有益的结论，可供发动机设计及推进剂配方设计参考。     

多臂协调操作自由飞行空间机器人的位置和内力混合控制

基于多臂自由飞行空间机器人多臂协调操使负载沿着期望的轨迹运动并且控制负载所受的内力为目的，在多臂自由飞行空间机器人系统协调操作的动力学方程基础上，推导了各个机械臂协调操作负载按期望轨迹运动时各个机械臂关节的驱动力矩的计算方法；给出了作用在负载的内力的定义，根据关节力矩计算方法和PID反馈控制原理，建立了多臂自由飞行空间机器人协调操作负载时的位置和内力的控制算法；讨论了所提出的控制算法的稳定性问题，得到了负载的位置误差和内力误差的约束条件。通过仿真实验证明该控制算法能够使负载的实际位姿和内力收敛到期望的轨迹和内力。     

电磁波与TVP相互作用

基于时变等离子体(TVP)的场方程,根据麦克斯韦方程,推导了TVP对入射电磁波的频率上移、时间衰减常数、反射系数,以及TVP的透射波和反射波电场幅值计算公式。通过实例计算分析了不同时间的新波频率、时间衰减常数和电场幅值。方法简单易行,可为TVP的应用提供一定的理论依据。     

Gravity waves generated by thunderstorms: South-East Asia tropical region study

Gravity waves are recognized as an integral part of earth’s atmosphere which are mainly responsible for energy and momentum distribution among different layers and regions in the atmosphere. Various sources present in land, ocean, and atmosphere such as mountains, convection, jets and fronts etc. are responsible for gravity waves generation. Thunderstorms (deep convection) are one of the major sources of gravity waves in the tropical region, capable of generating waves with a wide range of frequencies and scales and significantly affecting the existing waves. Previous numerical studies have characterised the wave properties that are generated from thunderstorms, but there are no statistically quantified studies. In this paper, we have modelled the relationship between the latent heat generated inside a thunderstorm and the gravity wave properties at the geo-collocated points. Gravity waves are identified over Singapore radiosonde station (with data available until 30?km altitude with 12?h temporal resolution) in the stratosphere using wavelet studies. Based on the GROGRAT ray tracing methods to identify the thunderstorm locations, and RAMS cloud-resolving models simulations to obtain the latent heating of the thunderstorm, a regression analysis is performed using 200 cases of gravity waves. Furthermore, cloud-top momentum flux analysis is performed for various cases latent heat. This study is expected to provide more quantified and concrete information on the coupling between the thunderstorm and gravity wave which includes the variance in these relationships due to wave frequency spectrum and generation mechanisms.     

二维装药内弹道数值模拟改进方法

研究了长细比大的管形装药固体火箭发动机在燃烧过程中的侵蚀燃烧和滞点漂移现象，视燃烧产物为准定常流动，使用分段解析法，进行内流场的数据模拟，并对滞点漂移进行了计算。     

Magnetospheric and ionospheric manifestations of interplanetary foreshocks

The geometry of a typical interplanetary shock front in the vicinity of the Earth’s orbit predicts that the leading edge of the foreshock region comes into contact with the magnetosphere a few hours ahead of geomagnetic sudden impulses (SI). There is reason to believe that the interaction of the magnetosphere with the foreshock leads to magnetic and ionospheric disturbances, which can be detected by ground-based instruments. We searched for specific precursors of SIs in data from the Scandinavian riometer network and in the short period geomagnetic pulsation data from mid-latitude magnetometers. We found that SIs were preceded by the following three features: (1) an increase in riometric absorption, (2) excitation of Pcl magnetic pulsations and (3) a spectral broadening of the Pc3 magnetic pulsations. Our observations may be useful for the study of acceleration processes in the solar wind. These observations are also of potential forecasting interest.