有无中心锥圆排波瓣喷管引射器内流场模拟与比较

用数值模拟手段研究了中心锥增进圆排波瓣喷管引射器内热混合流场的影响 ,推导了非正交曲线坐标系下有无中心锥圆排波瓣喷管引射器内流场的基本方程 ,采用 SIMPLEC算法和一种完全压力修正方法 ,以物理平面速度分量作为求解变量 ,以逆变速度作为界面流速 ,在同位网格上求解了有中心锥波瓣喷管引射器内的流场控制方程 ,并与实验测量结果和无中心锥的数值计算结果进行了比较。结果表明 ,计算结果与测量值符合较好。有中心锥的低温等值线可以延伸至中心轴线 ,与在没有中心锥的情况下 ,混合管中心轴线处的温度始终保持为高温状态有很大的不同。从而找到了有中心锥的圆柱混合管热混合效率大于没有中心锥的根本原因     

多线程控制技术在面向对象实时仿真中的应用

随着实时仿真复杂性的提高,单个的处理器不足以完成所有的必需仿真计算任务。希望能在不同的处理器上完成实时仿真的不同任务,对称多处理器的机制需要软件支持,以使每个处理器通过共享内存进行信息交换。利用多线程控制技术,可以在非全进程开销或不使用共享内存的条件下,使用多处理器。其理由在于线程本身就蕴涵有共享地址的概念。一个多线程的实时程序,利用其中的主线程控制其它的辅助线程,每个处理器用于完成一个辅助的实时计算线程,主线程负责实时时钟的监控,当时钟到达时,启动相应的辅助线程,辅助线程利用图形用户界面(GUI)来监控仿真的进行。     

直升机航姿信号仿真研究及其在电子特设系统综合模拟试验中的应用

本文介绍了某直升机电子特设系统综合模拟试验的直升机运动仿真模型,在此基础上着重对直升机航姿信号两种仿真方法进行了详细的阐述,并对两种方法的仿真试验结果进行了分析比较,指出了各自的优缺点。     

二维Euler方程的非结构网格再生成自适应方法

给出了提高二维Ｅｕｌｅｒ方程定常解质量的非结构网格自适应方法和模拟结果。流场算法为结点型有限体积法和Ｌａｘ－Ｗｅｎｄｒｏｆｆ格式，网格用阵面推进法生成，生成初始网格时使用均匀的直角坐标背景网格。     

The Extreme Ultraviolet Imager Investigation for the IMAGE Mission

The Extreme Ultraviolet Imager (EUV) of the IMAGE Mission will study the distribution of He⁺ in Earth's plasmasphere by detecting its resonantly-scattered emission at 30.4 nm. It will record the structure and dynamics of the cold plasma in Earth's plasmasphere on a global scale. The 30.4-nm feature is relatively easy to measure because it is the brightest ion emission from the plasmasphere, it is spectrally isolated, and the background at that wavelength is negligible. Measurements are easy to interpret because the plasmaspheric He⁺ emission is optically thin, so its brightness is directly proportional to the He⁺ column abundance. Effective imaging of the plasmaspheric He⁺ requires global `snapshots in which the high apogee and the wide field of view of EUV provide in a single exposure a map of the entire plasmasphere. EUV consists of three identical sensor heads, each having a field of view 30° in diameter. These sensors are tilted relative to one another to cover a fan-shaped field of 84°×30°, which is swept across the plasmasphere by the spin of the satellite. EUVs spatial resolution is 0.6° or 0.1 R _E in the equatorial plane seen from apogee. The sensitivity is 1.9 count s^–1 Rayleigh^–1, sufficient to map the position of the plasmapause with a time resolution of 10 min.     

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。     

单片机在船舶位置测控系统中的应用

介绍一种以AT89C55／51单片机为核心的主从机船舶位置控制系统。驾驶员在船长室通过键盘给定理想航向信号，选择航向传感器一电罗经测出实际航向信号，将这两个信号进行运算和处理，然后发出理想的舵偏转角信号给从机。从机安装在舵机所在现场，由精密电位器测出实际的航角信号，从机将其与理想的舵角信号进行比较，并发出控制步进电机转动的信号，从而系统快速可靠地实现船舶位置的串级控制。主从机之间的通信以RS-422标准实现。文中介绍了该系统的结构，详细分析系统原理并给出软件框图。     

Recursive mode star identification algorithms

Star identification can be accomplished by several different available algorithms that identify the stars observed by a star tracker. However, efficiency and reliability remain key issues and the availability of new active pixel cameras requires new approaches. Two novel algorithms for recursive mode star identification are presented here. The first approach is derived by the spherical polygon search (SP-search) algorithm, it was used to access all the cataloged stars observed by the sensor field-of-view (FOV) and recursively add/remove candidate cataloged stars according to the predicted image motion induced by camera attitude dynamics. Star identification is then accomplished by a star pattern matching technique which identifies the observed stars in the reference catalog. The second method uses star neighborhood information and a catalog neighborhood pointer matrix to access the star catalog. In the recursive star identification process, and under the assumption of "slow" attitude dynamics, only the stars in the neighborhood of previously identified stars are considered for star identification in the succeeding frames. Numerical tests are performed to validate the absolute and relative efficiency of the proposed methods.     

三角翼低速动态大攻角气动特性试验研究

对后掠角分别为X=60°、70°和80°尖前缘平板三角翼模型和一个前缘后掠角为（76° 40°）的双三角翼模型在低速风洞中作大攻角俯仰摩波运动，振幅am=30°、60°和90°，缩减频率K=0.01～0.12，基于根弦长雷诺数Re=2.76×10^5～8.23×10^5。进行了六分量动态气动载荷测量，动态流动显示和70°三角翼上翼面非定常压力测量，并分别与对应的静态试验结果比较。分析了运动参数包括缩减频率、振幅和Re数、后掠角对气流动态迟滞特性的影响。