三维内收缩前体/进气道设计参数影响规律研究

采用有旋特征线理论求解壁面压力分布可控的内收缩基准流场,再结合流线追踪,设计了五种不同位置的矩形捕获型线的三维内收缩前体/进气道。通过数值模拟,研究了进气道捕获型线的不同径向与周向位置对进气道性能与飞行器前体纵、航向气动性能的影响规律。结果表明:三维内收缩前体/进气道产生了较大的力与力矩,对飞行器纵、航向操稳特性均有影响;捕获型线径向位置远离中心体时,有利于改善前体/进气道的纵、航向静稳定性;捕获型线沿周向位置变化时,对纵向静稳定性影响较小,捕获型线纵向面对称时,溢流口朝下,能显著提高有攻角时进气道的流量系数,但会产生较大抬头力矩,航向静稳定性也变差。     

邻域辅助径迹法提高射线追踪效率

针对面元形式的目标数据,从提高入射点求解的成功率着手,采用增加对参考路径上参考面元的相邻单元进行相交性判断的方法,并将普通径迹法的单参考路径改为双参考路径,提高了径迹法射线追踪的效率.对邻域辅助径迹法在样条曲面格式目标文件上的应用作了探讨.分析了该方法与其它方法的兼容性和对计算资源的占用情况,给出了该方法提高射线追踪速度的上限.以2个典型目标为例,对该方法的效果进行了测试.结果表明,该方法通过减少真实、遍历式追踪的次数,能将普通径迹法射线追踪过程的计算量减少到原来的1/3左右.该方法对目标具有很强的适应性,并克服了普通径迹法对射线管的划分密度的依赖性.      

复合轧辊喷射铸造成形坐标跟踪法数值模拟分析

通过计算机模拟,采用跟踪复合轧辊表面轮廓线坐标的方法(坐标跟踪法),计算复合轧辊在不同时刻的形状和尺寸.并分析各种喷射铸造工艺参数对复合轧辊形状的影响规律,模拟结果表明,辊芯平移速度和辊芯半径的变化对复合轧辊的沉积层厚度影响较大,而辊芯旋转速度和喷射距离的单独变化对轧辊沉积厚度影响很小.     

展向截断曲面乘波压缩进气道气动布局

描述了所设计的展向截断曲面乘波压缩进气道.其特点是采用曲面乘波压缩前体,前体进气道压缩面基准流场由等熵压缩波轴对称流场组成,三维乘波面采用密切曲锥方法由前缘线各点流线跟踪拟合构成流面.乘波面根据飞行器和发动机的宽度要求进行了截断.数值计算和风洞试验结果表明:与相同几何收缩比的四波系压缩进气道相比,在马赫数为4.5时,曲面乘波压缩进气道流量系数提高12%,总压恢复系数提高39%;在马赫数为6时,曲面乘波压缩进气道流量系数提高4%,总压恢复系数提高50%.超然冲压发动机性能明显提高.      

电离层短波射线追踪

本文以电离层等离子体参量的平均背景模式计算为基础, 给出一种电离层短波射线轨迹计算方法。供短波通信系统、工作于短波段的其它系统(如HF雷达的目标定位系统)及有关研究工作使用参考。      

利用转移矩阵进行姿态控制

传统欧拉角控制方法在处理大姿态角机动时往往出现奇异和交联问题。针对这一问题对欧拉角的跳变现象进行了讨论,并从飞行器实际姿态与需求姿态之间的空间关系入手,给出了一种消除欧拉角跳变现象的有效方法－转移矩阵法,仿真计算表明,该方法在大型航天器的姿态控制中可以有效地消除欧拉角奇异、交联和跳跃现象,在欧拉角跳变的情况下仍然能够实现对飞行器的控制。     

耗散大气中风场对内重力波传播的影响

使用考虑大气耗散的射线跟踪算法,计算了风场作用下重力波的传播情况.结果表明,风场对快速重力波分量影响较小,但对反射和传播区域的慢速波的影响较大,表现在顺风时使反射区范围缩小,逆风时使反射区范围扩大.在传播区,顺风场使慢速波分量的传播距离变小,传播高度降低,而逆风则使慢速重力波分量的传播距离明显增大,传播高度上升.分析表明,重力波传播的丰富多样性是由风场对波的衰减和反射等滤波作用引起的.      

Numerical simulation on antenna temperature field of complex structure satellite in solar simulator

A thermal network model is developed for studying the temperature variation of complicated structure satellite surfaces. The solar incident areas, the infrared and solar radiation transfer coefficients among surfaces are numerically simulated by means of Monte Carlo ray tracing (MCRT) method in model. The non-uniformity and the instability of solar radiation, which plays the important roles in simulating outer-space heat flux designation parameters by solar simulator, are studied for analysis variation of antenna temperature fields in detail. Results showed non-uniformity irradiation effects are greater than those of instability for this kind of geometry sheltering structure.     

Time of flight measurements over a radio link from Uppsala to Bruntingthorpe and their application to testing predictions methods that approximate the ray tracing technique

Time of flight measurements (TOF) over the radio link between Uppsala (Tx: 59.9°N, 17.6°E) and Bruntingthorpe (Rx: 52.5°N, 1.1°W) have been performed every 2 min at six frequencies (4.637, 6.954, 8.008, 10.391, 11.118, and 14.364 MHz) during the period November 2006–January 2008. Such measurements have been compared with the TOF provided by three prediction methods that approximate the ray tracing technique: IRI-95, SIRM&BR_D, and ICEPAC. The root mean square deviation (rms) between TOF monthly median measurements and TOF monthly median predictions and the differences (DP) between the length of the median and predicted ray path have been calculated. The results, which are presented in terms of rms and DP for different seasons and different time periods, have indicated that the approximate methods are inadequate and that for more accurate predictions ray tracing techniques should be applied.     

Cosmic Ray Electrons

Modulation of cosmic electrons is similar to that of nuclei, but there are clear differences. At energies below 100 MeV the electron spectrum has a negative slope, which may in some way be related to electrons released from the magnetosphere of the planet Jupiter. If there is such a relationship, its nature is not established, and alternative explanations for the upturn exist. At higher energies, electrons are predominantly negatively charged, and it is probable that the difference in net charge sign from that of nuclei is responsible for many of the observed differences in the behavior of electrons and nuclei under modulation. A consistent picture of the cosmic positron abundance and its time variation may be emerging from the world dataset.