三维流场的计算干涉方法

计算干涉技术通过试验图像和计算图像相比较，可以验证CFD的有效性，是研究复杂流场的有力工具。作者根据M-Z干涉仪的光学成像原理，用计算机仿真实现了将数值计算获得的二维、轴对称和三维的复杂流体的密度场转换为“无限条纹”和“有限条纹”的干涉图像，尤其是在处理三维流场时，采用流场重构的方法，达到了很好的效果。     

超低比转速离心泵内流场计算及分析

运用FLUENT流体计算软件及GAMBIT前处理软件,采用三维k-ε双模型方程计算了一台高速超低比转速离心泵的内部流场。计算区域为从诱导轮进口到蜗壳出口的整个流场,通过计算得到了泵内流场的流动规律,并结合传统的泵水力估算方法,估算了泵的扬程、轴功率及效率,最后对该高速超低比转速离心泵进行了水力验证试验。验证结果表明所采用的计算方法可行。     

再入航天器陶瓷拐角环防热计算与结构适用性分析

文章基于近地轨道及探月返回再入热环境,应用超高温陶瓷到再入航天器的典型防热结构,计算分析了再入过程中的防热结构温度场。利用温度场计算结果,再结合超高温陶瓷抗烧蚀性能以及结构设计与工艺性分析,就超高温陶瓷作为再入航天器防热结构的适用性进行了深入探讨。结果表明,由于超高温陶瓷的优良耐高温及耐烧蚀性能,在近地轨道及探月返回再入航天器防热结构上具有良好的应用前景。     

Magnetic energy release near accreting black holes

The observed non-thermal emission from accreting compact objects is often understood in terms of the expected magnetic activity of accretion disks. This review discusses the constraints on this view point that can be obtained from, principally, the X-ray spectra and the X-ray variability of black hole candidates.Furthermore, the traditional view of an accretion disk corona, put forward as the source of the non-thermal emission, analogous to the solar corona is shown to be wrong on a few important points. Firstly, the density in the equilibrium accretion disk corona is extremely low. A reasonable plasma density is retained by pair production processes similar to those existing in the pulsar magnetosphere. Secondly, the dominant resistivity in the accretion the disk on the current carrying electrons.     

测速雷达的电波折射简易修正方法及精度分析

为尽量简化多测速雷达定轨系统的气象测量，探讨了采用Hopfield对流层折射指数模型代替探空气象测量的适用性。主要分析了采用Hopfield模型与采用实际探空测量数据的折射误差修正量差别，目标轨迹误差对修正量的影响，以及气象参数对修正量的影响。     

一种双脉冲发动机的技术研究

提出了一种带有中间喷管的新型双脉冲固体火箭发动机技术方案，设计了一台结构参数可调的试验发动机；改变发动机的结构参数进行多次点火试验，获得了试验数据；对该发动机的多喉道流动过程建立了二维非稳态流动模型，对试验方案进行了大量计算，并与试验数据进行了比较分析。试验结果与理论计算基本吻合，结构可靠，对工程设计有参考价值     

Force-free magnetic field in a cylindrical flux rope without a constant alpha

It is generally assumed that magnetic fields inside interplanetary magnetic clouds and flux ropes in the solar photosphere are force-free. In order to model such fields, the solution of rot B = B is commonly used where  = const. But comparisons of this solutions with observations show significant difference. To treat this problem,we examine the solutions with .     

Coronal streamers' theories

Some theoretical aspects of solar coronal streamers are discussed with emphasis on the current sheet and reconnection processes going on along the axis of the streamer. The dynamics of the streamer is a combination of MHD and transport, with acceleration of particles due to reconnection and leakage of plasma outwards as a slow solar wind as the observable results. The presence of the almost-closed magnetic bottles of streamers that can store high-energy particles for significant times provides the birdcage for solar cosmic rays, the reconnection in the sheet feeds medium-energy protons into the corona for the large-scale storage needed for certain flare models, and the build-up of excess density sets the stage for coronal mass ejections.     

某舰飞行甲板区域流场特性的水洞试验

为了满足舰载直升机的需要，南航直升机技术研究所对某舰飞行甲板区域流场进行了水洞试验。本文详述了水洞试验的方法和技术，通过对舰模在各种水速、各种航行偏角状态下的试验，得到了大量照片，并据此对该舰机库后部、飞行甲板上部周围流场进行了分析，得出了在飞行甲板机库门外有一趋于收缩的稳态区，随着流速Ｖ的增大，这一区域变短。稳态区之后很快变为乱流区。从侧面上看，稳态区高度有从降低再向上扩散的趋向。在向右偏航时，     

扇面波导宽面横缝的等效参量

给出扇面波导ＴＥ模式场分量的近似表达式，根据等效原理，应用矩量法求解了扇面波导宽面窄横缝口面电场的分布，研究了散射参数，归一化等效串联阻抗，谐振电阻，谐振长度等重要参数。