利用常规风洞进行二元翼型试验的竖置全跨方法

采用竖置全跨试验方案,在CARDC(中国空气动力研究与发展中心)4米×3米风洞进行了几个二元翼型模型风洞试验。最初选用的模型是NASA GA(W)-1翼型,并作为校验模型。试验雷诺数高达4.69×100~6,攻角范围为-10～24°,试验结果相当满意。     

应用Fuzzy ISODATA方法选择航空科研项目

 本文将Fuzzy ISODATA方法用于科研项目的选择,并结合中国航空发动机涡轮冷却专业的科研选题实例进行了定量分析。用Fuzzy ISODATA方法将14个备选项目按其对总目标的贡献值划分为3类。结果表明,该方法具有划分合理,结果直观,计算速度快便于对大量项目进行选择的优点。     

相位信息在故障诊断中的应用

 在故障诊断中,人们多从频域中寻找特征,但对于转子系统,许多故障的特征是相似的。相位作为旋转机械里一个很实用的量,在故障诊断中一直没有得到很好的应用,本文指出的相位计算和测量概念和方法,旨在进一步识别故障。     

粘性跨音速喷管流场计算

本文继用隐式近似因子分解法成功地计算无粘跨音速喷管流场之后,用同样的方法,结合任意曲线坐标系,通过非定常方程在相当长时间后的定常解,针对矩形截面喷管和轴对称喷管粘性跨音速流场,求解了可压缩层流薄层N-S方程,获得了核心流,特别是边界层中的流动参数.对于矩形截面和轴对称两种喷管进行了计算,其结果和实验数据相当一致.将本文的方法应用到粘性两相流动计算,可望较多的节省机时.     

光学测距传感器的工程计算

由于光学测距传感器能够有效地避开敌方电磁干扰并对目标距离进行测量,因而在现代飞机上仍然得到了广泛应用.本文从光学测距传感器的工作原理及其测距的工程实现方法入手,给出了一种通过数据融合的方法对目标距离信号的采集方式进行改进的方法.改进后的方法其实际测距曲线更接近于原理曲线,与传统的折线逼近法相比,有效地减小了测距信号的误差.由于测距信号精度的提高,航空武器系统的命中精度也得到了提高,使得飞机的作战效能得以提高.     

基于高度分集的两波束米波雷达测高方法及其应用

米波雷达的波束较宽、由于地面反射引起波瓣分裂,通常只能估高而不能用来测高.针对这一难题本文提出一种基于高度分集的两波束米波雷达测高方法.该方法采用高度不同的两个天线,利用波瓣分裂情况及相互相位关系来测量目标高度.文章分析了此方法测高的精度及影响精度的一些因素.本测高方法已应用于某型雷达信号处理机中,并取得良好效果.     

磁悬浮火箭发动机推力测试台

将电磁悬浮技术用于火箭发动机推力测试试验台是一次新的尝试。本文给出了应用电磁悬浮技术的发动机推力测试试验台的结构,推导了系统的运动方程,并对试验台进行了系统仿真。最后对整个试验台成功进行了多发现场试验,仿真结果和试验结果都表明电磁悬浮技术用于火箭发动机推力测试是成功的,提高了测试系统的性能和推力测试精度。     

Semi-analytic Solution of Steady Temperature Fields During Thin Plate Welding

Usually, it is very difficult to find out an analytical solution to thermal conduction problems during high temperature welding. Therefore, as an important numerical approach, the method of lines （MOLs） is introduced to solve the temperature field characterized by high gradients. The basic idea of the method is to semi-discretize the governing equation of the problem into a system of ordinary differential equations （ODEs） defined on discrete lines by means of the finite difference method, by which the thermal boundary condition with high gradients are directly embodied in formulation. Thus the temperature field can be obtained by solving the ODEs. As a numerical example, the variation of an axisymmetrical temperature field along the plate thickness can be obtained.     

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.     

Geoeffectivity of Coronal Mass Ejections

Coronal mass ejections and post-shock streams driven by them are the most efficient drivers of strong magnetospheric activity, magnetic storms. For this reason there is considerable interest in trying to make reliable forecasts for the effects of CMEs as much in advance as possible. To succeed this requires understanding of all aspects related to CMEs, starting from their emergence on the Sun to their propagation to the vicinity of the Earth and to effects within the magnetosphere. In this article we discuss some recent results on the geoeffectivity of different types of CME/shock structures. A particularly intriguing observation is that smoothly rotating magnetic fields within CMEs are most efficient in driving storm activity seen in the inner magnetosphere due to enhanced ring current, whereas the sheath regions between the shock and the ejecta tend to favour high-latitude activity.