采用机头边条改善飞机大迎角横侧气动特性的风洞试验研究

飞机大迎角横侧气动特性是决定其机动性及敏捷性的主要因素之一。本文就采用机头边条改善飞机大迎角横侧气动特性进行了讨论。着重对机头边条的大小、安装位置等对飞机稳定性的影响进行讨论。试验是在气动中心低速所４ｍ×３ｍ和３．２ｍ风洞中进行的。     

大型太阳帆板展开状态动态特性研究

利用有限元技术及自编的 FORTRAN程序计算了单翼太阳帆板约束模态的振型和频率 ,计算结果和实验结果比较表明 ,计算精度在工程上是可以接受的。在此基础上 ,以飞船带有双翼对称太阳帆板为模型 ,计算了太阳帆板在转动和不转动情况下非约束模态的振型和频率。上述计算结果为研究带有挠性太阳帆板的航天器的动力学与控制问题打下了基础     

Review of CASC Highlights in 2010

China Aerospace Science and Technology Corporation (CASC) is a well-known aerospace company,dealing with spacecraft manufacture,operation and providing related services for government and commercial customers worldwide.     

重复率电光调Q Nd3+:YAG激光器输出能量及激光器效率的测定

本文提出了一种在不同的泵浦电压下测量重复率电光调Q掺钕钇铝石榴石激光器输出能量的方法 ,实际测量了脉冲激光器静态输出和动态输出能量 ,并利用电光晶体激光调Q技术得到脉宽为亚毫微秒的激光脉冲 ,使得激光器动态输出功率达兆瓦量级     

LC4CS铝合金裂纹尖端腐蚀行为的实验研究

ＬＣ４ＣＳ铝合金是极为重要的航空材料，为评定其使用年限，在测定铝合金腐蚀疲劳裂纹的扩展速率时，需要弄清纹尖端金属的腐蚀电化学行为。在腐蚀环境中裂纹尖端由于不断露新鲜金属，因而将具有类似于双金属腐蚀时的电偶效应。为此，文中设计了一种新颖的缺口试样，再现裂纹尖端的真实状态，并在３．５％ＮａＣｌ溶液测定剪切口断裂后，裸露出的新鲜金属在耦合前后腐蚀电位的变化，以及裸露面积，ＮａＣｌ溶液的ｐＨ值与电偶电流的     

无线电陆空通话英语交际能力模型研究

民航无线电陆空通话语言是以英语为载体的一种空地交流的特殊语言。本文在应用语言学的研究成果之上,提出了该语言的交际能力模型,该模型包括语言能力、策略能力、背景知识和心理生理机制四个部分。笔者结合民航陆空通话实际,对模型各个部分进行了分析,重点解析了策略能力在模型中的核心功能。     

一个方便实用的旋翼数据库

本文介绍了一个以EXCEL和EXCEL VB建立的旋翼数据库。并以一个分库为例介绍了建立和使用方法。     

Executive Moves of CASC

On April 15,2013,the central committee of CPC and the State Council of China decided to establish a Board of Executives for China Aerospace Science and Technology(CASC)and Mr.Xu Dazhe was appointed Chairman of CASC     

蒙特卡洛方法在降落伞-返回舱系统中的应用

文章简要介绍了蒙特卡洛方法的起源和基本思想，随机数和随机抽样的产生方法，同时，基于蒙特卡洛方法的基本思想提出了用数值方法计算飞船返回舱着陆姿态参数的初步设想。对于此问题的研究，将有助于节约试验经费，分析返回舱缓冲结构的设计合理性及可靠性。     

Plasma and electromagnetic wave simulations of meteors

Every day billions of meteoroids impact and disintegrate in the Earth’s atmosphere. Current estimates for this global meteor flux vary from 2000 to 200,000 tons per year, and estimates for the average velocity range between 10 km/s and 70 km/s. The basic properties of this global meteor flux, such as the average mass, velocity, and chemical composition remain poorly constrained. We believe much of the mystery surrounding the basic parameters of the interplanetary meteor flux exists for the following reason, the unknown sampling characteristics of different radar meteor observation techniques, which are used to derive or constrain most models. We believe this arises due to poorly understood radio scattering characteristics of the meteor plasma, especially in light of recent work showing that plasma turbulence and instability greatly influences meteor trail properties at every stage of evolution. We present our results on meteor plasmas simulations of head echoes using particle in cell (PIC) ions, which show that electric fields strongly influence early stage meteor plasma evolution, by accelerating ions away from the meteoroid body. We also present the results of finite difference time domain electromagnetic simulations (FDTD), which can calculate the radar cross section of the simulated meteor plasmas. These simulations have shown that the radar cross section depends in a complex manner on a number of parameters. These include the angle between radar and meteor entry, a large dependence on radar frequency, which shows that for a given meteor plasma size and density, the reflectivity as a function of probing radar frequency varies, but typically peaks below 100 MHz.