复合材料机翼结构形状/尺寸综合优化设计

提出了一种复合材料机翼结构的形状／尺寸综合优化设计方法,对形状／尺寸综合优化问题进行解耦处理,得到了一种双层循环优化策略。采用均匀设计法给出若干样本点,使用准则优化手段进行尺寸优化设计,构造了形状设计变量与尺寸优化结果之间的二次多项式响应面模型,采用复合形法完成了基于响应面的形状优化设计。最后,对某型大展弦比飞翼结构进行了优化设计。优化算例结果表明,所提方法可行且有效,有较高的优化效率。     

基于模糊综合函数的目标识别融合及B/S模式在智能监控中的应用

针对虹桥机场通信管网人井的监控问题,本文利用基于模糊综合函数的目标识别融合理论实现多传感器决策级数据融合,提高通信人井井盖监测的准确性,并以B/S模式构建分布式通信人井多传感器集中智能监控系统。这两种理论保证了本套在线实时监控系统成功地应用于虹桥机场,保证了机场的通信管网安全畅通。     

DFD风洞测控系统设计

DFD风洞测控和数据采集处理系统以工业控制计算机为核心,通过PCL-818A/D数据采集卡完成试验数据采集、反馈信息入口和控制指令出口,实时进行实验条件监测。系统软件采用VB6.0编制,实现了风洞风速闭环控制、模型姿态处理调整、流场品质测量及全机模型低速风洞实验等。该系统造价低,操作界面友好,使用维护方便,具有很好的实用性。     

A lunar L2-Farside exploration and science mission concept with the Orion Multi-Purpose Crew Vehicle and a teleoperated lander/rover

A novel concept is presented in this paper for a human mission to the lunar L2 (Lagrange) point that would be a proving ground for future exploration missions to deep space while also overseeing scientifically important investigations. In an L2 halo orbit above the lunar farside, the astronauts aboard the Orion Crew Vehicle would travel 15% farther from Earth than did the Apollo astronauts and spend almost three times longer in deep space. Such a mission would serve as a first step beyond low Earth orbit and prove out operational spaceflight capabilities such as life support, communication, high speed re-entry, and radiation protection prior to more difficult human exploration missions. On this proposed mission, the crew would teleoperate landers/rovers on the unexplored lunar farside, which would obtain samples from the geologically interesting farside and deploy a low radio frequency telescope. Sampling the South Pole-Aitken basin, one of the oldest impact basins in the solar system, is a key science objective of the 2011 Planetary Science Decadal Survey. Observations at low radio frequencies to track the effects of the Universe’s first stars/galaxies on the intergalactic medium are a priority of the 2010 Astronomy and Astrophysics Decadal Survey. Such telerobotic oversight would also demonstrate capability for human and robotic cooperation on future, more complex deep space missions such as exploring Mars.     

一种数据采集卡自动校准系统及关键技术研究

数据采集卡已成为航空航天设备、现代武器装备生产验证、维修保障系统的重要部分。介绍了一种专用数据采集卡自动校准系统,分析了设计背景及实现的功能,同时提出了校准过程中噪声抑制、通道低电势和控制高可靠性三项关键技术的解决途径。     

提高无人机飞控系统数据采集准确度的算法准则

综述了无人机飞行控制系统各种参数采集、融合准确度对飞控系统稳定性的影响,提出了提高飞行控制系统各种参数采集、融合准确度的算法基本准则。     

基于多传感器数据融合技术的力学量测量系统研究

多传感器的数据融合已经在系统智能检测领域得到越来越多的应用,本论文针对传统的数据融合算法未考虑传感器自身可靠性这一不足,分析了面向传感器可靠性的数据融合算法,并在多元力学参数检测系统中加以应用,给出了系统的总体框架,并对数据融合的具体应用进行了分析,这对于进一步提高力学参数的智能传感检测及数据融合的研究具有一定的借鉴意义。     

对称加密数据随机性定量研究

通过对加密数据使用原理以及应用范围的分析,阐述了一种基于正态分布和卡方分布的加密数据随机性定量技术。结合M atLab中现有函数erfc（x）以及chi2cdf（x,y）,计算并绘制出随机性定量图,实验分析了不同对称加密算法密文随机程度,为加密数据识别提供强有力的技术支撑。     

Radio-faint BL Lac objects and their impact on the radio/gamma-ray connection

Radio and gamma-ray emissions in Active Galactic Nuclei (AGNs) are both related to the presence of relativistic particles in jets. With the advent of the Fermi Large Area Telescope (LAT), and thanks to its large sensitivity up to several GeV, many observational results are changing our understanding of these phenomena. BL Lac objects, which made up only a fraction of the known extragalactic gamma-ray source population before Fermi, have now become the most abundant class. However, since they are relatively weak radio sources, most of them are poorly known as far as their parsec scale structure and multi-wavelength properties are concerned. For this reason, we have selected a complete sample of 42 low redshift BL Lacs (independently of their gamma-ray properties) to study with a multi-wavelength (radio, optical, X-ray, gamma-ray) approach. Here, we present results and images of sources in the sample (most of which have never been observed before), using new VLBA observations at 8 and 15 GHz. Beyond this sample of BL Lacs, the population of gamma-ray AGNs has also dramatically enlarged in the Fermi era, permitting us to discuss the presence of a correlation between radio and gamma-ray properties with improved statistical significance. We explore the radio-gamma relation with several hundreds sources and using both simultaneous and archival radio data, thus tackling the impact of time variability.     

Observations of Extended Radio Emission in Clusters

We review observations of extended regions of radio emission in clusters; these include diffuse emission in ‘relics’, and the large central regions commonly referred to as ‘halos’. The spectral observations, as well as Faraday rotation measurements of background and cluster radio sources, provide the main evidence for large-scale intracluster magnetic fields and significant densities of relativistic electrons. Implications from these observations on acceleration mechanisms of these electrons are reviewed, including turbulent and shock acceleration, and also the origin of some of the electrons in collisions of relativistic protons by ambient protons in the (thermal) gas. Improved knowledge of non-thermal phenomena in clusters requires more extensive and detailed radio measurements; we briefly review prospects for future observations.