以外加辅助件推迟三角翼上涡破裂的初步水洞实验

对尖锐前缘、后掠角为60°的大攻角平板三角翼模型进行了水洞实验。利用附加的小辅助件,改变翼面上方的流场,使机翼前缘肌体涡推迟破裂。流动显示表明:在翼面上的适当位置安放圆弧形或三角形导流体,或在翼面上方另加一辅助小三角翼,能使涡破裂推迟的效果得到显著提高。此结果可供推迟涡破裂来改善飞机气动性能的研究工作参考。     

系统存在干扰及建模误差时的稳定自适应控制算法

 <正> 1.问题叙述 研究模型参考自适应控制系统,在不考虑系统的外界干扰及建模误差时如图1所示。     

液体火箭发动机基于主要目标的减损与延寿控制方法

首先通过构造目标函数、提取约束条件与问题解的分析,对液体火箭发动机减损与延寿控制技术的优化问题进行了数学描述,然后以某大型液氧/煤油火箭发动机为对象,考虑其涡轮叶片为关键部件,研究了发动机起动过程减损控制律综合分析的主要目标法,并在不同的约束条件下,对实现不同意义下的减损控制进行了仿真计算.结果表明该方法可行且有效,能够有效实现系统性能与关键部件损伤间的权衡并实现预期的减损目标,结果为工程中液体火箭发动机的改进和优化设计提供了重要的参考价值.      

基于Modelica和Dymola的航空发动机燃气发生器的建模与性能仿真

基于对压气机、涡轮与燃烧室共同工作条件的分析,建立了1种快速简便的单轴燃气发生器性能仿真模型;用Modelica语言和Dymola编译器实现了单轴燃气发生器的性能仿真,验证了该模型的有效性。结果表明:该模型能够模拟单轴燃气发生器的性能,并能实现非设计转速小流量工况下的性能仿真。     

基于域对象的文本过滤模型

提出了一种基于域对象的文本过滤模型,该模型采用改进了的基于概念的向量空间模型来表示域对象模型。在过滤过程中,先建立域对象模型,然后将待过滤文本进行信息提取、文本分析,建立待过滤文本的临时模型,通过模型匹配来判断待过滤文本是否属于过滤范畴。实验证明该模型有较好的过滤性能。     

作战飞机信息系统通用服务中间件研究

根据作战飞机数据传输的特点,对作战飞机综合信息系统进行了需求分析。在此基础上,提出了基于通用技术平台的系统的互联、互操作的体系框架。对作战飞机信息系统通用服务中间件声明管理服务和对象管理服务进行了设计,解决了作战飞机信息系统通用服务中间件的关键技术研究。该作战飞机信息系统通用服务中间件的应用将具有重大的军事价值。     

一种三维空间9-交模型的简化方法

9-交模型是一种表达三维空间拓扑关系的常用方法,但存在着冗余度大等问题。本文在Z latanova简化9-交模型工作的基础上,定义了点、线、面和体等简单三维空间对象,对它们之间的拓扑关系进行了研究。排除各种不可能的情况,共总结出24种可能的9-交结果以及80种点线面体之间的拓扑关系,并进行归类得到55种拓扑分析操作,从而大大简化了原模型。以线与体的拓扑关系分析为例,给出了根据简化以后的9-交模型进行拓扑分析操作的具体算法实现。     

Comparative analysis of global optical observability of satellites in LEO

With a growing number of resident space objects (RSOs), the facilities for near-Earth space surveillance have to cope with increasing workload. It also applies to low-cost small optical surveillance facilities which may present regional, national and global networks. Improved methods of planning and scheduling optical telescopes are required to use these instruments efficiently. Today, optical observations are only feasible if the following quite stringent requirements are met: the object should be illuminated by sunlight, and it should be above while the Sun is below the observer’s horizon. For different orbits, these preconditions result in varying degrees of the space object observability at various ground-based sites. Certainly, satellites in low Earth orbit (LEO) are particularly difficult to observe. This study aims at developing a new technique for assessing observability of a satellite in different types of orbits – namely, low, medium and high Earth orbits, imaging of the opportunity for its visibility in respective diagrams and their analysing for the existing near-Earth population of RSOs. Unlike other researches, wherein one or several observational stations have been chosen as target sites for in-depth analyses of visibility of all the satellites or just the selected ones, the present study focuses on examining the probability of optical surveillance of satellites in a certain orbit from any locations worldwide. It offers considerable scope for automation of surveillance planning and scheduling optical surveillance networks.     

Assessment of depth to magnetic sources using high resolution aeromagnetic data of some parts of the Lower Benue Trough and adjoining areas,Southeast Nigeria

High resolution airborne magnetic data acquired between 2005 and 2010 were used to determine depth to shallow and deep magnetic sources in some parts of Southeastern Nigeria. Various depth estimation methods such as standard Euler deconvolution (SED), source parameter imaging (SPI), spectral depth analysis (SDA) and two dimensional (2-D) forward modeling were applied. Results obtained from SED, SPI and models of profiles 1 and 2 indicate that the Abakaliki Anticlinorium (AA) and Ikom-Mamfe Rift (IMR) regions are dominated by short wavelength magnetic anomalies caused by extensive tectonic events. The SED map showed depth to shallow and deep magnetic sources ranging from ~ 16.6 to ~ 338.3 m and ~ 394.3 to ~ 5748.1 m respectively. Likewise, depth estimates from the SPI map varies from ~ 147.1 to ~ 554.2 m (shallow magnetic sources) and ~ 644.2 to ~ 6141.6 m (deep magnetic sources). The result obtained from SDA revealed depths to deep magnetic basement in the range of ~ 769 to ~ 6666 m with an average of ~ 3449 m. Also, it showed that depth to shallow magnetic sources vary between ~ 119 and ~ 434 m with mean of ~ 269 m. The 2-D forward modelling showed maximum depth values of ~ 4700, ~4600 and ~ 6500 m in the models of profiles 1, 2 and 3 within the Anambra Basin (AB), Afikpo Syncline (AS) and Calabar Flank (CF) respectively. Generally, from all the various methods applied the results indicate that AB, AS and CF are dominated by long wavelength anomalies. The 2-D models indicated that the basement framework is undulant. Also, depth estimates involving the various methods used in this study correlate strongly with each other in the AB, AS and CF geological regions.     

Generic functional modelling of multi-pulse auto-transformer rectifier units for more-electric aircraft applications

The Auto-Transformer Rectifier Unit (ATRU) is one preferred solution for high-power AC/DC power conversion in aircraft. This is mainly due to its simple structure, high reliability and reduced kVA ratings. Indeed, the ATRU has become a preferred AC/DC solution to supply power to the electric environment control system on-board future aircraft. In this paper, a general modelling method for ATRUs is introduced. The developed model is based on the fact that the DC voltage and current are strongly related to the voltage and current vectors at the AC terminals of ATRUs. In this paper, we carry on our research in modelling symmetric 18-pulse ATRUs and develop a generic modelling technique. The developed generic model can study not only symmetric but also asymmetric ATRUs. An 18-pulse asymmetric ATRU is used to demonstrate the accuracy and efficiency of the developed model by comparing with corresponding detailed switching SABER models provided by our industrial partner. The functional models also allow accelerated and accurate simulations and thus enable whole-scale more-electric aircraft electrical power system studies in the future.