双基地天基雷达功率孔径积分析

功率孔径积是制约天基雷达系统性能的一项重要因素.从接收功率的角度给出双基地天基雷达搜索方程的详细理论推导,并通过与单基地天基雷达搜索方程的比较得出一个重要的结论--双基地天基雷达的功率孔径积在面积覆盖率和目标散射系数固定条件下,只与接收距离有关而与发射距离无关.进一步证明了地球同步卫星-飞艇双基地天基雷达系统需要更低的...     

扩频测控系统干扰容限的分析

扩频测控系统以其诸多优点正成为卫星测控的主流体制,经典分析给出扩频系统的干扰容限只是一个宽泛的界。在同时考虑输入信号强度、多址干扰等因素的情况下,对扩频测控系统的干扰容限上界进行分析推导,得出更符合实际情况的干扰容限上界的闭式表达,通过计算给出干扰容限与多址干扰、干扰容限与输入信噪比强度的关系。     

GNSS中基于双星故障的RAIM中的数学关系

从理论上推导全球导航卫星系统(GNSS)中基于双星故障的接收机自主完好性监测(RAIM)中的两个基本定理,为基于双星故障的RAIM技术提供了理论支撑。第一个定理给出了RAIM中奇偶矢量与导航误差的关系,指出了两者的统计独立性,它表明只能通过多次测量的累积以统计方法得到导航定位精度;第二个定理指出可通过偏差修正方式得到正确的导航解。这两个结论与单星故障假设条件下得到的结论是相同的,这就表明,基于单星故障假设的RAIM方法,其基本原理是可以通用于双星以至于多星故障情形的,只需在具体操作上进行适应性改进。另外,推导方法本身也提供了一种进行GNSS分析的有力工具。     

卫星海色数据融合方法概述

阐述卫星海色数据融合的基本概念和优点,总结应用在海色遥感方面的数据融合方法,通过总结对比各融合方法的优缺点,探讨在海色融合中需要注意以及需要进一步改进的各问题。     

Design of a canard configured TransCruiser using CEASIOM

CEASIOM is a multidisciplinary software environment for aircraft design that has been developed as part of the European Framework 6 SimSAC project. It closely integrates discipline-specific tools such as those used for CAD, grid generation, CFD, stability analysis and control system design. The environment allows the user to take an initial design from geometry definition and aerodynamics generation through to full six degrees of freedom simulation and analysis. Key capabilities include variable fidelity aerodynamics tools and aeroelasticity modules. The purpose of this paper is to demonstrate the potential of CEASIOM by presenting the results of a Design, Simulate and Evaluate (DSE) exercise applied to a novel, project specific, transonic cruiser configuration called the TCR. The baseline TCR configuration is first defined using conventional methods, which is then refined and improved within the CEASIOM software environment. A wind tunnel model of this final configuration was then constructed, tested and used to verify the results generated using CEASIOM.     

二元双喉道射流推力矢量喷管流动参数影响的数值研究

采用数值模拟方法研究了不同流动参数对二元双喉道射流推力矢量喷管(Dual-throat fluidic Thrust-vectoring Nozzle,DTN)内流特性和推力矢量控制效果的影响。结果表明,DTN在非推力矢量情况下,NPR在3~4范围时,推力系数较大,达到0.968,而流量系数较小,仅为0.93;NPR再增大,推力系数迅速下降。在推力矢量情况下,落压比一定时,随着次流流量比的增加,推力矢量角增加,而流量系数、推力系数、推力矢量效率减小;次流流量比一定时,随着落压比的增加,推力矢量角减小,系统推力系数先增加后减小,流量系数略微增加。     

小展弦比飞翼标模雷诺数影响数值模拟研究

采用数值模拟方法开展小展弦比飞翼标模的雷诺数影响研究。使用自行研制的多块对接结构网格亚跨超声速流场解算器程序Mbflow,计算了试验雷诺数、二倍试验雷诺数和飞行雷诺数等三种雷诺数情况下小展弦比飞翼标模的流场。通过对计算结果的分析研究,得到了不同马赫数(Ma=0.2、0.8和1.5)和攻角情况下雷诺数对小展弦比飞翼标模的气动特性和流场特征的影响规律。小攻角情况下,雷诺数主要影响摩阻的大小;而大攻角时,雷诺数对压阻也有明显影响。在亚声速时,雷诺数主要影响分离涡的起始位置和强度;跨声速和超声速时,雷诺数还会影响到激波的位置和强度。进一步研究了小展弦比飞翼标模的自准区雷诺数问题,发现试验雷诺数接近于小展弦比飞翼标模的自准区雷诺数。     

在实时嵌入式环境下利用电子盘实现大容量数据记录的软件设计研究

嵌入式环境和实时操作系统目前广泛应用于航空领域。本文在介绍嵌入式系统的基础上,重点对实时多任务环境下大容量数据记录的实现方式进行了研究和利用,最后展望了电子盘实时多任务系统中记录大容量数据的前景。     

Microwave Photonics for Modern Radar Systems

The emerging new concepts and technologies based on microwave photonics have led to an ever-increasing interest in developing innovative radar systems with a net gain in functionality, bandwidth/resolution, size, mass, complexity and cost when compared with the traditional implementations. This paper describes the techniques de- veloped in the last few years in microwave photonics that might revolutionize the way to design multifunction radar systems, with an emphasis on the recent advances in optoelectronic oscillators （OEOs）, arbitrary waveform gener- ation, photonic mixing, phase coding, filtering, beamforming, analog-to-digital conversion, and stable radio-fre- quency signal transfer. Challenges in implementation of these components and subsystems for meeting the technique requirements of the multifunction radar applications are discussed.     

Effects of in-track maneuver on Sun illumination conditions of near-circular low Earth orbits

By developing approximate analytical models considering the J₂ perturbation, the effects of an in-track maneuver on the orbital Sun illumination conditions of near-circular low Earth orbits are analyzed. First, two approximate models for the variations in orbital sunshine angles are developed, one for variations at a given time and the other for variations at a given argument of latitude. Next, two approximate models for variations in orbital arc in Earth shadow are developed, one considers the small eccentricity and the other uses the zero eccentricity. Finally, the developed approximate models are applied to analyzing the Sun illumination conditions of a typical in-track maneuver mission on a near-circular low Earth orbit. From the results obtained, three major conclusions can be drawn. First, the variations in orbital sunshine angles at a given time may reach tens of degrees when the drifting time reaches hundreds of orbital periods, and the approximate model for that situation cannot effectively approach the numerical results. Second, the variations in orbital sunshine angles for any given argument of latitude are only a couple of degrees even when the drifting time reaches 500 orbital periods, and the approximation model developed can effectively approach the numerical results. Third, for variations in orbital arc in Earth shadow, the approximate model considering the small eccentricity has simple expressions and can effectively approach the numerical results; in contrast, the approximate model using the zero eccentricity has relatively worse precision.