Geostationary orbit determination using SATRE

A new strategy of precise orbit determination (POD) for GEO (Geostationary Earth Orbit) satellite using SATRE (SAtellite Time and Ranging Equipment) is presented. Two observation modes are proposed and different channels of the same instruments are used to construct different observation modes, one mode receiving time signals from their own station and the other mode receiving time signals from each other for two stations called pairs of combined observations. Using data from such a tracking network in China, the results for both modes are compared. The precise orbit determination for the Sino-1 satellite using the data from 6 June 2005 to 13 June 2005 has been carried out in this work. The RMS (Root-Mean-Square) of observing residuals for 3-day solutions with the former mode is better than 9.1 cm. The RMS of observing residuals for 3-day solutions with the latter mode is better than 4.8 cm, much better than the former mode. Orbital overlapping (3-day orbit solution with 1-day orbit overlap) tests show that the RMS of the orbit difference for the former mode is 0.16 m in the radial direction, 0.53 m in the along-track direction, 0.97 m in the cross-track direction and 1.12 m in the 3-dimension position and the RMS of the orbit difference for the latter mode is 0.36 m in the radial direction, 0.89 m in the along-track direction, 1.18 m in the cross-track direction and 1.52 m in the 3-dimension position, almost the same as the former mode. All the experiments indicate that a meter-level accuracy of orbit determination for geostationary satellite is achievable.     

民用飞机驾驶舱构型快速设计方法

为在方案设计阶段提高民用飞机总体方案的设计质量和形成效率,研究了民用飞机驾驶舱构型的设计措施,并在一个开放式的飞机总体设计环境中实现了这一功能.定义了飞机机身坐标系,研究了确定驾驶员设计眼位、驾驶舱布置和风挡参数化设计与模型构建的方法.建立了交互式民机驾驶舱构型二、三维快速设计环境.在此基础上,实现了驾驶舱模型的自动化调整,为总体设计阶段进行多学科设计优化奠定了基础.通过设计实例证明了该方法的有效性.     

前缘吹气控制舵面流动分离

针对各种飞行器大舵偏下出现的流动分离问题,在北航D4风洞对旨在消除舵面流动分离的舵面前缘吹气技术进行了研究,为了降低控制分离所用的吹气量,吹气点设置在舵面前缘气流分离点处.应用粒子图像测速(PIV,Particle Image Velocimetry)技术,分析了舵面绕流在吹气量由小变大过程中所经历的3个不同演化阶段;由测压得到的舵面压力分布则显示,前缘吹气造成的引射作用使前缘吸力峰随吹气量增大而增大,这是前缘吹气能够使舵面升力增大的主要机理.实验结果还表明,前缘吹气可明显提高舵面升力,同时也可以显著降低舵面阻力.     

多星联合任务规划方法

针对多星对地观测系统联合任务规划问题,考虑卫星载荷具备连续侧摆能力和多种数据压缩模式的新特点,构建了多星联合任务规划模型,在此基础上设计多星联合任务规划和数传调度算法框架,实现了卫星连续侧摆成像规划算法和基于任务优先级的数传任务调度算法,最后采用实际算例进行试验,结果表明文章提出的多星联合任务规划方法能在提高完成任务数量的同时降低卫星资源消耗,满足实际应用需求。     

我国空间电力线谐波辐射现象分析

研究了利用DEMETER卫星电磁场探测数据辨识电力线谐波辐射(PLHR,Power Line Harmonic Radiation)事件的方法,探讨了我国空间中PLHR事件的特点.通过采用时频分析和Welch功率谱估计法分析了2005-2010年6年我国空间中的全部卫星电场强度探测数据,共发现151例PLHR事件,给出了PLHR事件的统计分析和典型实例.结果表明我国空间PLHR事件的频率分布在1 000~4 500 Hz之间,多为50 Hz的奇数倍,间隔为50/100 Hz.PLHR事件与我国电网发展和变化有密切关系,与地磁活动水平无关,呈现出昼夜差异和季节差异.最后给出了影响PLHR事件探测的可能因素.     

基于空间映射的视觉注意力分配预测模型

为预测飞行员视觉注意力分配,在SEEV(Salient Effort Expectancy Value)模型和多因素模型的基础上引入注意控制空间和资源分配空间的概念.前者描述了影响注意力分配因素,而后者则反应了兴趣区域所获得的注意资源.并通过空间映射建立注意力分配的预测模型,应用模糊层次分析的方法对模型进行结算.为验证预测模型效度,采用16名被试在飞行模拟器上开展基于异常信息恢复的工效学实验,通过眼动追踪装置记录注视点分布作为注意力分配指标.被试需要根据实验条件对主飞行显示器仿真界面中的目标信息状态进行监视,并通过驾驶杆的指定操作对异常信息进行响应.实验结果表明,注意力分配预测模型的理论结果与工效实验中注视点分布的实验结果显著相关且吻合较好,验证了预测模型的可用性.     

A comprehensive numerical model investigating the thermal-dynamic performance of scientific balloon

The increase of balloon applications makes it necessary for a comprehensive understanding of the thermal and dynamic performance of scientific balloons. This paper proposed a novel numerical model to investigate the thermal and dynamic characteristics of scientific balloon in both ascending and floating conditions. The novel model consists of a dynamic model and thermal model, the dynamic model was solved numerically by a computer program developed with Matlab/Simulink to calculate the velocity and trajectory, the thermal model was solved by the Fluent program to find out the balloon film temperature distribution and inner Helium gas velocity and temperature field. These models were verified by comparing the numerical results with experimental data. Then the thermal and dynamic behavior of a scientific balloon in a real environment were simulated and discussed in details.     

Cosmic Ray Energetics And Mass for the International Space Station (ISS-CREAM)

The Cosmic Ray Energetics And Mass (CREAM) instrument is configured with a suite of particle detectors to measure TeV cosmic-ray elemental spectra from protons to iron nuclei over a wide energy range. The goal is to extend direct measurements of cosmic-ray composition to the highest energies practical, and thereby have enough overlap with ground based indirect measurements to answer questions on cosmic-ray origin, acceleration and propagation. The balloon-borne CREAM was flown successfully for about 161 days in six flights over Antarctica to measure elemental spectra of Z = 1–26 nuclei over the energy range 10¹⁰ to >10¹⁴ eV. Transforming the balloon instrument into ISS-CREAM involves identification and replacement of components that would be at risk in the International Space Station (ISS) environment, in addition to assessing safety and mission assurance concerns. The transformation process includes rigorous testing of components to reduce risks and increase survivability on the launch vehicle and operations on the ISS without negatively impacting the heritage of the successful CREAM design. The project status, including results from the ongoing analysis of existing data and, particularly, plans to increase the exposure factor by another order of magnitude utilizing the International Space Station are presented.     

基于流固耦合的充气翼内压对翼面变形影响分析

基于ABAQUS-FLUENT软件开展柔性充气翼流固耦合分析,采用反距离加权平均法实现耦合界面气动压力分布传递,采用常体积转换法实现变形数据传递,分析获得了充气翼翼面刚度和屈曲特性与翼面内外压差的关系;建立了充气翼模拟加载试验系统验证了分析方法的可行性.结果表明,流固耦合方法用于充气翼变形分析是可行的,分析结果与模拟试验结果能够较好地吻合.