飞机可靠性分配方法研究

针对现行飞机工程研制可靠性分配中存在的数据量少、主观因素影响较大的问题,提出了一种融合灰色关联理论与考虑重要度和复杂度的可靠性分配方法。该方法首先统计多型飞机分系统的可靠性指标,并将其代入灰色关联方法中计算各分系统的重要度;然后统计飞机各系统重要和新研改进部件数,利用考虑重要度和复杂度的分配方法对飞机可靠性指标进行分配。以某型飞机为案例进行分析计算,结果表明,该方法简单有效,客观性强。     

椭圆轨道非线性相对运动模型的周期解与应用

在长期的航天器编队飞行中传统的基于线性相对运动模型设计编队保持轨道的方法会引起较多的燃料消耗.首先采用摄动法解析地求得了考虑二阶非线性项时椭圆轨道相对运动模型的周期性条件和周期解;然后以此周期解为参考轨道设计了基于Lyapunov稳定的PD保持控制律.仿真结果表明:基于椭圆轨道非线性相对运动模型的周期解较基于椭圆轨道线性相对运动模型的周期解,精度明显提高;以前者为参考轨道的保持控制与以后者为参考轨道的保持控制相比,燃耗明显降低.     

多模型直接自适应执行器故障补偿控制系统

为了更快更好地补偿执行器故障带来的不确定性,发展了一种新的多模型自适应执行器故障补偿控制系统设计方法。首先,分析所有可能的执行器故障模式,得到故障模式集。再针对每一种故障模式,分别进行控制器设计,控制器设计时采用直接模型参考自适应执行器故障补偿控制方法进行设计。然后根据参数估计误差分别计算每种故障模式下系统的性能损失函数,选择性能损失最小的子系统对应的控制器作为当前的全局控制器。最后以飞行控制系统为例进行了仿真,仿真结果表明,所设计的多模型直接自适应执行器故障补偿系统闭环稳定,且有良好的跟踪性能。     

深空探测中多普勒的建模与应用

针对深空探测中的多普勒观测资料的单程和三程模式,分别给出了瞬时和积分的观测模型,双程多普勒观测模型是三程模式的一个特殊情况.通过比较瞬时和积分多普勒的差异,推断在积分周期取得足够小时,瞬时观测模型与积分模型是一致的.利用2009年8月份对火星探测器MEX的三程多普勒测轨资料的处理,检验了三程多普勒资料观测模型的正确性,利用约一个圈次8小时三程多普勒数据进行轨道计算,定轨结果与欧空局重建轨道位置差约几百米.     

基于H∞最优化与层次结构动态逆的非线性飞行控制器设计

针对扰动环境下的导弹飞行控制问题提出一种基于H∞最优化与层次结构动态逆(HSDI)的鲁棒非线性控制方法.设计层次结构动态逆控制器时将层次结构优化为3层,并按照时标分离的思想调整了各层次的状态变量,使得控制器更为简洁.在此基础上,将层次结构动态逆控制器与导弹6自由度(DOF)非线性模型联合作为H..控制的广义被控对象,通...     

A Modeling Language Based on UML for Modeling Simulation Testing System of Avionic Software

With direct expression of individual application domain patterns and ideas,domain-specific modeling language(DSML) is more and more frequently used to build models instead of using a combination of one or more general constructs.Based on the profile mechanism of unified modeling language(UML) 2.2,a kind of DSML is presented to model simulation testing systems of avionic software(STSAS).To define the syntax,semantics and notions of the DSML,the domain model of the STSAS from which we generalize the domain co...     

周向总压畸变条件下多级轴流压气机失速首发级预测分析

基于多级轴流压气机的逐级特性,发展了1种预测周向总压畸变条件下多级轴流压气机失速首发级的方法。该方法结合平行压气机模型和级叠加计算方法,以进气畸变条件下多级轴流压气机某级的有效相对气流角达到稳定状态时该级的最大相对气流角为条件,进行多级轴流压气机失速首发级的预测分析。通过对J85—13发动机8级轴流压气机总压畸变试验数据进行模拟计算,预测出该轴流压气机畸变条件下的失速首发级。     

Feasibility of performing space surveillance tasks with a proposed space-based optical architecture

Under ESA contract an industrial consortium including Aboa Space Research Oy (ASRO), the Astronomical Institute of the University of Bern (AIUB), and the Dutch National Aerospace Laboratory (NLR), proposed the observation concept, developed a suitable sensor architecture, and assessed the performance of a space-based optical (SBO) telescope in 2005. The goal of the SBO study was to analyse how the existing knowledge gap in the space debris population in the millimetre and centimetre regime may be closed by means of a passive optical instrument. The SBO instrument was requested to provide statistical information on the space debris population in terms of number of objects and size distribution. The SBO instrument was considered to be a cost-efficient with 20 cm aperture and 6° field-of-view and having flexible integration requirements. It should be possible to integrate the SBO instrument easily as a secondary payload on satellites launched into low-Earth orbits (LEO), or into geostationary orbit (GEO). Thus the selected mission concept only allowed for fix-mounted telescopes, and the pointing direction could be requested freely. Since 2007 ESA focuses space surveillance and tracking activities in the Space Situational Awareness (SSA) preparatory program. Ground-based radars and optical telescopes are studied for the build-up and maintenance of a catalogue of objects. In this paper we analyse how the proposed SBO architecture could contribute to the space surveillance tasks survey and tracking. We assume that the SBO instrumentation is placed into a circular sun-synchronous orbit at 800 km altitude. We discuss the observation conditions of objects at higher altitude, and select an orbit close to the terminator plane. A pointing of the sensor orthogonal to the orbital plane with optimal elevation slightly in positive direction (0° and +5°) is found optimal for accessing the entire GEO regime within one day, implying a very good coverage of controlled objects in GEO, too. Simulations using ESA’s Program for Radar and Optical Observation Forecasting (PROOF) in the version 2005 and a GEO reference population extracted from DISCOS revealed that the proposed pointing scenario provides low phase angles together with low angular velocities of the objects crossing the field-of-view. Radiometric simulations show that the optimal exposure time is 1–2 s, and that spherical objects in GEO with a diameter of below 1 m can be detected. The GEO population can be covered under proper illumination nearly completely, but seasonal drops of the coverage are possible. Subsequent observations of objects are on average at least every 1.5 days, not exceeding 3 days at maximum. A single observation arc spans 3° to 5° on average. Using a simulation environment that connects PROOF to AIUB’s program system CelMech we verify the consistency of the initial orbit determination for five selected test objects on subsequent days as a function of realistic astrometric noise levels. The initial orbit determination is possible. We define requirements for a correlator process essential for catalogue build-up and maintenance. Each single observation should provide an astrometric accuracy of at least 1”–1.5” so that the initially determined orbits are consistent within a few hundred kilometres for the semi-major axis, 0.01 for the eccentricity, and 0.1° for the inclination.     

CubeSail: A low cost CubeSat based solar sail demonstration mission

CubeSail is a nano-solar sail mission based on the 3U CubeSat standard, which is currently being designed and built at the Surrey Space Centre, University of Surrey. CubeSail will have a total mass of around 3 kg and will deploy a 5 × 5 m sail in low Earth orbit. The primary aim of the mission is to demonstrate the concept of solar sailing and end-of-life de-orbiting using the sail membrane as a drag-sail. The spacecraft will have a compact 3-axis stabilised attitude control system, which uses three magnetic torquers aligned with the spacecraft principle axis as well as a novel two-dimensional translation stage separating the spacecraft bus from the sail. CubeSail’s deployment mechanism consists of four novel booms and four-quadrant sail membranes. The proposed booms are made from tape-spring blades and will deploy the sail membrane from a 2U CubeSat standard structure. This paper presents a systems level overview of the CubeSat mission, focusing on the mission orbit and de-orbiting, in addition to the deployment, attitude control and the satellite bus.     

一种提高卫星相对轨道运动全物理仿真逼真度的新方法

现有的卫星控制系统全物理仿真很少对卫星绕地球的轨道运动进行模拟,即使在卫星间相对轨道运动的全物理仿真中也没有考虑地心引力差和惯性力项的存在,因此其逼真度受到了影响.提出一种在共面圆轨道近距离卫星相对运动全物理仿真中引入地心引力差和惯性力项的方法,提高了物理仿真实验的逼真度.