一种地理围栏内无人机航迹跟踪方法

针对UTM体制中无人机在地理围栏内的飞行监视问题,提出一种约束状态相关模态转换混合估计算法(CSDTHE)。采用随机线性混杂系统模型对无人机运动状态进行建模,利用CV、CT和CA三种模态描述无人机的飞行状态,以构建地理围栏内无人机运行的通用模态转换模型框架。利用飞行模态改变点(FMCP)定义相关模态转换参数,设计模态转换条件,生成模态转换概率矩阵,从而建立与状态相关的模态转换模型。运用约束卡尔曼滤波(CKF)方法对直线阶段和转弯阶段的无人机运动速度分别施加等式约束,并通过仿真实验验证了CSDTHE算法对无人机跟踪的有效性。     

二维复值Ginzburg-Landau方程的一个高阶紧致ADI差分格式

对二维复值金兹堡朗道(Ginzburg-Landau,GL)方程提出一个基于时间分裂的高阶紧致交替方向隐式有限差分格式。本文通过时间分裂法将GL方程分裂成一个非线性子问题及两个线性子问题,对非线性子问题以及其中一个线性子问题均通过精确积分进行计算,并对另一线性子问题构造紧致交替方向隐式差分格式进行数值计算。实际计算中,在每一时间步,利用追赶法求解一族常系数三对角线性代数方程组,从而使得算法既具有较高精度又拥有较快的计算速度。数值实验表明该算法在时间和空间方向分别具有二阶和四阶精度,并模拟了方程的一些动力学行为。     

基于连续同伦算法的天基仅测角初定轨方法

要进一步提高天基短弧初定轨的精度,在观测资料精度较高的情况下,仅考虑二体问题是不够的,还应考虑轨道摄动的影响。因此,基于无摄初轨的单位矢量法原理和矢量斜分解方法,给出了考虑摄动的天基仅测角初定轨单位矢量法。针对天基仅测角观测条件方程组求解过程中易出现迭代不收敛或收敛到平凡解的问题,引入连续同伦算法求解观测条件方程组,提出了单星观测方式下的空间目标天基仅测角初定轨方法,并通过数值仿真算例验证了该算法在较大范围的收敛性和数值稳定性。     

圆柱-平板角区湍流流动控制的风洞试验研究

角区流动中马蹄涡系的存在通常会造成不良影响。对圆柱-平板角区流动,在圆柱上游放置一倾斜的小圆棒能够改变角区流动结构。利用油流法和平板表面压力测量方法探讨了湍流流态下不同的小圆棒对平板表面的摩擦力线和压力分布的影响。油流实验揭示了倾斜棒能够改变角区的三维分离,新的分离线由倾斜棒和圆柱共同作用引起;倾斜棒对角区的作用可归类为两种不同的物理现象;倾斜棒能够引起圆柱侧面的分离线向下游发生极大的迁移,导致圆柱底部区域尾迹变窄。平板表面压力测量实验揭示附加的倾斜棒能够极大地改变压力分布情况,角区的逆压梯度相应减小;由此,逆压梯度引起的三维分离必然被削弱。     

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.     

自适应神经模糊推理模型在复杂社会技术系统中的应用(英文)

考虑复杂社会技术系统的特点,运用自适应神经模糊推理模型对提高公益科研机构的组织效率进行了实例研究。建立了针对公益科研机构员工激励决策的自适应模糊推理完整模型,利用调研数据及其处理结果验证了模型的有效性。该模型融合了神经网络的学习机制和模糊系统的语言推理能力,弥补了神经网络和模糊逻辑系统各自的不足。研究结果表明,自适应神经模糊推理模型适用于复杂社会技术系统,在解决管理领域的预测、评估和决策问题中有广阔的应用前景。     

基于波动耦合的复杂结构动力响应分析与研究

有限元法(FEM)适合低频分析,统计能量分析(SEA)方法适合高频分析,而一类较宽频带(中频段)的声振响应问题不适合单独用FEM或SEA方法解决。基于波动耦合的混合FE-SEA方法兼顾了FEM与SEA方法的优点,可预测中频段含一定不确定性的声振系统的稳态响应。本文阐释了混合FE-SEA方法的理论,分别通过典型结构的蒙特卡罗仿真与复杂系统的噪声试验两案例对该方法进行了验证,其中梁-板典型结构能量响应计算值与蒙特卡罗仿真值具有较好的一致性;复杂飞行器系统的振动响应与试验结果较为吻合,舱内噪声声压级(SPL)误差小于3dB,证明了混合FESEA方法的有效性,解决了FEM与SEA方法在中频复杂声振响应中的局限性这一问题。     

穿越微下冲气流的飞翼布局无人机控制方法

微下冲气流是最危险的低空风切变形式,为在起降阶段安全穿越该气流,飞翼布局的无人机控制律应具有快速响应能力和良好的鲁棒性。针对大展弦比飞翼布局无人机舵面附加升力大和低速状态俯仰操纵效能低的特点,提出了舵面附加升力和机体气动力相结合的复合控制方案,改进了以输出误差为参考量的非线性指令分配策略,设计了基于迎角保护的指令分配策略。将风干扰和模型的不确定性视为未知扰动,采用自抗扰控制(ADRC)理论设计飞翼布局无人机非线性控制律,使之对风干扰和模型的不确定性进行估计补偿。仿真结果表明,复合控制与ADRC相结合的方法加速了航迹倾角的单位阶跃响应速度,使上升时间缩短了64%,同时能够实现对风干扰的有效观测和补偿,使高度损失低于2m;能够在风切变中有效保护迎角,使其维持在5.5°以内。因此,该方法能够为飞翼布局无人机安全平稳地穿越微下冲气流提供一种参考方案。     

地球静止轨道微波辐射计技术

静止轨道微波辐射计可实现全天时、全天候、高频次云雨大气观测,在台风、流域性强降水探测和预报方面发挥重要作用。但在波束扫描、多频复用、系统定标等方面的运用存在较大困难,世界上尚无在轨应用先例。现从探测需求出发,对静止轨道微波辐射计进行了系统方案设计。提出了卫星平台与辐射计部件快慢结合扫描的方法,以解决波束扫描和系统定标难题;提出了低频选入射角层叠式布局准光学频段分离方法,以解决多频段复用难题。研制了微波辐射计原理样机,通过实验室和外场试验验证了系统设计,为静止轨道微波探测卫星研制提供了一定指导。     

工艺参数对砂布轮柔性抛光力影响规律的分析

为了掌握砂布轮抛光工艺参数对抛光力的影响规律，提高抛光质量，设计了四因素三水平正交试验，利用试验结果建立了抛光力预测模型，验证了模型的显著性；分析了工艺参数对抛光力耦合影响规律，结果表明：抛光力随砂布轮初始半径和粒度的减小而增大，随转速和压缩量的增大而增大；对叶片进气边的抛光实验效果表明：通过控制压缩量可以获得稳定的抛光力，进而获得理想的抛光效果。