基于模型的液体推进系统故障诊断算法

给出串联双涡轮结构以泵作为供应系统的液体火箭发动机系统故障仿真的准动态数学方法和基于灰色关联度分析的实时诊断算法。该算法对于调整计算确定的具体系统和预先设定的典型故障模式进行仿真计算、事先形成该发动机系统的故障模式样本集。试车时, 利用诊断算法对采集的发动机性能参数进行实时分析, 从而给出发动机所处的健康状况, 以便及时采取措施, 提高发动机的安全性和可靠性。      

空间辐射致冷器辐射耦合视因子的积分解法

本文以镜面反射成像理论为基础,提出了一种空间辐射致冷器表面热耦合视因子的积分解法。推导了有关的数学模型,给出了计算机程序的框图和典型的计算结果。     

跨音速平面叶栅全位势无粘-粘性迭代计算

本文发展了一种全位势与附面层、尾迹流正逆模式积分法迭代计算程序,给出了计算结果与国内外四个不同的叶栅风洞试验结果的对比分析。结果表明,对比是较为满意的,本文在网格生成,无粘跨音流求解和无粘流与附面层、尾迹流迭代等方面所作的发展和改进适用,使整个程序系统具有工程实用价值。      

基于自适应神经网络的非线性飞行控制

结合反馈线性化和神经网络提出了一种新的飞行控制系统设计方法,通过反馈线性化将非线性耦合系统等效转换为线性解耦系统,利用具有在线学习能力的神经网络补偿反馈线性化的误差,建立了基于自适应神经网络的控制结构,并利用李亚普诺夫函数导出了网络权值的自适应调整规则。在巡航弹地形跟踪应用中的结果表明,该控制系统不仅具有精确的跟踪性能而且具有良好的鲁棒性。     

重特征值模态灵敏度分析的非线性摄动法

利用非线性摄动等式,推导了实对称矩阵的重特征值模态灵敏度计算公式。该方法的优点是保持了原特征系统矩阵的对称性和带宽。数值算例表明该方法精度高,易于计算和实施。     

月面冯·卡门撞击坑的着陆选址和科学探测目标浅析

冯·卡门（Von Kármán）撞击坑位于月球背面南极—艾肯（South Pole-Aitken,SPA）盆地中部,是中国“嫦娥4号”计划的优先级较高的探测目标。对该撞击坑的着陆和探测,有助于揭示月球形成和演化的一些关键问题,在月球科学研究中具有重大的意义。论文概要总结了冯·卡门撞击坑的研究意义和科学价值;结合LRO卫星LOLA数据、Clementine UV-VIS数据、GRAIL数据、“嫦娥2号”卫星CELMS等数据,简要分析了冯·卡门撞击坑的地形、成分、深部结构和亮?%rater are analyzed with LRO satellite LOLA data,Clementine UV-VIS data,GRAIL data,and Chang''E-2 CELMS data and their scientific meanings are also presented. Finally,combined with our results and the previous prospects about theVon Kármán crater,three candidate landing sites and the possible scientific discoveries are proposed.     

简谐激励下大型低温贮箱防晃设计

针对某大型低温贮箱,基于水平环形防晃板和竖直防晃板设计了一种布置于整个贮箱的固定结构防晃板,采用CFD软件Flow-3D数值模拟了一定简谐激励下,不同充注率时该防晃板的防晃效果.通过与液面水平环形防晃板对比发现:两种结构防晃效果相近,均可以显著抑制不同充注率下液体的质量中心波动范围.当充注率为50%时,两防晃结构甚至可以使波动范围减小64%;在晃动过程中,相比于液面水平环形防晃板,固定结构防晃板中单层水平环形防晃板的受力更小,但是贮箱受到的压力会有所增加;对比相同面积液面水平环形防晃板和竖直防晃板的防晃效果,液面水平环形防晃板优势更加明显;随着充注率的增大,液体在贮箱内晃动时液体的质量中心波动范围逐渐减小.      

On the observability of Mars entry navigation using radiometric measurements

A thorough observability analysis of the Mars entry navigation using radiometric measurements from ground based beacons is performed. This analysis involves the evaluation of the Fisher information matrix which is derived from the maximum likelihood estimation. A series of navigation cases with multiple beacons are investigated, and both range and range-rate measurements are considered. The determinant of Fisher information matrix is used to quantify the observability of navigation system, while the trace of Fisher information matrix is used to determine the lower-bound of estimation errors. For one and two beacon cases, the navigation system is unobservable. However, the eigenvectors of Fisher information matrix give the observable and unobservable component. When three or more beacon measurements are employed, the states of entry vehicle become observable. Some valuable analytic conclusions on the relationship between the geometric configuration of beacons and observability are obtained consequently. Finally, simulation results from two navigation examples indicate that our effort is useful for understanding and assessing the observability of the Mars entry navigation using radiometric measurements.     

An innovative navigation scheme of powered descent phase for Mars pinpoint landing

Pinpoint landing (within 100 m from the target) is essential for future Mars exploration missions. This paper deals with one aspect of the pinpoint landing architecture—the navigation performance improvement during the powered descent phase, and proposes an innovative navigation scheme to obtain the vehicle complete and accurate states. On the basis of dead reckoning relying on the Inertial Measurement Unit, measurements of the Integrated Doppler Radar are adopted to correct the vehicle velocity and altitude. Distance between the vehicle and one Mars Orbiter as well as their line-of-sight relative velocity is measured by a radio sensor, and integrated in the filter to correct the vehicle horizontal position. The innovative navigation system is based on an Extend Kalman Filter. Two observation schemes are developed. One considers measurements of the Integrated Doppler Radar and radio range measurement. Another further considers radio velocity measurement. The performance of the innovative navigation scheme is greatly influenced by the position of the Mars Orbiter with respect to the target. Stochastic analyses are performed to obtain optimal locations of Mars Orbiter. Finally, the innovative navigation scheme performances are assessed through stochastic simulations. Its performance improvements are demonstrated by comparison with the Integrated Doppler Radar only navigation scheme.     

行星着陆探测中的动力学与控制研究进展

着陆探测是获取行星特性和科学数据最直接、最有效的途径,也是目前技术难度最大、最为复杂的探测方式。在行星着陆探测过程中,动力学与控制是影响任务成败的关键因素之一。文章首先分析了行星着陆探测动力学与控制研究所面临的挑战与难题;然后,针对火星和小行星的着陆探测,重点分析了火星着陆进入段和下降段所涉及的动力学与控制,小行星附着探测动力学建模与制导控制的研究现状与关键问题;最后,提出了我国在行星着陆探测动力学与控制领域的未来重点发展方向。