内装式空射运载火箭重力出舱机箭耦合动力学分析

研究了以运输机为平台的内装式运载火箭空射过程载机和火箭的耦合动力学建模。建模针对两个阶段：第一阶段，火箭固定于载机机舱内，两者构成一个整体，按照普通刚体的力学方法处理；第二阶段，火箭解锁后，沿着舱内的发射筒向外滑行，载机和火箭形成两刚体相互作用的耦合系统，基于牛顿-欧拉法建立系统动力学模型。载机在空射火箭过程中，油门和升降舵满偏，在加速前飞的同时拉大姿态俯仰角，火箭在自身重力分量和惯性力的作用下，沿着机舱内的发射筒加速向外滑行，直至与载机分离。数值仿真分析了空射过程载机的重要力学参数的变化过程，验证了载机操控策略的可行性和安全性，可为未来中国空射运载火箭技术设计提供数据参考。     

轨控大干扰下的系统角动量管理

摘要： 针对利用角动量交换装置系统实现轨控期间姿态维持的情况，研究当轨控推力器存在大力矩扰动时系统角动量管理方法.结合对地运行航天器轨道运动特性，分析轨控干扰力矩的积累角动量变化规律；考虑角动量管理装置系统的角动量存贮容量，基于角动量积累规律提出了一种结合偏置角动量建立与对称分布轨控位置选择的系统角动量管理方法，实现了对称轨控位置积累角动量互相抵消的自平衡效果，极大程度地提高轨控效率且避免系统角动量饱和现象.所提出的方法适用于喷气欠驱动控制系统，方法的有效性通过了数学仿真验证及在轨型号应用.     

部署retro-GEO巡视器的月球借力飞行轨道分析

retro-GEO是指逆行（retrograde）地球静止轨道（geostationary Earth orbit, GEO），该轨道与GEO轨道高度相同或相近，但倾角为180°，安装在retro-GEO卫星上的巡视器可每12h对GEO带空间资产附近碎片环境安全预警。直接西向发射retro-GEO卫星存在地面测控和发射能耗较大的困难。基于平面四体模型，为降低设计变量敏感性，以近月点参数为设计变量，建立了部署retro-GEO巡视器的月球借力飞行轨道设计模型，利用轨道动力学模型延拓策略，得到该类轨道绕月后返回地球飞行时长只能约为114.79h，该结论可用于求解该类轨道高精度轨道动力学模型解。     

An improved numerical method for constructing Halo/Lissajous orbits in a full solar system model

An improved numerical method that can construct Halo/Lissajous orbits in the vicinity of collinear libration points in a full solar system model is investigated. A full solar system gravitational model in the geocentric rotating coordinate system with a clear presentation of the angular velocity relative to the inertial coordinate system is proposed. An alternative way to determine patch points in the multiple shooting method is provided based on a dynamical analysis with Poincare′sections. By employing the new patch points and sequential quadratic programming, Halo orbits for L_1, L_2, and L_3 points as well as Lissajous orbits for L_1 and L_2 points in the EarthMoon system are generated with the proposed full solar system gravitational model to verify the effectiveness of the proposed method.     

椭圆轨道卫星对地全球覆盖电推进控制

针对椭圆轨道卫星近/远地点的星下点对全球或特定纬度区域的访问问题，提出一种连续小推力下的对地覆盖控制策略。首先，推导了自然摄动对卫星拱线变化的影响，并探讨了进行小推力覆盖控制的必要性。然后，针对燃料消耗的优化问题，将控制方程展开成含傅里叶级数的形式，用以获得便于星上计算的解析形式的次优解，同时探讨了截取阶数与优化程度的关系。在进行拱线控制的同时，通过合理设置约束，对椭圆轨道的近地点高度进行保护，确保卫星安全运行。仿真结果表明，提出的方法能够以适当的燃料消耗代价实现椭圆轨道的近/远地点的全球覆盖控制或特定纬度区域的反复推扫，且控制力在可接受的范围内。     

利用热源温度场迭加法诊断持续点热源的强度及位置

可重复使用运载器的防热瓦故障会使航天器的局部结构产牛热源，并在结构中形成温度场。应用热源温度场迭加法的解函数，解得结构温度历程，然后据此温度的变化率趋势判断出热源位置，在此基础上依据多点测最值构造出辨识参数用于热强度识别，通过对一薄壁结构模型算例的计算仿真，证明了本文所提方法的有效性。论文工作为进一步开展热源诊断技术研究，提供了可资工程实践应用的数值算法体系以及有益的数值计算结论。     

俯斜墙背条件下朗肯与库伦土压力理论的研究

从挡土墙抗滑、抗倾覆安全系数和挡土墙的主动土压力两个角度，研究建立在朗肯土压力理论与库伦土压力理论基础上的不同主动土压力计算方法所带来的误差，认为在俯斜的挡土墙墙背条件下，应使用抗滑、抗倾覆安全系数来判断土压力计算方法是否合理。     

弹道导弹自由段飞行中的守恒量及其应用

从精确弹道计算所用的数学模型出发，指出了弹性在自由段飞行中的两个具有明确物理意义的运动守恒量，并给出了用发射坐标系下的运动参数求这些守恒量的简洁计算公式。这两个守恒量可作为一种简单、实用的辅助评估手段用于计算结果可信性分析以及导弹发射诸元的校验。     

Aiming at a 1-cm Orbit for Low Earth Orbiters: Reduced-Dynamic and Kinematic Precise Orbit Determination

The computation of high-accuracy orbits is a prerequisite for the success of Low Earth Orbiter (LEO) missions such as CHAMP, GRACE and GOCE. The mission objectives of these satellites cannot be reached without computing orbits with an accuracy at the few cm level. Such a level of accuracy might be achieved with the techniques of reduced-dynamic and kinematic precise orbit determination (POD) assuming continuous Satellite-to-Satellite Tracking (SST) by the Global Positioning System (GPS). Both techniques have reached a high level of maturity and have been successfully applied to missions in the past, for example to TOPEX/POSEIDON (T/P), leading to (sub-)decimeter orbit accuracy. New LEO gravity missions are (to be) equipped with advanced GPS receivers promising to provide very high quality SST observations thereby opening the possibility for computing cm-level accuracy orbits. The computation of orbits at this accuracy level does not only require high-quality GPS receivers, but also advanced and demanding observation preprocessing and correction algorithms. Moreover, sophisticated parameter estimation schemes need to be adapted and extended to allow the computation of such orbits. Finally, reliable methods need to be employed for assessing the orbit quality and providing feedback to the different processing steps in the orbit computation process. This revised version was published online in August 2006 with corrections to the Cover Date.     

Earthshine and Asteroseismology Telescope (East) Network

Several automated optical telescopes have been setup at appropriate longitudes around the globe to study earthshine variations and asteroseismology. The first telescope has been setup at Teide Observatory, Tenerife, Spain in October 2004. The intensity of earthshine relates to the average of Earth’s albedo, and in turn relates to the global temperature of the Earth. A global network is necessary because each site can measure the earthshine reflected from only a part of the Earth. The network will also be used for asteroseismology study. It can measure photometric variations of pulsating stars. The long-term and continuous measurements allow the accurate determination of mode frequencies of stellar pulsations, which provides information on the properties of stellar interior.