失重条件下对称充液陀螺的不稳定行为研究

对于质心固定的，充满粘性均匀液体的旋转对称陀螺在失重条件下绕对称长轴旋转态的小扰动不稳定及其极限行为进行了研究，所给出的定理3比以往的不稳定定理[4]为强，且反映的信息量多很多。关于初始大扰动后的渐近行为，对文[8]已给出但未严格证明的两条定理给出了严格证明，它由定理1和定理2所描述。     

月球探测机器人运动控制算法研究

针对常规模糊控制的不足 ,本文提出一种模糊神经网络自适应控制 ,它综合模糊控制与神经网络控制各自的优点 ,实现模糊控制的智能化 ,并将其应用于月球探测机器人的运动控制中。仿真结果证明该控制方案的优越性、有效性和可行性     

月球遥感立体测绘技术的发展

对国外月球探测测绘历程进行了调研总结,并针对立体观测、干涉雷达测量、扫描激光测绘等3种主要的测绘方案进行分析比较,继而提出适合中国月球探测目标的三维遥感测绘成像技术途径。     

基于日地月方位信息的月球卫星自主导航

采用自主导航技术，可以降低月球卫星的任务成本，提高其生存能力。现研究了利用太阳敏感器、地球敏感器和月球敏感器测量出的卫星-太阳、卫星-地球和卫星-月球方向矢量作为观测量，采用迭代最小二乘方法、定历元时刻的卫星状态，并以轨道预报的方式实现月球卫星的自主导航。对该自主导航算法进行了数学仿真，分析比较了敏感器精度、部分轨道参数等因素对定位精度的影响，总结了其变化规律。最后对比了迭代最小二乘方法与扩展卡尔曼滤波的导航仿真结果，结果表明前者具有更高的精度。     

Algorithm and experiments of six-dimensional force/torque dynamic measurements based on a Stewart platform

Stewart platform (SP) is a promising choice for large component alignment, and interac-tive force measurements are a novel and significant approach for high-precision assemblies. The designed position and orientation (P&O) adjusting platform, based on an SP for force/torque-driven (F/T-driven) alignment, can dynamically measure interactive forces. This paper presents an analytical algorithm of measuring six-dimensional F/T based on the screw theory for accurate determination of external forces during alignment. Dynamic gravity deviations were taken into con-sideration and a compensation model was developed. The P&O number was optimized as well. Given the specific appearance of repeated six-dimensional F/T measurements, an approximate cone shape was used for spatial precision analysis. The magnitudes and directions of measured F/Ts can be evaluated by a set of standards, in terms of accuracy and repeatability. Experiments were also performed using a known applied load, and the proposed analytical algorithm was able to accu-rately predict the F/T. A comparison between precision analysis experiments with or without assem-bly fixtures was performed. Experimental results show that the measurement accuracy varies under different P&O sets and higher loads lead to poorer accuracy of dynamic gravity compensation. In addition, the preferable operation range has been discussed for high-precision assemblies with smal-ler deviations.     

冬季中层顶区域重力波谱特性

使用DYANA试验期间19枚Chaff火箭在81—105km高度范围测量的高分辨率水平速度数据，研究标量水平速度垂直波数谱在冬季的谱特性．分析结果显示冬季平均垂直波数谱有-3．02的谱斜率，这与各种饱和理论预测的-3谱斜率很一致，提供了饱和重力波谱在冬季的观测证据．与各种饱和理论比较表明，这个冬季谱的谱振幅与线性饱和理论预测的谱振幅完全一致，但是总是小于非线性饱和理论预期的、激光雷达测量的谱振幅．这个冬季谱与最近得到的夏季饱和重力波谱一道，共同表明我们的观测结果支持了线性饱和理论，而不管季节，地理位置和高度范围的不同．由这个冬季谱估计的盛行垂直波长为15km，它比夏季的12．8km盛行垂直波长稍大．     

多约束条件下探测器击中月球的轨道设计

讨论了探测器从低高度圆型地球停泊轨道出发，沿速度方向施加脉冲推力进入登月轨道，不加制导自由飞行击中月球的轨道设计问题。考虑的约束条件包括：①着月点光照；②探测器通视；③登月轨道初速及飞行时间限制；④着月时探测器相对月面落速大小和方向限制；等等。利用理论分析和简化假设，考虑节省能量、约束条件①和②，给出了着月区域、着月日期段、着月时刻段的选择方法及算例；基于数据分析和大量计算，考虑约束条件③和④，给出了确定标准轨道的方法和算例。该思路和方法经数值仿真验证是高效实用的，可为实际工程的登月轨道设计提供重要依据     

给定条件下直接命中月球轨道计算方法

在给定飞行时间、着月时间、着月入射角及停泊轨道等约束条件下，建立飞月轨道数学模型；采用可变容差多面体算法及罚函数方法进行二点边值搜索，借助双二体理论近似确定迭代初始条件，得到满足要求直接命中月球的飞月轨道。     

背景风场对中尺度受导重力波的影响

采用重力波的大气分层全波解法，计算得出了强逆风场作用下以及无风条件下中尺度重力波受导波模的色散曲线和衰减距离曲线，结果表明，强逆风场可以使得各中尺度受导波模衰减距离明显变长，并导致不同尺度重力波的衰减距离出现峰值分布，通过分析美国MillstoneHill台站和武汉电离层观象中的TID实测结果证实了这些风场支持的远距离传播波模的存在。     

Applying the mathematical theory of stochastic processes to lunar and planetary science: the ancient oceans on Mars case

The Mathematical Statistics Theory (MST) and the Mathematical Theory of Stochastic Processes (MTSP) are different branches of the more general Mathematical Probability Theory (MPT) that represents different aspects of some physical processes we can analyze using mathematics. Each model of a stochastic process according to the MTSP can provide one or more interpretations in the MST domain. The importance of MTSP is that each such interpretation can provide large amount of new information. While large body of work on the impact crater statistics according to MST has already been done, it is yet to be investigated as to how we can model a stochastic process according to MTSP; for example, bombardment of the planetary surface or something else in a Lunar and Planetary Science (LPS) domain. In order to show possible achievements, the possible existence of a Martian ocean was chosen as a query that could be addressed through computations using presumptions according to MTSP, including probability of existence as well as lateral and vertical extent and duration of time. While the presumptions for this particular case will also be addressed in certain degree, this will be done primarily to show complexities of some physical process that can be modeled, rather than to prove correctness of the concrete values computed here. While this in itself can be the objective in some future work toward the formal proof of the probability, extent, and timing of oceans on Mars, the basic idea here is to show the basic principles of MTSP, and its potential for addressing LPS-related phenomena. Here, I attempt to show how this approach can: (1) provide large amounts of previously unknown information about physical processes on the surface of the planet, (2) lead to a better understanding of the processes that have shaped the surface of the planet, and/or (3) help constrain the amount of resurfacing. Coupled with other current methodologies, MTSP can result in a better understanding of the history of Mars, as well as other lunar and planetary bodies.