以太阳风为源水分子在月球空间环境中的分布特征

近年来,越来越多的观测结果均显示月球上存在水.本文通过运用Monte-Carlo方法及基于能量守恒的有心力场中粒子轨道算法对水分子在近月表的输运过程进行建模,得到了水分子在近月表分布随时间演化的图像.模拟结果显示,分布在高纬地区的水分子较同经度的中低纬地区要多,这与目前探测得到的结论是一致的.同时,对最终进入永久阴影区的水分子的百分比进行了统计,在光解离常数为6.4×104s的情况下,有大约4.12%的水分子会被永久阴影区存储下来,这个比例与前人估算结果相吻合.      

嫦娥二号探测器轨道确定与支持

针对嫦娥二号探测器直接进入地月转移轨道、距月面100km高度捕获月球、完成既定任务后飞往日地第二拉格朗日平动点等飞行轨道方面的新特点,分析了定轨预报策略,利用事后精密轨道,全面评估了关键变轨点定轨预报和变轨后快速定轨的精度,其中,近月制动前3h定轨预报至近月点的位置误差为1km,速度误差为 0.3m/s 。利用不同月球引力场模型进行环月轨道精密定轨,根据实测数据残差分析和精密星历比对的结果,采用SGM100h引力场模型的定轨残差均方根最大。此外,针对嫦娥二号扩展任务,分析了不同测轨条件下的定轨精度,测量数据残差分析结果表明,在扩展任务中途修正前的定轨弧段内,测距、时延和时延率数据的残差分别为5m,5ns和1ps/s。     

极地科考小型无人飞行器

针对小型无人飞行器在极地科考中的抗风扰动问题,通过神经网络改进卡尔曼滤波算法,提高小型无人飞行器对环境的适应性.基于小型无人飞行器自身状态信息与误差信息,在线调整系统的量测噪声和估计参数,提高信息融合精度;利用矢量域方法构建轨迹跟踪控制算法,基于目标航迹在线调整航向,提高小型无人飞行器在顺风、逆风、转弯的飞行品质和压航线精度.经过大量的仿真试验、实际飞行试验验证了方法的有效性,改进的卡尔曼滤波算法可以提供长时高精度信息,小型无人飞行器可以在野外6级风源扰动的情况下,实现稳定飞行,平均误差不超过10m.小型无人飞行器在南极实地科考中得到成功应用.     

巡视器对地指向受月表地形的影响分析

对探月巡视器在静止状态和移动状态下的测控状态包括高低角和方位角进行了计算分析,计算考虑了理论状态以及叠加了虚拟地形的两种情况,分析了月表地形起伏对测控状态的影响。文章首先给出了着陆点在理论静止状态下高低角和方位角的计算结果以及与卫星仿真工具包(STK)的比对分析情况;其次考虑到月表地形的存在,构造一种虚拟地形,在月球车给定的行走路线上分析了地形对测控方位的影响。     

Multi-objective output-feedback control for microsatellite attitude control: An LMI approach

Mixed H₂/H_∞ output-feedback controller with pole placement constraints against the internal uncertainty of moment-of-inertia variation and space environmental disturbances is proposed for mircosatellite attitude control. The multi-objective controller is designed based on linear model of attitude dynamics. The H_∞ performance takes into account both robustness stability against moments-of-inertia uncertainty and the disturbance rejection aspect. H₂ performance takes into account the LQG aspect which avoids the undesirable wheels’ saturation effect. In addition, the closed-loop poles can be forced into some sector of the stable half-plane to obtain well-damped transient responses. The problem is then reduced to a convex optimization involving linear matrix inequalities (LMIs), so it can be efficiently solved. The simulation results demonstrate that the presented mixed H₂/H_∞ control system is robust stable and optimal in the sense of H₂ norm, and has good steady-state and dynamic performances against the parameter uncertainties and various disturbances for the microsatellite attitude control system.     

月球精确定点软着陆轨道设计及初始点选取

研究了一种应用参数化控制求解月球探测器精确定点软着陆最优控制问题的方法。 首 先用约束变换技术将不等式约束进行了近似处理,而后利用若干个分段的常数去逼近最优解 ,再根据强化技术通过时间轴上的变换,将每一段参数的持续时间转变为一组新的参数,于 是最优控制问题被转化为一系列参数优化问题。最后应用经典的参数优化方法即可求得最优 控制函数的一个近似解,通过增加参数个数,重复优化得到逼近连续最优解的参数化解。同 时在优化过程中考虑了制动初始点的选取对结果的影响。仿真结果表明了所提设计方法是简 单、有效的。〖JP〗     

模拟月壤钻进负载分析与试验研究

月壤与采样机具间的相互作用在月球自主采样器的设计、性能评价、控制和仿真等方面具有重要作用,目前对于月壤与采样机具间相互作用中的钻进负载研究尚不充分。本文基于被动土压力理论,根据不同的土体切削状态,将切削刃前土体分为堆积区和破坏区,重点分析堆积区土体和破坏区土体对总钻头负载的贡献,建立了月壤取心钻头钻进松散土体的钻进负载模型。HIT 2型取心钻头和HIT\|LS1#模拟月壤的钻进试验结果表明,钻进负载理论模型与实际情况具有较高的吻合度。     

本科秘书学概论教材建设探析

当前秘书学概论教材存在诸多不足。只有从端正教材编写态度、正确认识秘书学概论课程的地位和作用、明确学生就业实际出发,通过加强社会、学校、学生调研,统筹规划秘书学概论教学内容．创新教材叙述模式,加强教材多样化、立体化建设等途径,才能提高教材质量。     

Towards a cooperation between the arts,space science research and the European Space Agency – Preliminary findings of the ESA Topical Team Arts and Sciences (ETTAS)

The arts offer alternative insights into reality, which are explored by science in general, and broadened by the activities conducted by the European Space Agency [4] and other space agencies. Similar to the way the members of ESA are ambassadors for spaceflight and science, artists and cultural professionals are ambassadors for human expression, experimentation, and exploration. In June 2011, the ESA Topical Team Arts and Sciences (ETTAS) held a three-day workshop at the European Astronaut Centre in Cologne, Germany. During this workshop, topics and ideas were discussed to develop initiatives between the arts, sciences and ESA. The aim was to foster and expand the human and cultural aspects of space exploration, and at the same time offer a means of communication that aims to reach audiences beyond the scope of traditional space-related channels. The consensus of the team was that establishing and sustaining a transdisciplinary professional community consisting of ESA representatives, scientists and artists would fuel knowledge transfer, and mutual inspiration. Potential ways to provide a sustainable cooperation within and between the various groups were discussed. We present the preliminary findings including a number of measures and mechanisms to initiate and conduct such an initiative. Plausible organisational measures, procedures and consequences, as well as a proposition on how to proceed are also discussed. Overall, the involvement and cooperation between the arts, space science research and ESA will enhance in the citizens of the ESA member states the sense of public ownership of ESA results, and participation in ESA?s research.     

Instrument study of the Lunar Dust eXplorer (LDX) for a lunar lander mission

One of the highest-priority issues for a future human or robotic lunar exploration is the lunar dust. This problem should be studied in depth in order to develop an environment model for a future lunar exploration. A future ESA lunar lander mission requires the measurement of dust transport phenomena above the lunar surface. Here, we describe an instrument design concept to measure slow and fast moving charged lunar dust which is based on the principle of charge induction. LDX has a low mass and measures the speed and trajectory of individual dust particles with sizes below one micrometer. Furthermore, LDX has an impact ionization target to monitor the interplanetary dust background. The sensor consists of three planes of segmented grid electrodes and each electrode is connected to an individual charge sensitive amplifier. Numerical signals were computed using the Coulomb software package. The LDX sensitive area is approximately 400 cm². Our simulations reveal trajectory uncertainties of better than 2° with an absolute position accuracy of better than 2 mm.