Libration point orbits for lunar global positioning systems

With the development of lunar exploration, a lunar global positioning system (LGPS) is demanded for both on-ground and in-flight lunar exploration missions. The traditional configuration of constellation requires at least eighteen satellites to cover the whole lunar surface continuously. In this paper, the configurations of the libration point orbits (LPOs) constellations are investigated. By using the constellations on the Earth–Moon _L1$L_1$ and _L2$L_2$ LPOs, the basic functions of the LGPS can be realized by using eight to fourteen satellites. First, the LPO and the combinations of LPOs, which can be used in the constellations of the LGPS, are investigated. The criteria and procedures of the configuration design are introduced. Second, the configurations of LPOs constellations are investigated in the Earth–Moon circular-restricted three-body problem (CR3BP). The size of the LPOs and the distribution of the satellites on these LPOs are determined by using an exhaustive algorithm and a global optimization method, respectively. The key performance parameters of these constellations are computed. Third, the constellations with good performance in the CR3BP are redesigned in the more accurate Earth–Moon based Sun-perturbed bicircular four-body problem (B4BP). Moreover, in order to avoid the ground coverage problem caused by the perturbation of the Sun, some modifications are implemented, and the configuration of the no blind area LGPS in the B4BP is obtained.     

航空嵌入式系统2000年问题分析及检测方法

通过对航空系统嵌入式计算机的应用分析,根据航空系统嵌入式计算机应用领域和重要性的不同,将航空系统分为机载电子系统,遥测与导航系统,设备开发、测试和综合系统,以及生产加工系统四个层次。并针对每个层次绝对时间的使用特征,从系统参数共享到底层电路构型,提出了各自相应的 Ｙ２ Ｋ 问题检查方法,以及相应的检查内容和责任单位。     

关于计算机2000年问题的探讨

计算机２０００年问题已引起人们的普遍关注,必须在进入２０００年前予以妥善解决。对其可采用修改应用程序、更换系统软件、更换硬件设备等多种办法进行处理。在应用程序的修改中采用变形的日期移位法是对大多数办公系统容易实现且又行之有效的办法。     

多尺度子域基函数矩量法解的稳定性与迭代法

通过对几个具体实例的计算，证实了在电磁场边值问题的矩量法求解过程中，选用不同的基函数其解的数值稳定性会有很大的差别。从而有可能选择一种数值稳定性比较好的基函数来进行矩量法求解。另一方面，提出了选用多尺度子域基函数，并通过多次迭代来提高矩量法解的精度的算法。实例计算表明，该算法不仅可以有效地降低系数矩阵的条件数，而且还降低了对计算机内存容量的要求，是一种有效的、稳定的算法     

地月循环轨道动力学建模与计算研究

根据地月循环轨道的概念,按照生成第二类周期轨道的弧段进行分类,并讨论了其共振性与对称性在轨道设计与应用中的作用。然后归纳了三种循环轨道的动力学建模与计算方法及其轨道延拓策略,最后总结了三种方法的利弊和应用轨道类型。对地月系统循环轨道的研究和分析,能够为我国未来载人登月工程提供一种新的思路与理论支持。     

大型自由曲面光学器件的超精密抛光方法

旨在提高大尺寸自由曲面光学器件精密抛光技术的精度与效率。通过构建一个机器人抛光中心作为抛光平台,并在包括单位圆域、单位正方形域及自由边界域在内的平面映射域内求解旅行商问题,通过投影计算圆形度数值,进行映射区域的分类,并将所获得的平面轨迹映射到曲面上获得用于大尺寸自由度超精密光学器件的抛光路径。本文算法综合考虑到计算效率以及边界覆盖质量:当投影区域的圆形度超过0.9,则采用单位圆域作为映射平面域;当投影区域的圆形度值相对小,介于0.8与0.9之间,则采用单位方域作为映射平面域;当圆形度值小于0.8,则采用自由边界映射域。仿真及试验验证抛光结果表明,该方法可以获得高效的无交叉路径,有效降低单一方向运行导致的中频、高频误差,满足抛光路径方向不断变化的实际抛光加工需求,有效消除抛光纹理,并显著提高抛光精度和效率。     

解析计算在月球中继卫星Halo轨道设计中的应用

面向月球中继卫星工程轨道设计需求,研究解析计算方法在地月系L2点halo轨道设计中的应用问题。在讨论圆型限制性三体问题三阶解析近似计算方法的基础上,分析了解析计算与数值计算的差异,给出了解析近似计算在工程约束下的适用范围,进而提出了基于解析计算的轨道设计和特征筛选方法。分别采用解析初值和数值初值进行halo轨道外推,比对验证采用解析计算设计轨道的可行性。研究结果表明,解析计算方法适用于月球中继卫星轨道的初步设计、特征分析和构型筛选。     

复合式共轴直升机过渡模式的操纵策略

根据复合式共轴直升机的构型特点,建立了上/下旋翼、机翼、机身、全动平尾、垂尾（含方向舵）和螺旋桨的气动力模型,并在此基础上建立了过渡过程的配平方程.针对过渡飞行过程的操纵冗余问题,分别采用线性过渡和功率最小优化过渡两种过渡飞行方案,对复合式共轴直升机的过渡飞行过程的操纵策略进行了研究.以样例复合式共轴直升机为例,进行了过渡飞行模式下两种操纵策略的配平计算,并对两种过渡操纵策略下的需用功率、操纵量和姿态进行了对比.结果表明:所述两种过渡方案均能解决操纵冗余问题,并能合理给出过渡模式的操纵量和姿态.在操纵量变化的平稳度、飞行控制的难易程度和飞行品质方面,线性过渡方案更优.      

Thick galactic cosmic radiation shielding using atmospheric data

NASA is concerned with protecting astronauts from the effects of galactic cosmic radiation and has expended substantial effort in the development of computer models to predict the shielding obtained from various materials. However, these models were only developed for shields up to about 120 g/cm² in mass thickness and have predicted that shields of this mass thickness are insufficient to provide adequate protection for extended deep space flights. Consequently, effort is underway to extend the range of these models to thicker shields and experimental data is required to help confirm the resulting code. In this paper empirically obtained effective dose measurements from aircraft flights in the atmosphere are used to obtain the radiation shielding function of the Earth's atmosphere, a very thick, i.e. high mass, shield. Obtaining this result required solving an inverse problem and the method for solving it is presented. The results are shown to be in agreement with current code in the ranges where they overlap. These results are then checked and used to predict the radiation dosage under thick shields such as planetary regolith and the atmosphere of Venus.