低轨道卫星GPS精密定轨动力学方法的研究

结合低轨卫星简化动力学定轨算法,以及不同几何信息精度条件下的纯几何定轨和动力定轨精度比较,定量分析星载双频GPS实现精密定轨过程中的主要因素,得到星载GPS接收机性能设计所需的关键技术指标,为卫星精密定轨系统的顶层设计提供了科学合理的参考依据。     

基于WebGIS的卫星观测计划编制系统

用户在制定卫星观测计划时,需要知道卫星的星下点位置以及遥感器对地扫描区域的信息。通常这些信息是以数值描述的形式发给用户的,不够直观。本文介绍了一种基于WebGIS的卫星观测计划编制系统,介绍了WebGIS在计划编制系统中的应用,并从系统设计、功能、利用WebGIS进行计划策略判断方案等方面进行了深入讨论。     

0.8m 风洞风扇系统的设计和运转

为提高低速风洞的最大风速,根本的措施是设计高转速大功率的风扇系统。风扇系统的设计首先在于有一个良好的设计方法,选择高升阻比的风扇翼型,根据需要恰当地确定设计工况点,合理选择桨叶和反扭导流片的各个参数,如桨毂比、实度、升力系数和圆弧角等。设计中针对已经设计的外形,进行性能计算,可以迅速鉴别设计的优劣,检查是否能满足设计要求,节约研制成本和缩短周期。     

A null frame for spacetime positioning by means of pulsating sources

We introduce an operational approach to the use of pulsating sources, located at spatial infinity, for defining a relativistic positioning and navigation system, based on the use of four-dimensional bases of null four-vectors, in flat spacetime. As a prototypical case, we show how pulsars can be used to define such a positioning system. The reception of the pulses for a set of different sources whose positions in the sky and periods are assumed to be known allows the determination of the user’s coordinates and spacetime trajectory, in the reference frame where the sources are at rest. We describe our approach in flat Minkowski spacetime, and discuss the validity of this and other approximations we have considered.     

Evolution of periodic orbits near the Lagrangian point L2

A study of the evolution of the periodic and the quasi-periodic orbits near the Lagrangian point L₂, which is located to the right of the smaller primary on the line joining the primaries and whose distance from the more massive primary is greater than the distance between the primaries, in the framework of restricted three-body problem for the Sun–Jupiter, Earth–Moon (relatively large mass ratio) and Saturn–Titan (relatively small mass ratio) systems is made. Two families of periodic orbits around the smaller primary are identified using the Poincaré surface of section method – family I (initially elliptical, gradually becomes egg-shaped with the increase in the Jacobi constant C and elongated towards the more massive primary) and family II (initially egg-shaped orbits elongated towards L₂ and gradually becomes elliptical with the increase in C). The family I in the Sun–Jupiter and Saturn–Titan systems contains two separatrix caused by third-order and fourth-order resonances, while the Earth–Moon system has only one separatrix which is caused by third-order resonances. Also in the Sun–Jupiter and the Saturn–Titan systems, family I merge with family II, around Jacobian constant 3.0393 and 3.0163, respectively, while in the Earth–Moon system, family II evolves separately from two different branches. The two branches merge at C = 3.184515. In the Earth–Moon system, the family II contains a separatrix due to third-order resonances which is absent in the other two systems.     

基于多Agent的机群编队导航系统设计与研究

智能化建模在装备作战仿真领域中独居优势.将多Agent技术程序设计方法引入机群编队导航系统的设计中,对模型进行了顶层设计并分析了Agent子系统之间的信息交互过程,为机群编队导航系统的研发和设计提供了新的思路.     

微分对策理论及其研究现状分析

本文阐述了微分对策在经济和军事领域中的研究和应用,详尽地叙述了微分对策的分类,并采用定量和定性方法对微分对策进行了分析,指出了微分对策的研究难点,对发展趋势作了较为详细的探讨。     

Hilbert空间中严格伪压缩映像的强收敛定理

给出了一种求解严格伪压缩非自身映像不动点集上变分不等式的迭代算法，并证明了其强收敛性。此结果推广了姚永红和T．H．Kim等的研究结果。最后，进一步将结论推广到求解有限个严格伪压缩非自身映像公共不动点集上的变分不等式。     

终端区点融合进近程序设计方法研究

流量的增长导致终端区拥挤和航班延误,增大了管制压力和公司成本.以长沙黄花国际机场36号跑道为例,空城受限,4条航线汇聚一点,梯度曲折多变,航班排序难,指挥复杂度高.结合我国飞行程序设计和管制间隔要求,根据点融合的基本概念,设计跑道点融合进近程序,确定相关参数.对程序进行容量和下降梯度评估表明,静态容量可达到63架次/h,是当前运行最大流量的3.7倍;下降梯度得到明显改善,为连续下降实施奠定了基础.     

Space weather center in Japan

Progress in information technology has enabled to collecting data in near real-time. This significantly improves our ability to monitor space weather conditions. We deliver information on near real-time space weather conditions via the internet. We have started two collaborations with space weather users. One is a measurement of geomagnetically induced current (GIC) of power grids in collaboration with a Japanese power company. The other concerns radiation hazards for aircrews. The radiation exposure level for aircrews was been determined by the Japanese government by the end of 2005. The proposed upper limit is 5 mSV a year. We are actively seeking ways to contribute to this subject. Our activities at the Japanese space weather center are reported in this paper.