空间智能桁架模糊振动控制研究

研究了模糊控制应用于多输入、多输出的空间智能桁架系统的振动控制.首先建立空间智能桁架的有限元方程,在此基础上,设计了一个标准的模糊控制器,并通过选择合适的量化因子将该标准模糊控制器应用于每一对同位布置的作动器/传感器,各个控制器之间独立工作.这样就避免了设计MIMO模糊控制器带来的复杂问题.最后针对空间智能桁架进行仿真,结果表明,设计的模糊控制器可以有效抑制桁架的振动,并且具有结构简单、鲁棒性强、抑制控制溢出的优点.     

航天器交会对接中GPS的应用

卫星定位和卫星通讯是正在寻求的空间飞行器高级自主交会系统的首选测控手段。本文概述了航天器的交会对接基本要求和过程以及美国全球定位系统（ＧＰＳ）和组成、定位原理、精度和差分原理后，列出了两种形式的相对运动方程。利用运动方程求解、单纯ＧＰＳ、差分ＧＰＳ的结合，可以完成追踪航天器向目标航天器接近的整个导引过程，且可以省去庞大的地面遥控遥测、星上雷达等设备，减少误差源。仿真计算证实了这一设计思想的可行性和     

航天器热控系统中的热泵-蓄冷组合方案

提出了旨在降低热控系统质量的热泵-蓄冷组合热控方案。通过对负荷进行预测，对热泵蓄冷系统的集成模式，系统的运行策略，以及蓄冷设备的容量等问题进行了分析。结果表明：通过合理优化系统的运行参数，热泵蓄冷组合方案能实现热控系统的轻量化设计要求，在未来航天热管理系统中具有相当的应用潜力。     

卫星液体晃动气浮台仿真试验系统的运动分析

本文通过边界元数值法求解了部分充液自旋球腔内的液体晃动问题。以流体运动的基本方程和系统运动的Ｅｕｌｅｒ动力学方程为基础，考虑了贮箱偏置、涡旋、重力及Ｃｏｒｉｏｌｉｓ力等因素对流体晃动和系统运动状态的影响，求解出液体的速度场，并在此基础上估算液体的能量耗散率和系统的章动时间常数     

从图像信息容量和图像功率谱看 CBERS-1卫星图像

文章从信息容量和图像功率谱这两个方面评价了CBERS-1的图像质量。并通过将同一地区的CBERS-1图像和TM图像进行比较,客现反映了CBERS-1卫星的图像质量。实验结果表明CBERS-1图像在信息丰富程度和图像综合的纹理特征上与TM图像质量相当,具有很好的可比性。     

二十一世纪的纳米技术

论述纳米技术将引发21世纪的一次产业革命.     

对GPS区域映射系统中比例优化的研究

GPS区域映射系统通过对分布式转发器的时延控制，实现定位区域上的映射关系，使由GPS制导的武器错误定位，从而偏离原有的目标，实现对重要目标的保护^[1]。文章首先给出了求解区域映射系统中虚拟点邻域的迭代算法，在此基础上分析了虚拟点与真实点的位置关系以及转发器的分布对映射比例的影响，并在有效干扰区域内，对如何选择虚拟点的位置和转发器的分布以达到映射比例的优化进行了研究，得出的结论为实际应用提供了参考。     

Simulation study on slant-to-vertical deviation in two dimensional TEC mapping over the ionosphere equatorial anomaly

With the rapid increase of GPS/GNSS receivers being deployed and operated in China, real-time GPS data from nearly a thousand sites are available at the National Center for Space Weather, China Meteorology Administration. However, it is challenging to generate a high-quality regional total electron content (TEC) map with the traditional two-dimensional (2-D) retrieval scheme because a large horizontal gradient has been reported over east–south Asia due to the northern equatorial ionization anomaly. We developed an Ionosphere Data Assimilation Analysis System (IDAAS), which is described in this study, using an International Reference Ionosphere (IRI) model as the background and applying a Kalman filter for updated observations. The IDAAS can reconstruct a three-dimensional ionosphere with the GPS slant TEC. The inverse slant TEC correlates well with observations both for GPS sites involved in the reconstruction and sites that are not involved. Based on the IDAAS, simulations were performed to investigate the deviation relative to the slant-to-vertical conversion (STV). The results indicate that the relative deviation induced by slant-to-vertical conversion may be significant in certain instances, and the deviation varies from 0% to 40% when the elevation decreases from 90° to 15°, while the relative IDAAS deviation is much smaller and varies from −5% to 15% without an elevation dependence. Compared with ‘true TEC’ map derived from the model, there is large difference in STV TEC map but no obvious discrepancy in IDAAS map. Generally, the IDAAS TEC map is much closer to the “true TEC” than is STV TEC map is.     

Solar-photon sail hovering orbits about single and binary asteroids

Solar-photon sails can be useful for missions towards and about asteroids. Indeed, for the interplanetary transfer phase, missions to asteroids often require a large variation in inclination and solar-photon sails perform very well for such high energy missions. In the same way, solar-photon sails are also expected to perform well in the phase about the asteroid. This paper studies single and binary asteroids’ hovering regions by using a sailcraft. In order to consider a sailcraft with its own mass and shape, the mutual polyhedral method (usually used to study asteroid dynamics) is used; therefore, the sailcraft is designed by means of tetrahedra. The procedure to obtain the hovering regions about a single asteroid is presented and an accurate analysis of the control variables is carried out. Moreover, control torques required to maintain hovering orbits are obtained by considering the gravitational torques acting on the sailcraft due to the asteroid. In the end, the theory for hovering orbits is extended to binary-asteroid systems and applied to the binary system 1999 KW4.