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嫦娥一号卫星双轴天线轨迹规划 总被引:1,自引:0,他引:1
针对嫦娥一号卫星双轴天线指向地球的控制要求,给出双轴天线框架角的计算方法.根据地球可见条件及双轴天线转动角度和角速度的限制。确定星上双轴天线自主跟踪地球的范围.最后,在轨飞行试验结果验证了该方法的有效性. 相似文献
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高校图书流通的5M1E管理法 总被引:1,自引:1,他引:0
兰林蓉 《桂林航天工业高等专科学校学报》2009,14(1)
借鉴质量管理中的"人机料法环测"(5M1E)因果分析管理方法,提出了高校图书流通管理的5M1E分析管理方法.在分析高校图书流通过程中诸要素的作用及其相互关系的基础上,阐述了"以读者为核心,以网络为平台,以图书为对象,依规程做约束.依测量做评价,依环境做创新"的高校图书流通管理指导思想及分析管理方法. 相似文献
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介绍了512×512高速帧转移面阵CCD器件时序设计的方法。在分析器件结构和时序关系的’基础上,确定了时序设计的主要参数,并利用复杂可编程逻辑器件(CPLD)EPM7256AETC100—5实现了CCD器件工作所需的各种时序信号。通过时序仿真证明,设计方法正确可行,运行稳定。 相似文献
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Yongchun Zheng Shijie Wang Ziyuan Ouyang Yongliao Zou Jianzhong Liu Chunlai Li Xiongyao Li Junming Feng 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Lunar soil simulant is a geochemical reproduction of lunar regolith, and is needed for lunar science and engineering researches. This paper describes a new lunar soil simulant, CAS-1, prepared by the Chinese Academy of Sciences, to support lunar orbiter, soft-landing mission and sample return missions of China’s Lunar Exploration Program, which is scheduled for 2004–2020. Such simulants should match the samples returned from the Moon, all collected from the lunar regolith rather than outcrops. The average mineral and chemical composition of lunar soil sample returned from the Apollo 14 mission, which landed on the Fra Mauro Formation, is chosen as the model for the CAS-1 simulant. Source material for this simulant was a low-Ti basaltic scoria dated at 1600 years from the late Quaternary volcanic area in the Changbai Mountains of northeast China. The main minerals of this rock are pyroxene, olivine, and minor plagioclase, and about 20–40% modal glass. The scoria was analyzed by XRF and found to be chemically similar to Apollo 14 lunar sample 14163. It was crushed in an impact mill with a resulting median particle size 85.9 μm, similar to Apollo soils. Bulk density, shear resistance, complex permittivity, and reflectance spectra were also similar to Apollo 14 soil. We conclude that CAS-1 is an ideal lunar soil simulant for science and engineering research of future lunar exploration program. 相似文献
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Zhen Li Marek Ziebart Santosh Bhattarai David Harrison Stuart Grey 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(9):2352-2365
Physics based SRP (Solar Radiation Pressure) models using ray tracing methods are powerful tools when modelling the forces on complex real world space vehicles. Currently high resolution (1?mm) ray tracing with secondary intersections is done on high performance computers at UCL (University College London). This study introduces the BVH (Bounding Volume Hierarchy) into the ray tracing approach for physics based SRP modelling and makes it possible to run high resolution analysis on personal computers. The ray tracer is both general and efficient enough to cope with the complex shape of satellites and multiple reflections (three or more, with no upper limit). In this study, the traditional ray tracing technique is introduced in the first place and then the BVH is integrated into the ray tracing. Four aspects of the ray tracer were tested for investigating the performance including runtime, accuracy, the effects of multiple reflections and the effects of pixel array resolution.Test results in runtime on GPS IIR and Galileo IOV (In Orbit Validation) satellites show that the BVH can make the force model computation 30–50 times faster. The ray tracer has an absolute accuracy of several nanonewtons by comparing the test results for spheres and planes with the analytical computations. The multiple reflection effects are investigated both in the intersection number and acceleration on GPS IIR, Galileo IOV and Sentinel-1 spacecraft. Considering the number of intersections, the 3rd reflection can capture , and of the total reflections for GPS IIR, Galileo IOV satellite bus and the Sentinel-1 spacecraft respectively. In terms of the multiple reflection effects on the acceleration, the secondary reflection effect for Galileo IOV satellite and Sentinel-1 can reach 0.2? and 0.4? respectively. The error percentage in the accelerations magnitude results show that the 3rd reflection should be considered in order to make it less than . The pixel array resolution tests show that the dimensions of the components have to be considered when choosing the spacing of the pixel in order not to miss some components of the satellite in ray tracing. This paper presents the first systematic and quantitative study of the secondary and higher order intersection effects. It shows conclusively the effect is non-negligible for certain classes of misson. 相似文献