基于改进LF算法的雷达信号分选

在现代战争中随着新体制雷达的不断涌现,电磁环境变得越来越复杂,雷达脉冲相互交错,雷达信号的处理面临高密度信号环境。目前普遍采用的基于直方图统计的信号分选方法越来越不适应现代雷达信号环境。将蚁群聚类算法引入到雷达信号分选中,并对其进行了改进,提出了一种新的雷达信号分选方法。该方法不需要雷达信号的先验知识,适用于处理未知信...     

地月系低能转移轨道设计

分析了不同转移轨道间的性能指标,以黄道面与白道面交线作为庞加莱截面实现不同系统轨道的拼接,利用其中耗能最小的日地系稳定流形和地月系的不稳定流形设计了一条低能耗转移轨道.最后对不同轨 道进行了能量分析和对比,优化了国内提出的低能探月轨道.仿真结果表明,文中方法比直接通过霍曼转移节约21.1%的能量,对探月工程的轨道设计具...     

Exploring links between crater floor mineralogy and layered lunar crust

Floors of similar sized craters, representing material from similar depth horizons, have been studied to explore their suitability as mineralogy indicators at various depths within the lunar crust. Clementine UV–vis multispectral data was used to generate mineral abundance maps of crater floors and surroundings using a modified version of algorithm given by Pieters et al. (2001) [Pieters, C.M., Head, J.W., Gaddis, L., Jolliff, B. and Duke, M. Rock types of the south pole aitken basin and extent of basaltic volcanism, JGR (106) E11, 28001–28022, 2001.]. Substantial processing of the crater floor material due to variety of geological processes is evident in the generated maps, making straight forward interpretations difficult. However, systematic compositional trends in fresh craters on the floors of target craters seem to indicate the feasibility of such an effort.     

Does the lunar surface still offer value as a site for astronomical observatories?

Current thinking about the Moon as a destination has revitalized interest in lunar astronomical observatories. Once seen by a large scientific community as a highly enabling site, the dramatic improvement in capabilities for free-space observatories prompts reevaluation of this interest. Whereas the lunar surface offers huge performance advantages for astronomy over terrestrial sites, free-space locales such as Earth orbit or Lagrange points offer performance that is superior to what could be achieved on the Moon. While astronomy from the Moon may be cost-effective once infrastructure is there, it is in many respects no longer clearly enabling compared with free space.     

Scientific objectives and specification of the SELENE Multiband Imager

The Lunar Imager/SpectroMeter (LISM) is an instrument being developed for onboarding the SELENE satellite that will be launched in 2007. The LISM consists of the three subsystems: Terrain Camera (TC), Multiband Imager (MI), and Spectral Profiler (SP).     

Journey to the Moon: Recent results,science, future robotic and human exploration

The upcoming fleet of lunar missions, and the announcement of new lunar exploration initiatives, show an exciting “Journey to the Moon”, covering recent results, science, future robotic and human exploration. We review some of the questions, findings and perspectives given in the papers included in this issue of Advances in Space Research.     

基于改进人工蜂群算法的无人机实时航迹规划

为了适应现代战争战场环境的复杂性,针对所建立的突发威胁模型,提出了一种基于改进人工蜂群算法的无人机航迹规划方法,对无人机进行动态航迹寻优,并通过MATLAB进行了仿真验证。仿真结果表明,所设计的方法能够根据实时出现的威胁状况进行动态航迹规划、评价和选优,同时满足实时性要求。     

基于改进蚁群算法的改航路径规划研究

当航班遇到恶劣天气或者飞行冲突时,可以采取航班改航策略为需要改航的航班规划出合适的飞行路径。采用栅格法对环境进行建模并且对传统蚁群算法进行改进。首先,在转移概率的计算上加入危险天气的影响等级;其次,在节点选择上采用贝叶斯思想,通过后验概率对候选节点进行评估;最后,通过在短时间内信息素的增量上的差别来增大较优路径和其他路径之间的信息素量的差距,引导算法收敛到最优路径,同时加快算法的收敛速度。经算例分析证明了方法的有效性和可行性。     

Regolith effects in planetary X-ray fluorescence spectroscopy: Laboratory studies at 1.7–6.4 keV

Laboratory measurements are presented to study the effects of the physical properties of regolith on planetary soft X-ray fluorescence spectroscopy. Two laboratory setups are used to independently measure these regolith effects using lunar regolith analog samples with three different particle-size ranges. Discussion is given on the data analysis. Some of the data may be valid only for qualitative conclusions. Analytical modelling is used to separate the effects expected for a plane-parallel and homogeneous medium from those of measured regolith analogs. The surface roughness and porosity of the regolith are observed to induce an enhancement of the higher-energy part of the spectrum as a function of the incidence angle. The enhancement is larger for rougher surfaces. A brief discussion is given on the relevance of this study for future planetary missions carrying soft X-ray spectrometers.