基于双轴调整棱镜的惯导缓冲基座方位引出

分析并设计了一种将带双轴调整机构的棱镜作为基准棱镜的方位引出方法,并基于此提出了惯导缓冲基座复位精度试验方案.首先,根据直角棱镜作基准棱镜时放置位置对方位引出的影响,设计可双轴调整机构;然后,从双轴调整机构出发,利用坐标变换和矢量形式的棱镜反射公式推导了放置误差造成的方位引出误差,根据误差公式设计了试验方案;最后,分析与估算了方位引出精度,结果表明:此方案在控制经纬仪望远镜的俯仰角小于15°时,方位引出的均方误差小于5″.     

一种新的闭路制导导引方法

闭路制导方法是一种实用的方法误差比较小的制导方法。其中,如何将实际速度导引到需要速度至关重要,通常的闭路制导导引方法在关机点附近不稳定,会产生一定的方法误差。为了避免这种导引不稳定的影响,本文给出了一种采用目标瞬时方位角为基准的新型闭路制导导引方法。通过仿真计算,证明该方法关机点附近导引稳定,导引引起的方法误差较小。     

三点法测量线轮廓度和面轮廓度的数学模型

本文通过分析和研究三点法误差分离技术,建立了测量和评定工件线轮廓度、面轮廓度的数学模型。     

P向量实现快速星图识别的方法

 提出了一种快速的星图识别方法。该方法识别时提取出描述观测三角形的一维特征量P，根据该值快速检索到对应的导航三角形，减少了计算过程。由于获得星点位置的时候存在误差，所以将一定误差范围内的三角形均作为待选三角形考虑。上述识别后引入了验证识别环节，保证识别的准确性。随机实验统计表明，同等星点位置噪声方差下，该方法和栅格算法相比识别率提高约1%，识别时间约为后者的1/5。     

改善高校贫困生成长环境研究

党的十六大提出了在未来二十年要全面建设小康社会的宏伟目标，如何实现这一目标，工作是多方面的，而高校贫困生正是人们应该关注的重点对象。本文主要从高校贫困生的消费现状、贫困生心理、国家资助体系等存在的突出问题人手调查分析贫困生目前现状，并且在前人研究成果的基础上，从国家宏观经济政策和贫困生自身方面提出相应的解决措施。     

Feature selection for high-dimensional data in astronomy

With an exponentially increasing amount of astronomical data, the complexity and dimension of astronomical data are likewise growing rapidly. Extracting information from such data becomes a critical and challenging problem. For example, some algorithms can only be employed in the low-dimensional spaces, so feature selection and feature extraction become important topics. Here we describe the difference between feature selection and feature extraction methods, and introduce the taxonomy of feature selection methods as well as the characteristics of each method. We present a case study comparing the performance and computational cost of different feature selection methods. For the filter method, ReliefF and fisher filter are adopted; for the wrapper method, improved CHAID, linear discriminant analysis (LDA), Naive Bayes (NB) and C4.5 are taken as learners. Applied on the sample, the result indicates that from the viewpoints of computational cost the filter method is superior to the wrapper method. Moreover, different learning algorithms combined with appropriate feature selection methods may arrive at better performance.     

A geomagnetic activity forecast for improving the efficiency of aeromagnetic surveys in Greenland

In recent years several aeromagnetic surveys were carried out in Greenland and more will be carried out in the future. We describe some of the characteristics pertinent to surveys in Greenland and the problems faced and experiences made by the survey teams working there, with special emphasis on the west coast where most surveys were conducted. Both unfavorable terrestrial weather and space weather appear to complicate survey planning. We discuss possible options available to the survey teams for mitigating the adverse effect of part of the problems, namely survey data contamination by intense geomagnetic activity. The implementation of a prototype geomagnetic activity forecast service as an aid to planning survey flights is discussed in more detail. The forecast service was tested by an independent observer, and the performance of the scheme is evaluated by a subsequent comparison between forecast and actual measurements. The comparison rendered largely acceptable results, but their validity is limited by the fact that the two-month test interval was characterized by a mostly relatively quiet magnetic field.     

天文探测卫星定点观测模式外热流变化规律分析

针对天文探测卫星定点观测模式下的特定姿态,结合相关科学观测约束、整星能源和热控设计约束及轨道特点,进行了多约束条件下的外热流变化规律分析,对比了有、无遮阳挡板情况下,卫星外热流的差异,并通过虚拟热沉温度,分析了卫星各个舱板的散热能力。基于有、无遮阳挡板的外热流分析结果,从热控角度建议在定点观测模式下,对卫星的观测姿态进行约束,对有低温需求的天文探测器建议加设遮阳挡板,可为天文探测卫星的热控设计提供参考。     

快速迭代反卷积算法的超分辨性能分析

传统观念认为,扫描体制下的实孔径雷达方位分辨力决定于3dB波束宽度,这使得雷达难以从方位上区分同一波束内的两个等距目标。迭代反卷积算法是一种简单实用的超分辨算法,为分析迭代反卷积算法的超分辨性能,文章对线性迭代算法和P阶决速迭代算法进行了比较并对此做了仿真实验。仿真实验表明,P阶快速迭代反卷积算法的超分辨效果较佳,而且...     

大型星载固面天线热变形试验及仿真分析验证

星载天线在轨运行期间所经历的复杂温度环境,会使天线产生严重的热变形,从而对其电性能造成重要影响。文章根据大型星载固面天线热变形的特点,提出热变形试验与仿真一体化分析验证方法,并且将测试结果与数值仿真结果进行相互校验。该方法可为大型星载天线结构设计及验证提供参考。