毛悦, 宋小勇, 冯来平. X射线脉冲星导航可见性分析[J]. 武汉大学学报 ( 信息科学版), 2009, 34(2): 222-225.
引用本文: 毛悦, 宋小勇, 冯来平. X射线脉冲星导航可见性分析[J]. 武汉大学学报 ( 信息科学版), 2009, 34(2): 222-225.
MAO Yue, SONG Xiaoyong, FENG Laiping. Visibility Analysis of X-ray Pulsar Navigation[J]. Geomatics and Information Science of Wuhan University, 2009, 34(2): 222-225.
Citation: MAO Yue, SONG Xiaoyong, FENG Laiping. Visibility Analysis of X-ray Pulsar Navigation[J]. Geomatics and Information Science of Wuhan University, 2009, 34(2): 222-225.

X射线脉冲星导航可见性分析

Visibility Analysis of X-ray Pulsar Navigation

  • 摘要: 概述了X射线脉冲星可见性分析需要考虑的影响因素,给出了脉冲星高度角以及第三天体遮挡的计算公式。根据导航需要,按照脉冲星优选准则,选取50颗X射线脉冲星进行了仿真计算。分析了可见脉冲星个数随位置、时间、高度的变化规律,单颗脉冲星在1 d时间内可见性的变化情况,以及日月对脉冲星的遮挡情况。

     

    Abstract: The influent factors,which should be considered in the analysis of X-ray pulsar visibility,were summarized.The calculation formulas of pulsar elevation angle and the shelter from the three-body were also presented.According to the requirement of navigation,fifty X-ray pulsars were selected based on the rules of pulsar selection.The change of visible pulsar number with position,time,height were analyzed through calculations.The change of visibility of a single pulsar in a single day and the shelter from sun and moon were studied.Finally,conclusion is drawn.

     

/

返回文章
返回