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Autonomous orbit determination using observations of a sodium guide-star network

机译:利用钠导星网络的观测确定自主轨道

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摘要

A new method of spacecraft orbit determination is developed based on position information from the observation of fluorescing streaks in the atomic sodium of Earth's upper atmosphere. This concept could be used for GPS constellation autonomous navigation (AutoNav). This new orbit determination method uses a spacecraft-mounted camera to observe fluorescing line segments in the sodium layer. The fluorescence is excited by ground-based sodium guide-star lasers. The system also uses a star tracker in order to reference the measured guide-star directions to inertial coordinates. The measured direction to an unknown point on a known guide-star segment at a known time defines a plane on which the spacecraft must lie. Seven or more independent measurements suffice to determine a Keplerian orbit and the spacecraft clock offset. Cramer-Rao analysis indicates that 1 - sigma position accuracies on the order of 20 m or better may be achievable for filtering intervals of several days.
机译:根据位置信息,开发了一种新的航天器轨道确定方法,该信息来自对地球高层大气原子钠中荧光条纹的观察。此概念可用于GPS星座自主导航(AutoNav)。这种新的轨道确定方法是使用安装在航天器上的照相机观察钠层中的发荧光线段。地基钠导向星激光激发荧光。该系统还使用星形跟踪器,以便将测得的引导星形方向参考到惯性坐标。在已知时间到已知引导星段上未知点的测量方向定义了航天器必须所在的平面。七个或更多独立测量值足以确定开普勒轨道和航天器的时钟偏移量。 Cramer-Rao分析表明,对于几天的过滤间隔,可以达到20 m或更佳的1 sigma位置精度。

著录项

  • 来源
    《Navigation》 |2019年第2期|385-400|共16页
  • 作者单位

    Virginia Tech Dept Aerosp & Ocean Engn Blacksburg VA 24061 USA;

    ExoAnalyt Solut Space Situat Awareness Grp Mission Viejo CA USA;

    US Air Force Syst Engn Directorate Chantilly VA USA;

  • 收录信息 美国《工程索引》(EI);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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