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Research of autonomous orbit determination of navigation constellation using satellite –to-satellite tracking data

机译:卫星到卫星跟踪数据确定导航星座自主轨道的研究

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Autonomous navigation of the Global Navigation Satellite System (GNSS) is a new technology. As we know,satellites of GNSS may lose track of the ground tracking system in some special conditions. Satellite constellation ofthe GNSS should complete orbit determination and time synchronization without ground-based tracking data in thisspecial condition. Several problems of autonomous orbit determination using only Satellite-to-Satellite Tracking(SST) data will be discussed in this paper. The bias of the state parameters (position-velocity vectors of satellites)can be controlled by orbit determination using only SST when errors of initial orbit and force model are not too large.The result of the orbit determination will not be good if the errors of the priori information are too large. However,SST cannot restrict the net rotation of the whole constellation in orbit determination, hence the errors caused by netrotation will be enlarged when the grand-tracking data is absent. The most important force model error inautonomous orbit determination is the solar radiation pressure (SRP) error. The result of the orbit determination willalso not be good if the error of the SRP is too large. Both analytical and numerical methods will be presented in thispaper to solve the problems in autonomous orbit determination.
机译:全球导航卫星系统(GNSS)的自主导航是一项新技术。据我们所知, 在某些特殊情况下,GNSS卫星可能会失去对地面跟踪系统的跟踪。的卫星星座 GNSS应该在没有地面跟踪数据的情况下完成轨道确定和时间同步 特殊情况。仅使用卫星到卫星跟踪来确定自主轨道的几个问题 (SST)数据将在本文中进行讨论。状态参数的偏差(卫星的位置速度矢量) 当初始轨道和力模型的误差不太大时,可以通过仅使用SST进行轨道确定来控制。 如果先验信息的误差太大,则轨道确定的结果将不好。然而, SST不能在确定轨道时限制整个星座的净旋转,因此,由净误差引起的误差 缺少大跟踪数据时,旋转将被放大。最重要的力模型误差 自主轨道确定是太阳辐射压力(SRP)误差。确定轨道的结果将 如果SRP的误差太大,也不太好。分析和数值方法都将在本节中介绍 解决自主轨道确定中的问题。

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