A long baseline tracking network for improved NavIC orbit determination

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
B. N. Ramakrishna, P. D. Mishra, T. Subramanya Ganesh, Sharda Vashisth, Amitava Sen Gupta
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Abstract

Currently, the orbit determination accuracy of Navigation with Indian Constellation (NavIC) satellites is better than 20 m using the measurements from one-way ranging network of stations. The NavIC ephemerides along with time are continuously transmitted from the NavIC satellites. The transmitted ephemerides are also known as the broadcast ephemerides. These ephemerides are functions of precise orbit determination and dynamical model used for the orbit propagation and are one of the major error sources in the NavIC receiver position. In this paper, a study has been carried out to improve the orbit determination. This is performed through the precise orbit determination using extended tracking network with a sufficiently long baseline tracking stations (LBTS). We first attempted to fix a suitable number of LBTS based on several criteria, such as geometry, elevation cut-off angle, minimum tracking duration, etc. LBTS are optimally selected to reduce the along-track, in-track and cross-track errors in the estimated orbit. We also address the precise orbit determination of NavIC satellites by employing a weighed least square differential correction method. In the orbit determination process, the numerical integration orbit propagator using Cowell’s method, a step-by-step algorithm, is utilized. The simulated one-way range measurements are used for the precise orbit determination with a white noise sigma of 10 cm. We found that the observed position accuracy improvements are better than 10 m.

Abstract Image

改进NavIC轨道确定的长基线跟踪网络
目前,印度星座卫星导航利用单向测距站网测量的定轨精度优于20米。导航星历表随时间从导航卫星连续传送。传输的星历表也被称为广播星历表。这些星历表是精确定轨和轨道传播所用动力学模型的函数,是导航系统接收机位置误差的主要来源之一。本文对提高卫星定轨精度进行了研究。这是通过使用具有足够长的基线跟踪站(LBTS)的扩展跟踪网络精确确定轨道来实现的。我们首先尝试根据几个标准来确定合适的LBTS数量,例如几何形状、高程截止角度、最小跟踪持续时间等。对LBTS进行了优化选择,以减小估计轨道上的沿轨、轨内和跨轨误差。本文还采用加权最小二乘差分修正方法解决了导航卫星的精确定轨问题。在定轨过程中,采用分步算法Cowell法的数值积分轨道传播算子。模拟的单向距离测量用于精确的轨道确定,白噪声sigma为10 cm。我们发现观测到的位置精度提高了10 m以上。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Journal of Astrophysics and Astronomy
Journal of Astrophysics and Astronomy 地学天文-天文与天体物理
CiteScore
1.80
自引率
9.10%
发文量
84
审稿时长
>12 weeks
期刊介绍: The journal publishes original research papers on all aspects of astrophysics and astronomy, including instrumentation, laboratory astrophysics, and cosmology. Critical reviews of topical fields are also published. Articles submitted as letters will be considered.
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