Doresa和Milena Galileo卫星广播星历的精度评价

U. Robustelli, G. Benassai, G. Pugliano
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引用次数: 9

摘要

2014年8月22日,多雷萨和米莱娜伽利略卫星在错误的轨道上发射。2014年11月,欧洲航天局启动了一项回收任务,使两颗卫星可用。2016年8月5日,这两颗卫星开始在导航电文中广播星历表,用于测试目的。这些星历表中的任何错误都将直接影响伽利略定位的准确性。本文将利用广播星历计算的所有伽利略卫星位置与IGS提供的精确位置进行了比较,重点是Doresa和Milena卫星。在20天的数据中,每秒钟进行一次比较。对这些误差进行了统计分析。在2018年2月21日(DOY 52)至3月12日(DOY 71)期间,利用IGS产品确定广播轨道与IGS精确轨道之间每秒的位置误差。分析表明,多雷萨卫星和米莱娜卫星广播轨道的日三维均方根误差约为2米,与伽利略卫星的日三维均方根误差相当。只有在DOY 62上,他们显示的RMS 3d误差约为40米。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Accuracy evaluation of Doresa and Milena Galileo satellites broadcast ephemerides
On 22 August 2014 Doresa and Milena Galileo satellites were launched in wrong orbit. In November 2014 European space agency started a salvaged mission to make two satellites usable. On 5 August 2016 these two satellites started broadcasting ephemerides in navigation message for testing purposes. Any errors in these ephemerides will directly impact the accuracy of Galileo positioning. This paper compares all the Galileo satellites position computed using broadcast ephemerides with the precise position provided by the IGS with a focus on Doresa and Milena satellites. The comparison was undertaken every second during 20 days of data. The statistics of these errors were also analyzed. The position error between the broadcast orbit and the IGS precise orbit was determined for each second for the period starting on February 21, 2018 (DOY 52) to March 12 (DOY 71) by using IGS products. The analysis shows that the broadcast orbit of Doresa and Milena satellite has a daily 3d RMS error of about 2 meters that is a comparable value with that of the other Galileo satellites. Only on DOY 62 they show an RMS 3d error of about 40 meters.
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