Estimation of the Accuracy of Geostationary Satellite Observations

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
M. O. Kulichenko, N. V. Maigurova, O. V. Shulga, V. F. Kryuchkovskiy
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Abstract

Continuous monitoring of artificial space objects requires periodic quality control of observational data. Estimating the internal accuracy of observations in the form of an RMS error of positions makes it possible to monitor and detect outliers in primary data array. For artificial satellites of the Earth, the orbital elements calculated at the Research Institute Nikolaev Astronomical Observatory (RI NAO) can be externally compared with the data of the International Laser Ranging Service (ILRS) or the Global Navigation Satellite System (GNSS). Such a comparison makes it possible to detect time synchronization problems and to identify and evaluate systematic errors. At the RI NAO, regular observations of artificial satellites in different orbits using several telescopes have been carried out for more than 10 years, and a catalog of orbital elements in the two-line element (TLE) format is maintained. The software for calculating orbital elements has been developed in cooperation with the Astronomical Observatory of the Odessa National University. This article presents the analysis of the processing results of an array of observations from 149 geostationary satellites (GSS’s). The observations have been made during 2020…2021 using the RI NAO telescope complex. Time synchronization has been provided by the Resolution-T GPS receiver with an RMS error of 40 ns. All GSS observations have been carried out using the combined observation method developed at the RI NAO. A total of 134 461 GSS positions have been obtained for which the residual O–C differences with respect to the orbit calculated at the RI NAO have been determined. The RMS error of the GSS positions in the apparent magnitude range 9m…13m is 0.5″ in right ascension and declination. A comparison of the GSS orbital positions calculated from the RI NAO orbital elements and the ILRS website data shows that the differences between the corresponding geocentric Cartesian coordinates at the start of the prediction are dX = 0.72 km, dY = –0.52 km, and dZ = 1.28 km.

Abstract Image

地球静止卫星观测精度的估计
对人造空间物体的持续监测需要定期对观测数据进行质量控制。以位置均方根误差的形式估计观测值的内部精度,可以监测和检测主数据阵列中的异常值。对于地球人造卫星,尼古拉耶夫天文台(RI NAO)计算的轨道要素可以对外与国际激光测距服务(ILRS)或全球导航卫星系统(GNSS)的数据进行比较。这样的比较使检测时间同步问题和识别和评估系统错误成为可能。在国际气象观测中心,使用几架望远镜对不同轨道上的人造卫星进行了10多年的定期观测,并保存了一份双线元格式的轨道要素目录。计算轨道元素的软件是与敖德萨国立大学天文台合作开发的。本文分析了149颗地球同步卫星(GSS)的一系列观测数据的处理结果。这些观测是在2020年至2021年期间使用RI NAO望远镜进行的。分辨率- t GPS接收机提供的时间同步,均方根误差为40 ns。所有的GSS观测都是使用RI NAO开发的联合观测方法进行的。总共获得了134 461个GSS位置,并确定了相对于在RI NAO计算的轨道的剩余O-C差。在视星等9m ~ 13m范围内,赤经和赤纬下GSS位置的均方根误差为0.5″。对比RI NAO轨道元与ILRS网站数据计算的GSS轨道位置,预测开始时对应的地心坐标差值分别为dX = 0.72 km, dY = -0.52 km, dZ = 1.28 km。
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来源期刊
Kinematics and Physics of Celestial Bodies
Kinematics and Physics of Celestial Bodies ASTRONOMY & ASTROPHYSICS-
CiteScore
0.90
自引率
40.00%
发文量
24
审稿时长
>12 weeks
期刊介绍: Kinematics and Physics of Celestial Bodies is an international peer reviewed journal that publishes original regular and review papers on positional and theoretical astronomy, Earth’s rotation and geodynamics, dynamics and physics of bodies of the Solar System, solar physics, physics of stars and interstellar medium, structure and dynamics of the Galaxy, extragalactic astronomy, atmospheric optics and astronomical climate, instruments and devices, and mathematical processing of astronomical information. The journal welcomes manuscripts from all countries in the English or Russian language.
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