第二次地球方向参数预测比较活动(2nd EOP PCC):综述

IF 0.7 Q4 ASTRONOMY & ASTROPHYSICS Artificial Satellites-Journal of Planetary Geodesy Pub Date : 2022-12-01 DOI:10.2478/arsa-2022-0021
J. Śliwińska, Tomasz Kur, M. Wińska, J. Nastula, H. Dobslaw, Aleksander Partyka
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引用次数: 0

摘要

摘要在地球表面和太空中进行精确定位和导航需要精确的地球定向参数(EOP)数据和预测。在过去的几十年里,EOP预测已成为国际大地测量界越来越关注的主题,例如空间机构、卫星运营商、研究地球自转动力学的研究人员和导航系统用户。由于这一事实,世界各地的许多研究中心都开发了专门的EOP预测方法。目前正在第二次地球定向参数预测比较运动(第二次EOP PCC)的框架内对各种EOP预测能力进行评估,该运动于2021年9月开始,将持续到2022年底。这场新的运动是由波兰华沙的巴丹Kosmicznych Polskiej Akademii Nauk中心(CBK PAN)运营的EOP PCC办公室与GeoForschungsZentrum(GFZ)合作,在国际地球自转和参考系统服务(IERS)的赞助下准备的。在本文中,我们概述了第二次EOP PCC启动五个月后的情况。我们讨论了技术方面的问题,并提供了迄今为止收到的关于参与者和有效预测文件的统计数据。此外,我们还介绍了不同参考解决方案与官方IERS 14 C04 EOP系列的初步比较结果。极移、日长和进动章动分量的不同解的均方根值分别在0.04至0.36 mas、0.01至0.10 ms和0.01至0.18 mas的水平上显示差异。
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Second Earth Orientation Parameters Prediction Comparison Campaign (2nd EOP PCC): Overview
Abstract Precise positioning and navigation on the Earth’s surface and in space require accurate earth orientation parameters (EOP) data and predictions. In the last few decades, EOP prediction has become a subject of increased attention within the international geodetic community, e.g., space agencies, satellite operators, researchers studying Earth rotation dynamics, and users of navigation systems. Due to this fact, many research centres from around the world have developed dedicated methods for the forecasting of EOP. An assessment of the various EOP prediction capabilities is currently being pursued in the frame of the Second Earth Orientation Parameters Prediction Comparison Campaign (2nd EOP PCC), which began in September 2021 and will be continued until the end of the year 2022. The new campaign was prepared by the EOP PCC Office run by Centrum Badań Kosmicznych Polskiej Akademii Nauk (CBK PAN) in Warsaw, Poland, in cooperation with GeoForschungsZentrum (GFZ) and under the auspices of the International Earth Rotation and Reference Systems Service (IERS). In this paper, we provide an overview of the 2nd EOP PCC five months after its start. We discuss the technical aspects and present statistics about the participants and valid prediction files received so far. Additionally, we present the results of preliminary comparisons of different reference solutions with respect to the official IERS 14 C04 EOP series. Root mean square values for different solutions for polar motion, length of day, and precession-nutation components show discrepancies at the level from 0.04 to 0.36 mas, from 0.01 to 0.10 ms, and from 0.01 to 0.18 mas, respectively.
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