Estimation and evaluation of hourly Meteorological Operational (MetOp) satellites' GPS receiver differential code biases (DCBs) with two different methods

IF 1.7 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
Linlin Li, Shuanggen Jin
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引用次数: 0

Abstract

Abstract. Differential code bias (DCB) is one of the Global Positioning System (GPS) errors, which typically affects the calculation of total electron content (TEC) and ionospheric modeling. In the past, DCB was normally estimated as a constant in 1 d, while DCB of a low Earth orbit (LEO) satellite GPS receiver may have large variations within 1 d due to complex space environments and highly dynamic orbit conditions. In this study, daily and hourly DCBs of Meteorological Operational (MetOp) satellites' GPS receivers are calculated and evaluated using the spherical harmonic function (SHF) and the local spherical symmetry (LSS) assumption. The results demonstrated that both approaches could obtain accurate and consistent DCB values. The estimated daily DCB standard deviation (SD) is within 0.1 ns in accordance with the LSS assumption, and it is numerically less than the standard deviation of the reference value provided by the Constellation Observing System for Meteorology Ionosphere and Climate (COSMIC) Data Analysis and Archive Center (CDAAC). The average error's absolute value is within 0.2 ns with respect to the provided DCB reference value. As for the SHF method, the DCB's standard deviation is within 0.1 ns, which is also less than the standard deviation of the CDAAC reference value. The average error of the absolute value is within 0.2 ns. The estimated hourly DCB with LSS assumptions suggested that calculated results of MetOpA, MetOpB, and MetOpC are, respectively, 0.5 to 3.1 ns, −1.1 to 1.5 ns, and −1.3 to 0.7 ns. The root mean square error (RMSE) is less than 1.2 ns, and the SD is under 0.6 ns. According to the SHF method, the results of MetOpA, MetOpB, and MetOpC are 1 to 2.7 ns, −1 to 1 ns, and −1.3 to 0.6 ns, respectively. The RMSE is under 1.3 ns and the SD is less than 0.5 ns. The SD for solar active days is less than 0.43, 0.49, and 0.44 ns, respectively, with the LSS assumption, and the appropriate fluctuation ranges are 2.0, 2.2, and 2.2 ns. The variation ranges for the SHF method are 1.5, 1.2, and 1.2 ns, respectively, while the SD is under 0.28, 0.35, and 0.29 ns.
基于两种不同方法的逐时气象业务卫星GPS接收机差分码偏差(DCBs)估算与评价
摘要差分码偏(DCB)是全球定位系统(GPS)误差之一,它通常会影响总电子含量(TEC)的计算和电离层模拟。过去,DCB通常在1 d内是一个常数,而低地球轨道卫星GPS接收机的DCB由于复杂的空间环境和高度动态的轨道条件,在1 d内可能会有较大的变化。本文利用球谐函数(SHF)和局地球对称(LSS)假设,对气象业务卫星(MetOp) GPS接收机的日、时dcb进行了计算和评价。结果表明,两种方法均能获得准确一致的DCB值。根据LSS假设估算的日DCB标准差(SD)在0.1 ns以内,在数值上小于星座气象电离层与气候观测系统(COSMIC)数据分析与档案中心(CDAAC)提供的参考值的标准差。相对于提供的DCB参考值,平均误差绝对值在0.2 ns以内。对于SHF方法,DCB的标准差在0.1 ns以内,也小于CDAAC参考值的标准差。绝对值的平均误差在0.2 ns以内。基于LSS假设的每小时DCB估算结果表明,MetOpA、MetOpB和MetOpC的计算结果分别为0.5 ~ 3.1 ns、- 1.1 ~ 1.5 ns和- 1.3 ~ 0.7 ns。均方根误差(RMSE)小于1.2 ns, SD小于0.6 ns。根据SHF法,MetOpA、MetOpB和MetOpC的测定结果分别为1 ~ 2.7 ns、−1 ~ 1ns和−1.3 ~ 0.6 ns。均方根误差小于1.3 ns,标准差小于0.5 ns。在LSS假设下,太阳活动日数的SD分别小于0.43、0.49和0.44 ns,适宜的波动范围分别为2.0、2.2和2.2 ns。SHF方法的变化范围分别为1.5、1.2和1.2 ns,而SD在0.28、0.35和0.29 ns以下。
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
Annales Geophysicae
Annales Geophysicae 地学-地球科学综合
CiteScore
4.30
自引率
0.00%
发文量
42
审稿时长
2 months
期刊介绍: Annales Geophysicae (ANGEO) is a not-for-profit international multi- and inter-disciplinary scientific open-access journal in the field of solar–terrestrial and planetary sciences. ANGEO publishes original articles and short communications (letters) on research of the Sun–Earth system, including the science of space weather, solar–terrestrial plasma physics, the Earth''s ionosphere and atmosphere, the magnetosphere, and the study of planets and planetary systems, the interaction between the different spheres of a planet, and the interaction across the planetary system. Topics range from space weathering, planetary magnetic field, and planetary interior and surface dynamics to the formation and evolution of planetary systems.
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