Phase residuals analysis in kinematic orbit determination of GRACE-FO
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作者:
Zhang, Rui
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Southwest Jiaotong Univ, Fac Geosci & Engn, Chengdu, Sichuan, Peoples R ChinaSouthwest Jiaotong Univ, Fac Geosci & Engn, Chengdu, Sichuan, Peoples R China
Zhang, Rui
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Xiong, Yongliang
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Southwest Jiaotong Univ, Fac Geosci & Engn, Chengdu, Sichuan, Peoples R ChinaSouthwest Jiaotong Univ, Fac Geosci & Engn, Chengdu, Sichuan, Peoples R China
Xiong, Yongliang
[1
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Xu, Shaoguang
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Southwest Jiaotong Univ, Fac Geosci & Engn, Chengdu, Sichuan, Peoples R ChinaSouthwest Jiaotong Univ, Fac Geosci & Engn, Chengdu, Sichuan, Peoples R China
Xu, Shaoguang
[1
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[1] Southwest Jiaotong Univ, Fac Geosci & Engn, Chengdu, Sichuan, Peoples R China
The GRACE-FO based scientific research will benefit from the improvement of the kinematic orbit quality. This study investigated the errors that could potentially impact the accuracy of orbit determination and applied error corrections to the observations, including phase center variation (PCV) and multipath error, with a specific focus on enhancing the performance of GRACE-FO kinematic precise orbit determination based on the zero-difference method. When the observation model for precise orbit determination is highly consistent with the actual situation, the phase residuals should only consist of observation noise. However, the phase residuals encompass both modeled errors and unmodeled errors, such as PCV and multipath errors. The study utilized the GPS observation data of the GRACE-FO satellites in January 2022 to derive the fixed ambiguity solutions based on the zero-difference ionosphere-free linear combination, thereby obtaining the phase residuals. Subsequently, the antenna PCV was estimated based on the residual method, resulting in a substantial reduction in carrier phase residuals through PCV correction. A comparison with the reference orbits revealed that the root mean square (RMS) of the fixed solutions with PCV correction improved by 2.8 to 4.3 mm in three directions. Furthermore, the wavelet decomposition was performed on the phase residuals to extract the multipath errors and reconstruct the carrier phase observations. The RMS of the kinematic orbits improved by 4.3 to 5.9 mm with the incorporation of both the PCV and multipath error corrections. The RMS of the satellite laser ranging (SLR) residuals of the two GRACE-FO (GRACE-C and GRACE-D) satellites were 1.43 cm and 1.48 cm, respectively. The results indicate that these methods have the potential to enhance the kinematic orbit accuracy of the GRACE-FO satellites, bringing it closer to the a posteriori scientific orbit accuracy. (c) 2024 COSPAR. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).
机构:
Shanghai Univ, Sch Commun & Informat Engn, Shanghai 200444, Peoples R China
Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R ChinaShanghai Univ, Sch Commun & Informat Engn, Shanghai 200444, Peoples R China
Luo, Peng
Jin, Shuanggen
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Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
Nanjing Univ Informat Sci & Technol, Sch Remote Sensing & Geomat Engn, Nanjing 210044, Peoples R China
Henan Polytech Univ, Sch Surveying & Land Informat Engn, Jiaozuo 454000, Henan, Peoples R ChinaShanghai Univ, Sch Commun & Informat Engn, Shanghai 200444, Peoples R China
Jin, Shuanggen
Shi, Qiqi
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Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R ChinaShanghai Univ, Sch Commun & Informat Engn, Shanghai 200444, Peoples R China
机构:
Southwest Jiaotong Univ, Fac Geosci & Engn, Chengdu 611756, Peoples R ChinaSouthwest Jiaotong Univ, Fac Geosci & Engn, Chengdu 611756, Peoples R China
Zhang, Jiahui
You, Wei
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Southwest Jiaotong Univ, Fac Geosci & Engn, Chengdu 611756, Peoples R ChinaSouthwest Jiaotong Univ, Fac Geosci & Engn, Chengdu 611756, Peoples R China
You, Wei
Yu, Biao
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Southwest Jiaotong Univ, Fac Geosci & Engn, Chengdu 611756, Peoples R ChinaSouthwest Jiaotong Univ, Fac Geosci & Engn, Chengdu 611756, Peoples R China
Yu, Biao
Fan, Dongming
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Southwest Jiaotong Univ, Fac Geosci & Engn, Chengdu 611756, Peoples R ChinaSouthwest Jiaotong Univ, Fac Geosci & Engn, Chengdu 611756, Peoples R China
机构:
Yunnan Power Grid Co Ltd, Elect Power Res Inst, Joint Lab Power Remote Sensing Technol, Kunming 650217, Peoples R ChinaYunnan Power Grid Co Ltd, Elect Power Res Inst, Joint Lab Power Remote Sensing Technol, Kunming 650217, Peoples R China
Ma, Yi
Yang, Zhouming
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Chinese Acad Sci, Innovat Acad Precis Measurement Sci & Technol, State Key Lab Geodesy & Earths Dynam, Wuhan 430071, Peoples R ChinaYunnan Power Grid Co Ltd, Elect Power Res Inst, Joint Lab Power Remote Sensing Technol, Kunming 650217, Peoples R China
Yang, Zhouming
Yuan, Yunbin
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Chinese Acad Sci, Innovat Acad Precis Measurement Sci & Technol, State Key Lab Geodesy & Earths Dynam, Wuhan 430071, Peoples R ChinaYunnan Power Grid Co Ltd, Elect Power Res Inst, Joint Lab Power Remote Sensing Technol, Kunming 650217, Peoples R China
Yuan, Yunbin
Sun, Qinglei
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Chinese Acad Sci, Innovat Acad Precis Measurement Sci & Technol, State Key Lab Geodesy & Earths Dynam, Wuhan 430071, Peoples R ChinaYunnan Power Grid Co Ltd, Elect Power Res Inst, Joint Lab Power Remote Sensing Technol, Kunming 650217, Peoples R China
Sun, Qinglei
Zhou, Fangrong
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Yunnan Power Grid Co Ltd, Elect Power Res Inst, Joint Lab Power Remote Sensing Technol, Kunming 650217, Peoples R ChinaYunnan Power Grid Co Ltd, Elect Power Res Inst, Joint Lab Power Remote Sensing Technol, Kunming 650217, Peoples R China
Zhou, Fangrong
Wen, Gang
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Yunnan Power Grid Co Ltd, Elect Power Res Inst, Joint Lab Power Remote Sensing Technol, Kunming 650217, Peoples R ChinaYunnan Power Grid Co Ltd, Elect Power Res Inst, Joint Lab Power Remote Sensing Technol, Kunming 650217, Peoples R China
机构:
Chinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R China
Univ Chinese Acad Sci, Beijing 100049, Peoples R China
Space Star Technol Co Ltd, Beijing 100194, Peoples R ChinaChinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R China
Jin, Biao
Li, Yuqiang
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Chinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R ChinaChinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R China
Li, Yuqiang
Jiang, Kecai
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Wuhan Univ, GNSS Res Ctr, 129 Luoyu Rd, Wuhan 430079, Peoples R ChinaChinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R China
Jiang, Kecai
Li, Zhulian
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Chinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R ChinaChinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R China
Li, Zhulian
Chen, Shanshan
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Space Star Technol Co Ltd, Beijing 100194, Peoples R ChinaChinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R China