中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
An application of pulsar timing in dynamic reference frame transformation of solar system

文献类型:期刊论文

作者Zhu, Xing-zhi1,2; Tong, Ming-lei1,2; Zhao, Cheng-shi1,2; Yang, Ting-gao2; Gao, Yu-ping1,2
刊名ASTRONOMISCHE NACHRICHTEN
出版日期2023-01-31
页码9
关键词ephemerides pulsars reference systems
ISSN号0004-6337
DOI10.1002/asna.20220026
英文摘要The establishment of pulsar space-time reference frame is of great significance for X-ray pulsar deep space navigation. To demonstrate that the pulsar parameters are accurate enough to be used as a spatial reference, the transformation parameters, that is, alpha, beta, and gamma, of different reference frames determined based on pulsar timing are shown and compared with that of the heliocentric coordinates of Earth-Moon barycenter. The JPL ephemerides such as DE421, DE200 and INPOP series, are mainly selected for conversion parameter calculation. For the best-determined parameter gamma, the discrepancy between the two different data is 0.38 mas/1.33 sigma. The timing positions of pulsars clearly show the frame-tie of different ephemerides, indicating that MSPs have the potential to be a candidate for constructing time-space standard. It is also found that the rotation angles change linearly with time, and PSR J0437 - 4715 plays a critical role in the fitting of alpha. By employing a few high-quality MSPs, the transformation precision of the right ascension is evaluated to be on the order of sub-milliarcsecond, which is an order of magnitude higher than that of the declination.
WOS关键词EPHEMERIDES ; PACKAGE ; TEMPO2 ; TIE
资助项目National SKA Program of China[2020SKA0120103] ; National Natural Science Foundation of China (NSFC)[U1831130] ; National Natural Science Foundation of China (NSFC)[11973046] ; program of Young Scholars Western China[XAB2021YN27]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000921252300001
出版者WILEY-V C H VERLAG GMBH
资助机构National SKA Program of China ; National SKA Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; program of Young Scholars Western China ; program of Young Scholars Western China ; National SKA Program of China ; National SKA Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; program of Young Scholars Western China ; program of Young Scholars Western China ; National SKA Program of China ; National SKA Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; program of Young Scholars Western China ; program of Young Scholars Western China ; National SKA Program of China ; National SKA Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; program of Young Scholars Western China ; program of Young Scholars Western China
源URL[http://210.72.145.45/handle/361003/14356]  
专题国家授时中心_守时理论与方法研究室
通讯作者Zhu, Xing-zhi; Tong, Ming-lei
作者单位1.Chinese Acad Sci, Natl Time Serv Ctr, Key Lab Time & Frequency Primary Stand, Xian, Peoples R China
2.Chinese Acad Sci, Natl Time Serv Ctr, 3 Shuyuan East Rd, Xian, Shaanxi, Peoples R China
推荐引用方式
GB/T 7714
Zhu, Xing-zhi,Tong, Ming-lei,Zhao, Cheng-shi,et al. An application of pulsar timing in dynamic reference frame transformation of solar system[J]. ASTRONOMISCHE NACHRICHTEN,2023:9.
APA Zhu, Xing-zhi,Tong, Ming-lei,Zhao, Cheng-shi,Yang, Ting-gao,&Gao, Yu-ping.(2023).An application of pulsar timing in dynamic reference frame transformation of solar system.ASTRONOMISCHE NACHRICHTEN,9.
MLA Zhu, Xing-zhi,et al."An application of pulsar timing in dynamic reference frame transformation of solar system".ASTRONOMISCHE NACHRICHTEN (2023):9.

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