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![]() |
刊名 | ASTRONOMISCHE NACHRICHTEN
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出版日期 | 2023-01-31 |
页码 | 9 |
关键词 | ephemerides pulsars reference systems |
ISSN号 | 0004-6337 |
DOI | 10.1002/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. |
入库方式: OAI收割
来源:国家授时中心
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