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The NTSC VLBI System and its application in UT1 measurement 被引量:3

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摘要 In order to measure the Universal Time(UT1)in real time,National Time Service Center(NTSC)has built a VGOS-like(VLBI Global Observing System)broadband VLBI network,which includes three13-m radio telescopes located in Jilin,Sanya and Kashi,and a data analysis center in Xi’an.Each station is equipped with a highly stable hydrogen atomic clock and a self-developed VLBI backend,and is colocated with two GPS receivers.This VGOS-like VLBI network may play an important role in improving the Chinese broadband VLBI technology and making valuable contributions to domestic VLBI measurements of UT1.In this paper,we introduce the specifications of this VLBI network,and present the UT1 measurements at C-band conducted in 2018 using the Jilin-Kashi baseline of this network.The comparisons between our UT1 estimates and those provided by IERS suggest that the NTSC VLBI network is capable to determine UT1 accurate at the level of 58.8μs.
作者 姚当 吴元伟 张波 孙靖 孙焱 徐双敬 刘佳 马浪明 弓剑军 杨颖 杨旭海 Dang Yao;Yuan-Wei Wu;Bo Zhang;Jing Sun;Yan Sun;Shuang-Jing Xu;Jia Liu;Lang-Ming Ma;Jian-Jun Gong;Ying Yang;Xu-Hai Yang(National Time Service Center,Chinese Academy of Sciences,Xi'an 710600,China;University of Chinese Academy of Sciences,Beijing 100049,China;Shanghai Astronomical Observatory,Chinese Academy of Sciences,Shanghai 200030,China;National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100101,China)
出处 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2020年第6期229-238,共10页 天文和天体物理学研究(英文版)
基金 supported by the National Natural Science Foundation of China(Grant Nos.11703033,11673051,11603001 and U1831136) the West Light Foundation of the Chinese Academy of Sciences(XAB2016A06) supported by the 100 Talents Project of the Chinese Academy of Sciences(CAS)。
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