Impact of the annular solar eclipse on June 21, 2020 on BPL time service performance

被引:3
作者
Chen, Yingming [1 ,2 ,3 ,4 ]
Feng, Ping [1 ,2 ,3 ]
Changhong, Liu [2 ]
Chen, Yongqi [2 ,3 ]
Huang, Luxi [1 ,2 ,3 ,4 ]
Duan, Jianwen [2 ]
Hua, Yu [1 ,2 ,4 ]
Li, Xiaohui [1 ,2 ,3 ,4 ]
机构
[1] Univ Chinese Acad Sci, Beijing 100049, Peoples R China
[2] Chinese Acad Sci, Natl Time Serv Ctr, Xian 710600, Peoples R China
[3] Fengkai Low Frequency Time Code Time Serv Stn, Zhaoqing 526500, Peoples R China
[4] Chinese Acad Sci, Key Lab Precise Nav & Timing Technol, Xian 710600, Peoples R China
关键词
D O I
10.1063/5.0064445
中图分类号
TB3 [工程材料学];
学科分类号
0805 ; 080502 ;
摘要
BPL is a special Chinese long-wave time service system constructed and maintained by the National Time Service Center of the Chinese Academy of Sciences. Two experimental paths were designed to analyze the impact of the annular solar eclipse that occurred on June 21, 2020, on the BPL time service performance. In the first path, the receiving point was located in the ring eclipse zone, whereas in the other path, the sky-wave reflection point was located in the ring eclipse zone. The time of arrival (TOA) data during 19-23 June 2020 at the Sanya test point (sky-wave reflection point located in the ring eclipse zone) and field strength from 21 to 22 June 2020 at the Xiamen test point (receiving point located in the ring eclipse zone) were measured and analyzed. The experimental results show that under normal conditions of BPL time service signal transmission, the TOA and field strength undergo significant changes during the annular solar eclipse, the TOA data change up to 5.17 mu s, and the field strength data change up to 17.72 dB mu V. The data tend to increase initially and then decrease. This change is consistent with the ionospheric change caused by the annular solar eclipse. The BPL time service performance is affected at the receiving points located in the south of the BPL time service station with the great circle distance ranging from 1426 to 1844 km. (C) 2021 Author(s).
引用
收藏
页数:10
相关论文
共 22 条
  • [1] [Anonymous], 1986, J SHAANXI OBS, V12-31, P62
  • [2] Ionospheric Total Electron Content Response to the Great American Solar Eclipse of 21 August 2017
    Cherniak, Iurii
    Zakharenkova, Irina
    [J]. GEOPHYSICAL RESEARCH LETTERS, 2018, 45 (03) : 1199 - 1208
  • [3] Global Responses of the Coupled Thermosphere and Ionosphere System to the August 2017 Great American Solar Eclipse
    Dang, Tong
    Lei, Jiuhou
    Wang, Wenbin
    Zhang, Binzheng
    Burns, Alan
    Le, Huijun
    Wu, Qian
    Ruan, Haibing
    Dou, Xiankang
    Wan, Weixing
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2018, 123 (08) : 7040 - 7050
  • [4] Spectral solar variations during the eclipse of March 20th, 2015 at two European sites
    Groebner, Julian
    Kazadzis, Stelios
    Kouremeti, Natalia
    Doppler, Lionel
    Tagirov, Rinat
    Shapiro, Alexander I.
    [J]. RADIATION PROCESSES IN THE ATMOSPHERE AND OCEAN, 2017, 1810
  • [5] Nightside Detection of a Large-Scale Thermospheric Wave Generated by a Solar Eclipse
    Harding, B. J.
    Drob, D. P.
    Buriti, R. A.
    Makela, J. J.
    [J]. GEOPHYSICAL RESEARCH LETTERS, 2018, 45 (08) : 3366 - 3373
  • [6] Ionospheric response over Europe during the solar eclipse of March 20, 2015
    Hoque, Mohammed Mainul
    Wenzel, Daniela
    Jakowski, Norbert
    Gerzen, Tatjana
    Berdermann, Jens
    Wilken, Volker
    Kriegel, Martin
    Sato, Hiroatsu
    Borries, Claudia
    Minkwitz, David
    [J]. JOURNAL OF SPACE WEATHER AND SPACE CLIMATE, 2016, 6
  • [7] Hu Xiong, 2011, Chinese Journal of Space Science, V31, P596
  • [8] Ionospheric Responses at Low Latitudes to the Annular Solar Eclipse on 21 June 2020
    Huang, Fuqing
    Li, Qiaoling
    Shen, Xuhui
    Xiong, Chao
    Yan, Rui
    Zhang, Shun-Rong
    Wang, Wenbin
    Aa, Ercha
    Zhong, Jiahao
    Dang, Tong
    Lei, Jiuhou
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2020, 125 (10)
  • [9] [李涌涛 Li Yongtao], 2018, [空间科学学报, Chinese Journal of Space Science], V38, P847
  • [10] Pan L., 1990, CHIN J RADIO SCI, V5, P38, DOI [10.13443/j.cjors.1990.01.009, DOI 10.13443/J.CJORS.1990.01.009]