Pulsar and Magnetar Navigation with Fermi/GBM and GECAM
The determination of the absolute and relative position of a spacecraft is critical for its operation, observations, data analysis, scientific studies, as well as deep-space exploration in general. A spacecraft that can determine its own absolute position autonomously may perform better than those t...
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Article |
| Language: | English |
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IOP Publishing
2023-01-01
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| Series: | The Astrophysical Journal Supplement Series |
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| Online Access: | https://doi.org/10.3847/1538-4365/acc79d |
| _version_ | 1797699720618967040 |
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| author | Xi-Hong Luo Shuo Xiao Shi-Jie Zheng Ming-Yu Ge You-Li Tuo Shao-Lin Xiong Shuang-Nan Zhang Fang-Jun Lu Yue Huang Cheng Yang Qi-Jun Zhi Li-Ming Song Wen-Xi Peng Xiang-Yang Wen Xin-Qiao Li Zheng-Hua An Jin Wang Ping Wang Ce Cai Cheng-Kui Li Xiao-Bo Li Fan Zhang Ai-Jun Dong Wei Xie Jian-Chao Feng Qing-Bo Ma Hua Wang De Lun-Hua Shang Xin Xu Meng-Xuan Zhang Zi-Ping Dong Shi-Jun Dang |
| author_facet | Xi-Hong Luo Shuo Xiao Shi-Jie Zheng Ming-Yu Ge You-Li Tuo Shao-Lin Xiong Shuang-Nan Zhang Fang-Jun Lu Yue Huang Cheng Yang Qi-Jun Zhi Li-Ming Song Wen-Xi Peng Xiang-Yang Wen Xin-Qiao Li Zheng-Hua An Jin Wang Ping Wang Ce Cai Cheng-Kui Li Xiao-Bo Li Fan Zhang Ai-Jun Dong Wei Xie Jian-Chao Feng Qing-Bo Ma Hua Wang De Lun-Hua Shang Xin Xu Meng-Xuan Zhang Zi-Ping Dong Shi-Jun Dang |
| author_sort | Xi-Hong Luo |
| collection | DOAJ |
| description | The determination of the absolute and relative position of a spacecraft is critical for its operation, observations, data analysis, scientific studies, as well as deep-space exploration in general. A spacecraft that can determine its own absolute position autonomously may perform better than those that must rely on transmission solutions. In this work, we report an absolute navigation accuracy of ∼20 km using 16 day Crab pulsar data observed with Fermi’s Gamma-ray Burst Monitor (GBM). In addition, we propose a new method with the inverse process of the triangulation for joint navigation using repeated bursts like those from the magnetar SGR J1935+2154 observed by the Gravitational-wave High-energy Electromagnetic Counterpart All-sky Monitor and GBM. |
| first_indexed | 2024-03-12T04:11:55Z |
| format | Article |
| id | doaj.art-6da9c7d6483342eeb1fa0c54d18881b4 |
| institution | Directory Open Access Journal |
| issn | 0067-0049 |
| language | English |
| last_indexed | 2024-03-12T04:11:55Z |
| publishDate | 2023-01-01 |
| publisher | IOP Publishing |
| record_format | Article |
| series | The Astrophysical Journal Supplement Series |
| spelling | doaj.art-6da9c7d6483342eeb1fa0c54d18881b42023-09-03T10:55:50ZengIOP PublishingThe Astrophysical Journal Supplement Series0067-00492023-01-0126611610.3847/1538-4365/acc79dPulsar and Magnetar Navigation with Fermi/GBM and GECAMXi-Hong Luo0Shuo Xiao1https://orcid.org/0000-0003-2957-2806Shi-Jie Zheng2Ming-Yu Ge3https://orcid.org/0000-0002-2749-6638You-Li Tuo4https://orcid.org/0000-0003-3127-0110Shao-Lin Xiong5https://orcid.org/0000-0002-4771-7653Shuang-Nan Zhang6https://orcid.org/0000-0001-5586-1017Fang-Jun Lu7https://orcid.org/0000-0003-3248-6087Yue Huang8Cheng Yang9Qi-Jun Zhi10https://orcid.org/0000-0001-9389-5197Li-Ming Song11https://orcid.org/0000-0003-0274-3396Wen-Xi Peng12Xiang-Yang Wen13Xin-Qiao Li14https://orcid.org/0000-0003-3466-9493Zheng-Hua An15Jin Wang16Ping Wang17https://orcid.org/0000-0003-0466-2223Ce Cai18https://orcid.org/0000-0002-6540-2372Cheng-Kui Li19Xiao-Bo Li20https://orcid.org/0000-0003-4585-589XFan Zhang21Ai-Jun Dong22https://orcid.org/0000-0003-4151-0771Wei Xie23https://orcid.org/0000-0001-5553-4577Jian-Chao Feng24Qing-Bo Ma25https://orcid.org/0000-0001-9493-4565Hua Wang De26Lun-Hua Shang27Xin Xu28Meng-Xuan Zhang29Zi-Ping Dong30Shi-Jun Dang31Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China xiaoshuo@gznu.edu.cn; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; xiongsl@ihep.ac.cnGuizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China xiaoshuo@gznu.edu.cn; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; xiongsl@ihep.ac.cnKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cnKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cnKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cn; Institut für Astronomie und Astrophysik, University of Tübingen , Sand 1, D-72076 Tübingen, GermanyKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cnKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cn; University of Chinese Academy of Sciences, Chinese Academy of Sciences , Beijing 100049, People's Republic of ChinaKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cnKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cnGuizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China xiaoshuo@gznu.edu.cn; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; xiongsl@ihep.ac.cnGuizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China xiaoshuo@gznu.edu.cn; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; xiongsl@ihep.ac.cnKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cnKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cnKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cnKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cnKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cnKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cnKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cnCollege of Physics, Hebei Normal University , 20 South Erhuan Road, Shijiazhuang 050024, People's Republic of ChinaKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cnKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cnKey Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China zhangsn@ihep.ac.cn, qjzhi@gznu.edu.cnGuizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China xiaoshuo@gznu.edu.cn; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; xiongsl@ihep.ac.cnGuizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China xiaoshuo@gznu.edu.cn; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; xiongsl@ihep.ac.cnGuizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China xiaoshuo@gznu.edu.cn; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; xiongsl@ihep.ac.cnGuizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China xiaoshuo@gznu.edu.cn; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; xiongsl@ihep.ac.cnGuizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China xiaoshuo@gznu.edu.cn; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; xiongsl@ihep.ac.cnGuizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China xiaoshuo@gznu.edu.cn; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; xiongsl@ihep.ac.cnGuizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China xiaoshuo@gznu.edu.cn; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; xiongsl@ihep.ac.cnSchool of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; xiongsl@ihep.ac.cnSchool of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; xiongsl@ihep.ac.cnGuizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China xiaoshuo@gznu.edu.cn; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; xiongsl@ihep.ac.cnThe determination of the absolute and relative position of a spacecraft is critical for its operation, observations, data analysis, scientific studies, as well as deep-space exploration in general. A spacecraft that can determine its own absolute position autonomously may perform better than those that must rely on transmission solutions. In this work, we report an absolute navigation accuracy of ∼20 km using 16 day Crab pulsar data observed with Fermi’s Gamma-ray Burst Monitor (GBM). In addition, we propose a new method with the inverse process of the triangulation for joint navigation using repeated bursts like those from the magnetar SGR J1935+2154 observed by the Gravitational-wave High-energy Electromagnetic Counterpart All-sky Monitor and GBM.https://doi.org/10.3847/1538-4365/acc79dPulsarsMagnetarsAstronomical techniques |
| spellingShingle | Xi-Hong Luo Shuo Xiao Shi-Jie Zheng Ming-Yu Ge You-Li Tuo Shao-Lin Xiong Shuang-Nan Zhang Fang-Jun Lu Yue Huang Cheng Yang Qi-Jun Zhi Li-Ming Song Wen-Xi Peng Xiang-Yang Wen Xin-Qiao Li Zheng-Hua An Jin Wang Ping Wang Ce Cai Cheng-Kui Li Xiao-Bo Li Fan Zhang Ai-Jun Dong Wei Xie Jian-Chao Feng Qing-Bo Ma Hua Wang De Lun-Hua Shang Xin Xu Meng-Xuan Zhang Zi-Ping Dong Shi-Jun Dang Pulsar and Magnetar Navigation with Fermi/GBM and GECAM The Astrophysical Journal Supplement Series Pulsars Magnetars Astronomical techniques |
| title | Pulsar and Magnetar Navigation with Fermi/GBM and GECAM |
| title_full | Pulsar and Magnetar Navigation with Fermi/GBM and GECAM |
| title_fullStr | Pulsar and Magnetar Navigation with Fermi/GBM and GECAM |
| title_full_unstemmed | Pulsar and Magnetar Navigation with Fermi/GBM and GECAM |
| title_short | Pulsar and Magnetar Navigation with Fermi/GBM and GECAM |
| title_sort | pulsar and magnetar navigation with fermi gbm and gecam |
| topic | Pulsars Magnetars Astronomical techniques |
| url | https://doi.org/10.3847/1538-4365/acc79d |
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