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Space debris observation performance research of CSTAR at Kunlun Station in Antarctica
Li, Gongqiang1,2; Jiang, Hai1,2; Cheng, Haowen1,2; Liu, Jing1,2; Yang, Chenwei3; Jiang, Peng3
刊名ADVANCES IN SPACE RESEARCH
2019-10-15
卷号64期号:8页码:1527-1536
关键词Antarctica Space debris Detection Simulation Telescopes
ISSN号0273-1177
DOI10.1016/j.asr.2019.07.023
英文摘要Increasing space debris has seriously threatened the safety of spacecraft of various countries. The polar regions are the most densely distributed regions of Low-Earth orbit (LEO) space debris, and are ideal sites for observing LEO space debris. Through the real observation data and detection capabilities simulation, the advantages of China's Kunlun Station in Antarctica in observing LEO space debris are analyzed. Firstly, the real observation data of Chinese Small Telescope Array (CSTAR) are analyzed and compared with the space objects cataloging database (mean www.space-track.org), which confirms the high performance and superiority of Kunlun Station in LEO space debris observation. Secondly, the space debris observation performance of CSTAR is simulated and compared with its historical observation data in the same period, to confirm the reliability of the simulation model. Finally, based on the real observation data and simulation results, some hypothesis simulations and prospects for future space debris observation facilities at Kunlun Station are made. The simulation results can provide support for future observations at Kunlun Station in Antarctica. (C) 2019 COSPAR. Published by Elsevier Ltd. All rights reserved.
资助项目National Natural Science Foundation of China, China[11803052] ; Space Debris Research Project, China[KJSP2016010101] ; Space Debris Research Project, China[KJSP2016020101] ; Space Debris Research Project, China[KJSP2016020201] ; Space Debris Research Project, China[KJSP2016020301] ; Natural Science Foundation of Shanghai, China[18ZR1443300]
WOS关键词DOME ; ENVIRONMENT
WOS研究方向Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences
语种英语
出版者ELSEVIER SCI LTD
WOS记录号WOS:000488322700004
资助机构National Natural Science Foundation of China, China ; National Natural Science Foundation of China, China ; Space Debris Research Project, China ; Space Debris Research Project, China ; Natural Science Foundation of Shanghai, China ; Natural Science Foundation of Shanghai, China ; National Natural Science Foundation of China, China ; National Natural Science Foundation of China, China ; Space Debris Research Project, China ; Space Debris Research Project, China ; Natural Science Foundation of Shanghai, China ; Natural Science Foundation of Shanghai, China ; National Natural Science Foundation of China, China ; National Natural Science Foundation of China, China ; Space Debris Research Project, China ; Space Debris Research Project, China ; Natural Science Foundation of Shanghai, China ; Natural Science Foundation of Shanghai, China ; National Natural Science Foundation of China, China ; National Natural Science Foundation of China, China ; Space Debris Research Project, China ; Space Debris Research Project, China ; Natural Science Foundation of Shanghai, China ; Natural Science Foundation of Shanghai, China
内容类型期刊论文
源URL[http://ir.bao.ac.cn/handle/114a11/28036]  
专题中国科学院国家天文台
通讯作者Li, Gongqiang
作者单位1.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
2.China Natl Space Adm, Space Debris Observat & Data Applicat Ctr, Beijing 100101, Peoples R China
3.Polar Res Inst China, Shanghai 200136, Peoples R China
推荐引用方式
GB/T 7714
Li, Gongqiang,Jiang, Hai,Cheng, Haowen,et al. Space debris observation performance research of CSTAR at Kunlun Station in Antarctica[J]. ADVANCES IN SPACE RESEARCH,2019,64(8):1527-1536.
APA Li, Gongqiang,Jiang, Hai,Cheng, Haowen,Liu, Jing,Yang, Chenwei,&Jiang, Peng.(2019).Space debris observation performance research of CSTAR at Kunlun Station in Antarctica.ADVANCES IN SPACE RESEARCH,64(8),1527-1536.
MLA Li, Gongqiang,et al."Space debris observation performance research of CSTAR at Kunlun Station in Antarctica".ADVANCES IN SPACE RESEARCH 64.8(2019):1527-1536.
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