MIOS optical subsystem for determining physical and chemical properties of meteors producing plasma irregularities
文献类型:期刊论文
作者 | Yang, Sipeng1,3,6![]() |
刊名 | ADVANCES IN SPACE RESEARCH
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出版日期 | 2021-08-01 |
卷号 | 68期号:3页码:1556-1567 |
关键词 | Optical meteor Meteoroid Spectroscopy MIOS |
ISSN号 | 0273-1177 |
DOI | 10.1016/j.asr.2021.03.031 |
英文摘要 | A Meteor and ionospheric Irregularity Observation System (MIOS)-optical subsystem, which currently consists of 26 video cameras (4 spectrographs) at two stations Sanya (18.3 degrees N, 109.6 degrees E) and Ledong (18.4 degrees N, 109 degrees E) separated by about 70 km was developed. One of the major goals of MIOS is to study how the entry of meteoroids into the Earth's atmosphere changes the ionosphere through combining measurements of optical meteor with radar specular and non-specular meteor echoes and ionospheric irregularity echoes. This paper outlines the MIOS optical subsystem design for optical meteor detecting and methods for inferring physical and chemical properties. The spectrum and common volume optical trail observations from the two stations allow identifying emissions from meteor and atmospheric species, and calculating the meteor velocity, trajectory and orbital parameters. Preliminary results of meteors detected by the MIOS optical subsystem during July-August 2019 are presented and discussed. (C) 2021 COSPAR. Published by Elsevier B.V. All rights reserved. |
WOS关键词 | DOUBLE-STATION ; SPECTROSCOPIC OBSERVATIONS ; SIMULTANEOUS RADAR ; MHZ RADAR ; SPECTRA ; ORBIT |
资助项目 | National Natural Science Foundation of China[41727803] ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences[E051850301] |
WOS研究方向 | Engineering ; Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences |
语种 | 英语 |
WOS记录号 | WOS:000663718200010 |
出版者 | ELSEVIER SCI LTD |
资助机构 | National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the Institute of Geology and Geophysics, Chinese Academy of Sciences |
源URL | [http://ir.iggcas.ac.cn/handle/132A11/101974] ![]() |
专题 | 地质与地球物理研究所_中国科学院地球与行星物理重点实验室 |
通讯作者 | Li, Guozhu |
作者单位 | 1.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China 2.Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing, Peoples R China 3.Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing, Peoples R China 4.Chinese Acad Sci, Inst Geol & Geophys, Mohe Observ Geophys, Beijing, Peoples R China 5.Mirasteilas Observ, Falera, Switzerland 6.Chinese Acad Sci, Innovat Acad Earth Sci, Beijing, Peoples R China |
推荐引用方式 GB/T 7714 | Yang, Sipeng,Wu, Zhi,Dubs, Martin,et al. MIOS optical subsystem for determining physical and chemical properties of meteors producing plasma irregularities[J]. ADVANCES IN SPACE RESEARCH,2021,68(3):1556-1567. |
APA | Yang, Sipeng.,Wu, Zhi.,Dubs, Martin.,Sun, Wenjie.,Hu, Lianhuan.,...&Li, Guozhu.(2021).MIOS optical subsystem for determining physical and chemical properties of meteors producing plasma irregularities.ADVANCES IN SPACE RESEARCH,68(3),1556-1567. |
MLA | Yang, Sipeng,et al."MIOS optical subsystem for determining physical and chemical properties of meteors producing plasma irregularities".ADVANCES IN SPACE RESEARCH 68.3(2021):1556-1567. |
入库方式: OAI收割
来源:地质与地球物理研究所
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