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Observational evidence of high-altitude meteor trail from radar interferometer

文献类型：期刊论文

作者Li, Guozhu1,2; Ning, Baiqi1; Wan, Weixing1; Reid, I. M.3,4; Hu, Lianhuan1; Yue, Xinan5; Younger, J. P.3,4; Dolman, B. K.3,4
刊名GEOPHYSICAL RESEARCH LETTERS
出版日期2014-10-16
卷号41期号:19页码:6583-6589
ISSN号0094-8276
DOI10.1002/2014GL061478
文献子类Article
英文摘要Whether radar meteor echoes occur at high altitudes (above similar to 130 km) in the Earth's atmosphere is a long-standing question within the meteor radar community. Using observations from the Sanya VHF coherent radar interferometer during 11 July to 10 August 2013, we have found a new class of range-spread high-altitude meteor trail echoes (HAMEs), some of which appeared at similar to 170 km altitude lasting more than 10 s. A statistical analysis on the local time dependence of the identified HAME events shows a maximum around 00-04 LT. The results imply that there could be much more meteor mass input due to meteoroid sputtering at high altitudes in the Earth's atmosphere than previously thought.
WOS关键词LEONID METEORS ; IRREGULARITIES ; ECHOES
WOS研究方向Geology
语种英语
WOS记录号WOS:000344913800006
出版者AMER GEOPHYSICAL UNION
资助机构Natural Science Foundation of China(41422404 ; Natural Science Foundation of China(41422404 ; Natural Science Foundation of China(41422404 ; Natural Science Foundation of China(41422404 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; National Important Basic Research Project of China(2011CB811405) ; National Important Basic Research Project of China(2011CB811405) ; National Important Basic Research Project of China(2011CB811405) ; National Important Basic Research Project of China(2011CB811405) ; 41174136 ; 41174136 ; 41174136 ; 41174136 ; KZZD-EW-01-3) ; KZZD-EW-01-3) ; KZZD-EW-01-3) ; KZZD-EW-01-3) ; 41374163 ; 41374163 ; 41374163 ; 41374163 ; 41374164 ; 41374164 ; 41374164 ; 41374164 ; 41321003) ; 41321003) ; 41321003) ; 41321003) ; Natural Science Foundation of China(41422404 ; Natural Science Foundation of China(41422404 ; Natural Science Foundation of China(41422404 ; Natural Science Foundation of China(41422404 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; National Important Basic Research Project of China(2011CB811405) ; National Important Basic Research Project of China(2011CB811405) ; National Important Basic Research Project of China(2011CB811405) ; National Important Basic Research Project of China(2011CB811405) ; 41174136 ; 41174136 ; 41174136 ; 41174136 ; KZZD-EW-01-3) ; KZZD-EW-01-3) ; KZZD-EW-01-3) ; KZZD-EW-01-3) ; 41374163 ; 41374163 ; 41374163 ; 41374163 ; 41374164 ; 41374164 ; 41374164 ; 41374164 ; 41321003) ; 41321003) ; 41321003) ; 41321003) ; Natural Science Foundation of China(41422404 ; Natural Science Foundation of China(41422404 ; Natural Science Foundation of China(41422404 ; Natural Science Foundation of China(41422404 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; National Important Basic Research Project of China(2011CB811405) ; National Important Basic Research Project of China(2011CB811405) ; National Important Basic Research Project of China(2011CB811405) ; National Important Basic Research Project of China(2011CB811405) ; 41174136 ; 41174136 ; 41174136 ; 41174136 ; KZZD-EW-01-3) ; KZZD-EW-01-3) ; KZZD-EW-01-3) ; KZZD-EW-01-3) ; 41374163 ; 41374163 ; 41374163 ; 41374163 ; 41374164 ; 41374164 ; 41374164 ; 41374164 ; 41321003) ; 41321003) ; 41321003) ; 41321003) ; Natural Science Foundation of China(41422404 ; Natural Science Foundation of China(41422404 ; Natural Science Foundation of China(41422404 ; Natural Science Foundation of China(41422404 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; Chinese Academy of Sciences(KZCX2-YW-Y10 ; National Important Basic Research Project of China(2011CB811405) ; National Important Basic Research Project of China(2011CB811405) ; National Important Basic Research Project of China(2011CB811405) ; National Important Basic Research Project of China(2011CB811405) ; 41174136 ; 41174136 ; 41174136 ; 41174136 ; KZZD-EW-01-3) ; KZZD-EW-01-3) ; KZZD-EW-01-3) ; KZZD-EW-01-3) ; 41374163 ; 41374163 ; 41374163 ; 41374163 ; 41374164 ; 41374164 ; 41374164 ; 41374164 ; 41321003) ; 41321003) ; 41321003) ; 41321003)
源URL[http://ir.iggcas.ac.cn/handle/132A11/85141]  
专题中国科学院地质与地球物理研究所
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.Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing, Peoples R China
3.ATRAD Pty Ltd, Adelaide, SA, Australia
4.Univ Adelaide, Sch Chem & Phys, Adelaide, SA, Australia
5.Univ Corp Atmospher Res, COSM Program Off, Boulder, CO USA
推荐引用方式
GB/T 7714		 Li, Guozhu,Ning, Baiqi,Wan, Weixing,et al. Observational evidence of high-altitude meteor trail from radar interferometer[J]. GEOPHYSICAL RESEARCH LETTERS,2014,41(19):6583-6589.
APA Li, Guozhu.,Ning, Baiqi.,Wan, Weixing.,Reid, I. M..,Hu, Lianhuan.,...&Dolman, B. K..(2014).Observational evidence of high-altitude meteor trail from radar interferometer.GEOPHYSICAL RESEARCH LETTERS,41(19),6583-6589.
MLA Li, Guozhu,et al."Observational evidence of high-altitude meteor trail from radar interferometer".GEOPHYSICAL RESEARCH LETTERS 41.19(2014):6583-6589.

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来源：地质与地球物理研究所

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