Observation of upper atmospheric temperature by Kunming all-sky meteor radar

被引:9
|
作者
Yi Wen [1 ,2 ]
Chen Jin-Song [2 ,3 ,4 ]
Ma Chun-Bo [1 ]
Li Na [2 ]
Zhao Zhen-Wei [2 ]
机构
[1] Guilin Univ Elect Technol, Sch Informat & Commun, Guilin 541004, Peoples R China
[2] China Res Inst Radio Wave Propagat, Natl Key Lab Electron Magnet Environm, Qingdao 266107, Peoples R China
[3] Chinese Acad Sci, State Key Lab Space Weather, Beijing 100190, Peoples R China
[4] Univ Chinese Acad Sci, Beijing 100049, Peoples R China
来源
关键词
Meteor radar; Atmospheric temperature; Bipolar diffusion coefficient; Temperature gradient; Mesopause; Height of peak meteor activity; DIFFUSION; LIDAR;
D O I
10.6038/cjg20140804
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Using the data collected by the all-sky meteor radar with two different operating frequencies at the Kunming station (25. 6 degrees N, 103. 8 degrees E) during the special joint observation experiment in 2011, we determined the mesopause above the height of peak meteor activity based on the method improved by Hocking with different temperature gradient retrieval of atmospheric temperature at 88 km and 85 km over Kunming. Comparison with the Aura satellite temperature data shows that two separate meteor radars can measure correct atmospheric temperature at the height of peak meteor activity, however the correlation between temperature determined by the meteor radar using temperature gradient model and satellite temperature is not well. While the temperature determined by meteor radar using satellite temperature gradients have good correlation with satellite temperature. It is concluded that the accurate temperature gradient is very important in the Hocking's method.
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页码:2423 / 2432
页数:10
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