Analysis on magnetic storms reported by Beijing observatory

被引:6
作者
Li, Q
Gao, YF
Han, DS
机构
[1] China Earthquake Adm, Inst Geophys, Beijing 100081, Peoples R China
[2] Chinese Acad Sci, Key Lab Space Weather, Beijing 100080, Peoples R China
[3] Kyoto Univ, Dept Geophys, Grad Sch Sci, Kyoto 6068502, Japan
关键词
magnetic storm; occurrence; asymmetry; statistics;
D O I
10.1016/j.jastp.2005.02.016
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
A complete statistical study is made for all magnetic storms reported by Beijing observatory during 1979 to 2000. It includes occurrence dependence on type of the storm, intensity of the storm, and time (year, season, and month). A comparison between the occurrence and the number of sunspots is also carried out. Further statistical analysis for part of the great magnetic storms shows that there are obvious differences between activity level represented by Beijing observatory and that by Dst. Such differences depend upon local time of Beijing (BLT). Cubic polynomial fitting results show that the activity level is lower at dawn and higher at dusk in Beijing than that represented by Dst, and the difference between dusk and dawn is about 63% of Dst. (c) 2005 Elsevier Ltd. All rights reserved.
引用
收藏
页码:853 / 861
页数:9
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