The auroral occurrence over Zhongshan Station, Antarctica

被引：4

作者：

胡红桥

刘瑞源

杨惠根

机构：

来源：

Chinese Journal of Polar Science | 1999年 / 02期

关键词：

aurora; auroral occurrence; Kp index; Antarctica; Zhongshan Station;

D O I：

暂无

中图分类号：

P427.33 [极光];

学科分类号：

0706 ; 070601 ;

摘要：

The auroral data observed by all sky TV camera during 1995 and 1997 at Zhongshan Station of Antarctica are used to analyze the statistic characteristics of the aurora over Zhongshan Station. Around postnoon (1200 - 1600UT ) and midnight (2000 - 0100 UT ), the aurora appears more frequently and stronger than those in evening (1600- 2000UT ). The corona type auroras mainly occur at poleward and overhead of Zhongshan Station during postnoon and around midnight. The hand type auroras mainly appear during postnoon. while during evening and around midnight only appear at equatorward. The active surges mostly appear around midnight,while the transpolar arcs mainly occur after midnight. Except for the transpolar arcs. the occurrences of the other three type auroras are related with Kp index. Usually Zhongshan Station enters the auroral oval at postnoon,the exact time depends on Kp index.

引用

页码：101 / 109

页数：9

共 3 条

[1]

Kikuchi M, Sato N(1999b): Postnoon aurora observedat Zhongshan Station.Antarctica during quiet period -A case study. J. Wuhan Univ. (Nat. Hu HQ,Liu RY,Yang HG,Wang JF,Makita K. Sci.Ed. ) .

[2]

Lu DR(1998): Geospace environrnental monitoring at Zhongshan Station.Mem. Natl. Inst. PolarRes.Spec. Liu RY. Issue .

[3]

Liu RY (1998 ): Postnoon aurora observed at Zhongshan Station, Antarctica -A case study. Makita K,Kikuchi M,Sato N,Ayukawa M,Wang X,Yang HG. Proc. NIPR Symp. Upper Atmos. Phys .

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