Characteristics of low-latitude Pi 2 pulsations along the 210 degrees magnetic meridian

被引:18
作者
Osaki, H [1 ]
Yumoto, K [1 ]
Fukao, K [1 ]
Shiokawa, K [1 ]
Menk, FW [1 ]
Fraser, BJ [1 ]
机构
[1] UNIV NEWCASTLE,DEPT PHYS,NEWCASTLE,NSW 2308,AUSTRALIA
来源
JOURNAL OF GEOMAGNETISM AND GEOELECTRICITY | 1996年 / 48卷 / 11期
关键词
D O I
10.5636/jgg.48.1421
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
In order to understand the characteristics of lower-latitude Pi 2 geomagnetic pulsations along a magnetic meridian, we have analyzed 1 year's data from the Adelaide (geomagnetic latitude Phi = -46.72 degrees), Birdsville (-37.08 degrees), Weipa (-23.06 degrees), Guam (9.02 degrees), Chichijima (20.65 degrees), Kagoshima (25.23 degrees), and Moshiri (37.76 degrees) stations along the 210 degrees magnetic meridian. The characteristics of the lower-latitude (\Phi\ < 50 degrees) Pi 2 pulsations are summarized as follows: (1) 80% of H- and D-component Pi 2 events show very similar wave forms and the same frequency component; (2) not only H-component Pi 2 events but also D-component Pi 2 events are observed within +/-5 s; (3) H-component Pi 2 amplitudes are of almost the same order, but D-component Pi 2 pulsations have a minimum near the magnetic equator and increase exponentially from lower to higher latitudes; (4) the observed amplitudes of both H- and D-component Pi 2 pulsations are larger in the summer hemisphere than in the winter hemisphere. Results 1 and 2 show that lower-latitude Pi 2 pulsations are not propagating-mode but global-mode oscillations in the inner magnetosphere. Result 4 cannot be explained by the ordinary screening effect in the ionosphere but gives a clue to the unresolved generation mechanism of lower-latitude Pi 2 pulsations.
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页码:1421 / 1430
页数:10
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