首页 | 本学科首页   官方微博 | 高级检索  
     检索      

行星际磁场扇形边界与地磁扰动
引用本文:谢榴香,都亨.行星际磁场扇形边界与地磁扰动[J].空间科学学报,1985,5(3):209-213.
作者姓名:谢榴香  都亨
作者单位:中国科学院空间物理研究所
摘    要:本文分析了地球通过行星际磁场扇形边界前后的AE、|Dst|、磁扰日出现的频次ND和磁静日出现的频次NQ四种地磁指数的变化规律, 根据磁场的极性变化可以将扇形边界分成以下四种类型, (Ⅰ)极性从负到正, (Ⅱ)极性从正到负, (Ⅲ)极性从负到多变以及(Ⅳ)极性从正到多变. 

收稿时间:1984-05-11

The Sector Boundary of IMF and the Geomagnetic Disturbance
Institution:Institute of Space Physics, Academia Sinica
Abstract:The variation of the geomagnetic indices AE, Dst, the frequency of occurrence of disturbance day ND and quiet day NQduring the time before and after the earth’s passage through the sector boundary of the interplanetary magnetic field (IMP) is studied. According to the change of the polarity of IMF at the sector boundary, the sector boundaries can be divided into the following types: (I) from negative to positive polarity; (II) from positive to negative polarity; (III) from negative to a varied polarity, and (IV) from positive to a varied polarity. The results are:The sector boundary type Iand IIcan be regarded as one of the sources of the geomagnetic disturbance. After the earth’s passage through the sector boundary the geomagnetic indices increase (but NQdecreases) and remain constant in three days.For sector boundary type III and IV, the variation of the IMF and geomagnetic indices are rather complicated. It is found that before the earth’s passage through the sector boundary, AE, Dst and ND have already increased and NQ decreased. 
Keywords:
本文献已被 CNKI 等数据库收录!
点击此处可从《空间科学学报》浏览原始摘要信息
点击此处可从《空间科学学报》下载免费的PDF全文
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号