A kinky heliospheric current sheet: Cause of CDAW-6 substorms
A kinky heliospheric current sheet: Cause of CDAW-6 substorms
复制标题
奇怪的日光层电流片：CDAW-6 亚暴的原因
DOI：
10.1029/gl011i004p00339
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发表时间：
1984
影响因子：
5.2
通讯作者：
R. Lin
中科院分区：
文献类型：
--
作者：
B. Tsurutani;C. Russell;J. King;R. Zwickl;R. Lin
两次磁层亚暴和第二次亚暴的增强是由行星际磁场和与弯曲的日球电流片（KHCS）相关的冲压压力变化引起的。负责行星际功能发生在一个高度压缩的区域之间的太阳耀斑相关的冲击波和冷驱动气体。排除了行星际结构是“磁云”的可能性。
Two magnetospheric substorms and the intensification of the second are caused by interplanetary magnetic field and ram pressure changes associated with a kinky heliospheric current sheet (KHCS). The responsible interplanetary features occur in a highly compressed region between a solar flare-associated shock wave and the cold driver gas. The possbility that the interplanetary structure is a “magnetic cloud” is ruled out.