Dependence of geomagnetic activity during magnetic storms on the solar wind parameters for different types of streams: 2. Main phase of storm

被引：0
作者：
N. S. Nikolaeva
Yu. I. Yermolaev
I. G. Lodkina
机构：
[1] Russian Academy of Sciences,Space Research Institute
来源：
Geomagnetism and Aeronomy | 2012年 / 52卷
关键词：
Solar Wind; Interplanetary Magnetic Field; Magnetic Storm; Geomagnetic Storm; Geomagnetic Activity;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
The paper analyses the development of the main phase of magnetic storms with Dst ≤ −50 nT, the interplanetary source of which consists of eight types of solar wind streams: magnetic clouds (MC, 17 storms); corotating interaction regions (CIR, 49 storms); Ejecta (50 storms); compressed region (Sheath) before Ejecta ShE (34 storms); the Sheath before a magnetic cloud ShMC (6 storms); all Sheath before all ICME, ShE + ShMC (40 storms); all ICME, MC + Ejecta (67 storms); and an indeterminate type of stream IND (34 storms).
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页码：28 / 36
页数：8
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