VARIATIONS OF THE IMF B-Z COMPONENT OVER A SOLAR-ACTIVITY CYCLE FOR DIFFERENT REGIMES OF SOLAR-WIND FORMATION

被引：1
|
作者：
KOVALENKO, VA
MOLODYKH, SI
机构：
[1] Institute for Solar-Terrestrial Physics, Irkutsk, 664033
来源：
ASTRONOMISCHE NACHRICHTEN | 1995年 / 316卷 / 02期
关键词：
SUN; CORONA; SOLAR WIND; B-Z COMPONENT; VARIATIONS;
D O I：
10.1002/asna.2103160205
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The behavioural features of the IMF B-z component for different solar wind velocity regimes have been studied. The study revealed a significant difference in variations of the B-z component between high-speed and low-speed regimes. Formation mechanisms for the IMF meridional component as well as the relationship of B-z with dynamical properties of the large-scale magnetic fields on the Sun are discussed.
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页码：105 / 111
页数：7
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