Jet phenomena in the solar atmosphere caused by interaction between emerging flux and coronal fields

被引：0
|
作者：
Miyagoshi, T [1 ]
Yokoyama, T [1 ]
Isobe, H [1 ]
Shibata, K [1 ]
机构：
[1] Kyoto Univ, Kwasan Observ, Yamashima Ku, Kyoto 6078471, Japan
来源：
Solar-B Mission and the Forefront of Solar Physics, Proceedings | 2004年 / 325卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We have studied jet phenomena in the solar atmosphere with MHD numerical simulations. Emerging flux could interact coronal magnetic fields through magnetic reconnection. Then, magnetic energy is released and magnetic topology drastically changes. Our numerical simulation results show that coronal jets are produced through this process.
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收藏
页码：69 / 74
页数：6
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