CORONAL X-RAY JETS OBSERVED WITH YOHKOH SXT

被引：0
|
作者：
SHIBATA, K [1 ]
YOKOYAMA, T [1 ]
SHIMOJO, M [1 ]
机构：
[1] TOKAI UNIV,DEPT PHYS,HIRATSUKA,KANAGAWA 25912,JAPAN
来源：
SOLAR FLARE, CORONAL AND HELIOSPHERIC DYNAMICS | 1995年 / 17卷 / 4/5期
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D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The soft X-ray telescope (SXT) aboard Yohkoh has discovered coronal X-ray jets associated with small flares in X-ray bright points (XBPs), emerging flux regions (EFRs), or active regions (ARs). The common observed characteristics of these jets are discussed mainly from morphological points of view. It is suggested that magnetic reconnection between emerging magnetic flux and the overlying coronal/chromospheric magnetic field is a key physical process for producing these jets.
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页码：197 / 200
页数：4
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