摘要
太阳活动高产区NOAA6891是一个岛型δ黑子,它有5条中性线,表现出不同的性质.其中第3条的横场比较弱,但是由于有剪切,所以有耀斑活动.而第2条中性线的横场较大,剪切得非常厉害,所以在这个区域产生了大量的耀斑,包括2个白光耀斑.正因为如此,所以要对磁场作三维分析,其中用磁场拓扑界面来分析是一种好的途径.
The superactive region NOAA 6891 is an : island' delta-sunspot. There are five magnetic inversion lines in it. Across the 2nd and 3rd invedon lines there are highly sheared field configurations, and at there two places a lot of flares occurred.Especially near the 2nd inversion line, two white-light flares were produced. Magnetic inversion lines have different characteristics. This is due to their different magnetic circumstances. So we should study three-dimensional magnetic fields, and it is a useful way to study the magnetic topology separatrices.
出处
《天文学报》
CSCD
北大核心
1997年第2期167-174,T001,共9页
Acta Astronomica Sinica
关键词
磁场中性线
磁场
拓扑界面
耀斑
太阳活动区
magnetic inversion line, magnetic topology separatrix, solar flare