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导致太阳耀斑爆发的暗条扭绞
林元章1; Gaizauskas V2
1994
Source Publication天文学报
ISSN0001-5245
Volume035Issue:002Pages:219
Abstract本文主要根据Ha线心和不同偏带的观测资料,结合紫外CIV1548谱线的测量结果,分析研究了1980年6月25日AR2522活动区中一段暗条在耀斑爆发前15分钟所经历的三次逐渐增强的间歇式扭绞,最终导致暗条破裂和耀斑爆发的物理过程,并且用无力场磁绳近似模拟时间条的扭绞运动,估算了暗条扭绞引直怕无力因子a的变化,轴向电流增大和守能,讨论了暗条的稳定性,试图对暗条的瓦解和耀斑爆发予以理论解释。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/51052
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.加拿大科学院Herzberg天体物理所
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
林元章,Gaizauskas V. 导致太阳耀斑爆发的暗条扭绞[J]. 天文学报,1994,035(002):219.
APA 林元章,&Gaizauskas V.(1994).导致太阳耀斑爆发的暗条扭绞.天文学报,035(002),219.
MLA 林元章,et al."导致太阳耀斑爆发的暗条扭绞".天文学报 035.002(1994):219.
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