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几个活动区精细H↓α结构的物理浅析
吴蓓; 宋慕陶; 胡福民
1994
Source Publication天体物理学报
ISSN0253-2379
Volume014Issue:002Pages:178
Abstract本文利用紫金山天文台赣榆站太阳精细结构望远镜拍得的高分辨率色球Hα照片,分析了三个典型活动区,文中利用并检验了七十年代获得的磁图推导法则,应用自己的数值模拟知识和Zwaan对AFS系新浮流区概括的特征,参考七十和九十年代总结的有关耀斑和Ellerman Bomb的再现规律,逐日分析活动区发展,定出其内部的中性线位置,提出简单和复合中性线的区分,由AFS系和亮谱斑同时出现判断新浮流区,从近离带图找等
Language英语
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/30543
Collection中国科学院紫金山天文台
Affiliation中国科学院紫金山天文台
First Author Affilication中国科学院紫金山天文台
Recommended Citation
GB/T 7714
吴蓓,宋慕陶,胡福民. 几个活动区精细H↓α结构的物理浅析[J]. 天体物理学报,1994,014(002):178.
APA 吴蓓,宋慕陶,&胡福民.(1994).几个活动区精细H↓α结构的物理浅析.天体物理学报,014(002),178.
MLA 吴蓓,et al."几个活动区精细H↓α结构的物理浅析".天体物理学报 014.002(1994):178.
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