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Morphological analysis of the large sunspot group of October 1972
Ding YJ(丁有济); Li WB(李维宝); Hong QF(洪琴芳); Li ZK(李治凯); DING, YJ
发表期刊CHINESE ASTRONOMY
1978
卷号2期号:1页码:70-90
DOI10.1016/0146-6364(78)90006-3
产权排序第1完成单位
收录类别SCI
摘要1. 1. The main morphological feature of this proton active region is the clockwise spiral structure of the penumbral filaments of the large preceding spot “A”. 2. 2. The formation of this spiral structure may be caused by the anti-clockwise spin of umbra “A”. This point is discussed in detail. 3. 3. The anti-clockwise rotation of the NS magnetic axis of the sunspot group was directly correlated to the spin of spot “A”, and the direction of both rotations was opposite to that of the effect of the differential rotation.
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0146-6364
URL查看原文
WOS记录号WOS:A1978GQ02600005
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
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文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/5990
专题太阳物理研究组
通讯作者DING, YJ
作者单位Yunnan Observatory, Academia Sinica, China
推荐引用方式
GB/T 7714
Ding YJ,Li WB,Hong QF,et al. Morphological analysis of the large sunspot group of October 1972[J]. CHINESE ASTRONOMY,1978,2(1):70-90.
APA Ding YJ,Li WB,Hong QF,Li ZK,&DING, YJ.(1978).Morphological analysis of the large sunspot group of October 1972.CHINESE ASTRONOMY,2(1),70-90.
MLA Ding YJ,et al."Morphological analysis of the large sunspot group of October 1972".CHINESE ASTRONOMY 2.1(1978):70-90.
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