中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
HEMISPHERIC SUNSPOT UNIT AREA: COMPARISON WITH HEMISPHERIC SUNSPOT NUMBER AND SUNSPOT AREA

文献类型:期刊论文

作者Li KJ(李可军)1,2; Xiang NB(向南彬)1,3; Qu ZN(屈智宁)1,3; Xie JL(谢婧岚)1,3
刊名ASTRONOMICAL JOURNAL
出版日期2014-03
卷号147期号:3页码:1-7
关键词Sun: activity Sun: general sunspots
ISSN号0004-6256
产权排序第一完成单位
通讯作者Li, KJ (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China.
英文摘要The monthly mean northern and southern hemispheric sunspot numbers (SNs) and sunspot areas (SAs) in the time interval of 1945 January to 2012 December are utilized to construct the monthly northern and southern hemispheric sunspot unit areas (SUAs), which are defined as the ratio of hemispheric SA to SN. Hemispheric SUAs are usually found to rise at the beginning and to fall at the ending time of a solar cycle more rapidly, forming a more irregular cycle profile than hemispheric SNs and SAs, although it also presents Schwabe-cycle-like hemispheric SNs and SAs. Sunspot activity (SN, SA, and SUA) is found asynchronously and is asymmetrically distributed in the northern and southern hemispheres, and hemispheric SNs, SAs, and SUAs are not in phase in the two hemispheres. The similarity of hemispheric SNs and SAs is found to be much more obvious than that of hemispheric SUAs and SNs (or SAs), and also for their north-south asymmetry. A notable feature is found for the behavior of the SUA around the minimum time of cycle 24: the SUA rapidly decreases from the cycle maximum value to the cycle minimum value of sunspot cycles 19-24 within just 22 months.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]NORTH-SOUTH ASYMMETRY ; SOLAR-ACTIVITY RECONSTRUCTION ; POLAR FACULAE ; FLARE INDEX ; R-S ; CYCLE ; VARIABILITY ; COHERENCE ; CATALOG ; SHAPE
收录类别SCI
原文出处http://iopscience.iop.org/article/10.1088/0004-6256/147/3/51/meta
语种英语
WOS记录号WOS:000331125600006
源URL[http://ir.ynao.ac.cn/handle/114a53/6256]  
专题云南天文台_太阳物理研究组
作者单位1.National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China
2.Key Laboratory of Solar Activity, National Astronomical Observatories, CAS, Beijing 100012, China
3.Graduate School of CAS, Beijing 100863, China
推荐引用方式
GB/T 7714
Li KJ,Xiang NB,Qu ZN,et al. HEMISPHERIC SUNSPOT UNIT AREA: COMPARISON WITH HEMISPHERIC SUNSPOT NUMBER AND SUNSPOT AREA[J]. ASTRONOMICAL JOURNAL,2014,147(3):1-7.
APA Li KJ,Xiang NB,Qu ZN,&Xie JL.(2014).HEMISPHERIC SUNSPOT UNIT AREA: COMPARISON WITH HEMISPHERIC SUNSPOT NUMBER AND SUNSPOT AREA.ASTRONOMICAL JOURNAL,147(3),1-7.
MLA Li KJ,et al."HEMISPHERIC SUNSPOT UNIT AREA: COMPARISON WITH HEMISPHERIC SUNSPOT NUMBER AND SUNSPOT AREA".ASTRONOMICAL JOURNAL 147.3(2014):1-7.

入库方式: OAI收割

来源:云南天文台

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