HEMISPHERIC SUNSPOT UNIT AREA: COMPARISON WITH HEMISPHERIC SUNSPOT NUMBER AND SUNSPOT AREA

被引:12
作者
Li, K. J. [1 ,2 ]
Xiang, N. B. [1 ,3 ]
Qu, Z. N. [1 ,3 ]
Xie, J. L. [1 ,3 ]
机构
[1] Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China
[2] Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China
[3] Chinese Acad Sci, Grad Sch, Beijing 100863, Peoples R China
基金
中国国家自然科学基金;
关键词
Sun: activity; Sun: general; sunspots; NORTH-SOUTH ASYMMETRY; SOLAR-ACTIVITY RECONSTRUCTION; POLAR FACULAE; FLARE INDEX; R-S; CYCLE; VARIABILITY; COHERENCE; CATALOG; SHAPE;
D O I
10.1088/0004-6256/147/3/51
中图分类号
P1 [天文学];
学科分类号
0704 ;
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.
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页数:7
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