ON THE VARIATION OF SOLAR RADIUS IN ROTATION CYCLES
文献类型:期刊论文
作者 | Qu ZN(屈智宁)1,2,3![]() ![]() ![]() |
刊名 | ASTROPHYSICAL JOURNAL
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出版日期 | 2015-01-10 |
卷号 | 798期号:2 |
关键词 | Sun: fundamental parameters Sun: magnetic fields Sun: rotation |
ISSN号 | 0004-637X |
产权排序 | 第一完成单位 |
通讯作者 | Qu, ZN (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Yunnan, Peoples R China. |
英文摘要 | The Date Compensated Discrete Fourier Transform and CLEANest algorithm are used to study the temporal variations of the solar radius observed at Rio de Janeiro Observatory from 1998 March 2 to 2009 November 6. The CLEANest spectra show several significant periodicities around 400, 312, 93.5, 86.2, 79.4, 70.9, 53.2, and 26.3 days. Then, combining the data on the daily solar radius measured at Calern Observatory and Rio de Janeiro Observatory and the corresponding daily sunspot areas, we study the short-term periodicity of the solar radius and the role of magnetic field in the variation of the solar radius. The rotation period of the daily solar radius is determined to be statistically significant. Moreover, its temporal evolution is anti-phase with that of sunspot activity, and it is found anti-phase with solar activity. Generally, the stronger solar activity is, the more obvious is the anti-phase relation of radius with solar activity. This indicates that strong magnetic fields have a greater inhibitive effect than weak magnetic fields on the variation of the radius. |
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] | DIAMETER MEASUREMENTS ; DIFFERENTIAL ROTATION ; TERM PERIODICITIES ; CONVECTION ZONE ; SUNSPOT NUMBERS ; CALERN SITE ; ASTROLABE ; CONSTANCY ; DYNAMO ; SUN |
收录类别 | SCI |
原文出处 | http://iopscience.iop.org/article/10.1088/0004-637X/798/2/113/meta |
语种 | 英语 |
WOS记录号 | WOS:000350853700048 |
公开日期 | 2016-05-03 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/6275] ![]() |
专题 | 云南天文台_太阳物理研究组 |
作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan 650011, China 2.University of Chinese Academy of Sciences, Beijing 100049, China 3.Key Laboratory of Solar Activity, National Astronomical Observatories, CAS, Beijing 100012, China 4.Research Center of Analysis and Measurement, Kunming University of Science and Technology, Kunming 650093, China 5.Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University) Ministry of Education, Nanjing 210093, China |
推荐引用方式 GB/T 7714 | Qu ZN,Kong DF,Xiang NB,et al. ON THE VARIATION OF SOLAR RADIUS IN ROTATION CYCLES[J]. ASTROPHYSICAL JOURNAL,2015,798(2). |
APA | Qu ZN,Kong DF,Xiang NB,&Feng, W.(2015).ON THE VARIATION OF SOLAR RADIUS IN ROTATION CYCLES.ASTROPHYSICAL JOURNAL,798(2). |
MLA | Qu ZN,et al."ON THE VARIATION OF SOLAR RADIUS IN ROTATION CYCLES".ASTROPHYSICAL JOURNAL 798.2(2015). |
入库方式: OAI收割
来源:云南天文台
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