Hemispheric Distribution of Solar Active Regions during Solar Cycles 23-25
文献类型:期刊论文
作者 | Liu, Yuxia1; Xu, Tingting1; Wan, Miao1; Deng, Linhua1; Zhao, Xinhua2,3; Qi, Shiyang4; Xiang NB(向南彬)5![]() |
刊名 | ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
![]() |
出版日期 | 2025-06-01 |
卷号 | 278期号:2 |
ISSN号 | 0067-0049 |
DOI | 10.3847/1538-4365/adcd60 |
产权排序 | 第5完成单位 |
文献子类 | Article |
英文摘要 | Solar active regions (ARs) are crucial for understanding the long-term evolution of solar activities and predicting eruptive phenomena, including solar flares and coronal mass ejections. However, the cycle-dependent properties in the north-south asymmetry of ARs are not fully understood. In this study, we investigate the hemispheric distribution of ARs from Carrington rotations 1909-2278 (between 1996 May and 2023 November) by using three parameters that describe the magnetic field distribution of ARs: number, area, and flux. The main findings are as follows: (1) The three AR parameters show significant hemispheric asymmetry in cycles 23-25. The strong correlation between the AR area and flux indicates that they can better reflect the intrinsic properties of the solar magnetic field. (2) The correlation between sunspot activity and AR parameters varies in the two hemispheres across the different cycles. The AR parameters provide additional information for the variations in sunspot activity, which can better predict the intensity and cyclical changes of solar activity. (3) The variation in the fitting slope sign of the asymmetry index for AR parameters reflects periodic changes in hemispheric ARs, providing valuable insights into the activity of other stars. (4) Both the dominant hemisphere and the cumulative trend of AR parameters display a cycle-dependent behavior. Moreover, the trend variations in the AR area and flux are similar, reflecting the long-term evolutionary characteristics of the solar magnetic field. Our analysis results are relevant for understanding the hemispheric coupling of solar magnetic activity and its cyclic evolutionary patterns. |
学科主题 | 天文学 ; 太阳与太阳系 |
URL标识 | 查看原文 |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
WOS关键词 | NORTH-SOUTH ASYMMETRY ; LIVE HOMOGENEOUS DATABASE ; MAGNETIC-FIELD REVERSAL ; NUMBERS R-N ; SUNSPOT ACTIVITY ; PHASE ; AREAS ; PREDICTION ; FACULAE ; FLUX |
资助项目 | National Nature Science Foundation of China[12463009]; Yunnan Fundamental Research Projects[202301AV070007]; Yunnan Fundamental Research Projects[202401AU070026]; Yunnan Fundamental Research Projects[202501AU070154]; The Yunnan Revitalization Talent Support Program Innovation Team Project[202405AS350012]; Scientific Research Foundation Project of Yunnan Education Department[2025Y0720]; Scientific Research Foundation Project of Yunnan Education Department[2025Y0721]; Scientific Research Foundation Project of Yunnan Education Department[2025J0502]; GHfund A[202407016295] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:001502267300001 |
出版者 | IOP Publishing Ltd |
资助机构 | National Nature Science Foundation of China[12463009] ; Yunnan Fundamental Research Projects[202301AV070007, 202401AU070026, 202501AU070154] ; The Yunnan Revitalization Talent Support Program Innovation Team Project[202405AS350012] ; Scientific Research Foundation Project of Yunnan Education Department[2025Y0720, 2025Y0721, 2025J0502] ; GHfund A[202407016295] |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/28338] ![]() |
专题 | 云南天文台_抚仙湖太阳观测站 云南天文台_中国科学院天体结构与演化重点实验室 |
通讯作者 | Zhou, Weihong |
作者单位 | 1.School of Mathematics and Computer Science, Yunnan Minzu University, Kunming, Yunnan, 650504, People's Republic of China; zwh@ymu.edu.cn; 2.State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, People's Republic of China; 3.Radio Science and Technology Center (π Center), Chengdu, Sichuan, 610041, People's Republic of China; 4.College of Science, Henan Agricultural University, Zhengzhou, Henan, 450002, People's Republic of China; 5.Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan, 650216, People's Republic of China; 6.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, Yunnan, 650216, People's Republic of China |
推荐引用方式 GB/T 7714 | Liu, Yuxia,Xu, Tingting,Wan, Miao,et al. Hemispheric Distribution of Solar Active Regions during Solar Cycles 23-25[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2025,278(2). |
APA | Liu, Yuxia.,Xu, Tingting.,Wan, Miao.,Deng, Linhua.,Zhao, Xinhua.,...&Zhou, Weihong.(2025).Hemispheric Distribution of Solar Active Regions during Solar Cycles 23-25.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,278(2). |
MLA | Liu, Yuxia,et al."Hemispheric Distribution of Solar Active Regions during Solar Cycles 23-25".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 278.2(2025). |
入库方式: OAI收割
来源:云南天文台
浏览0
下载0
收藏0
其他版本
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。