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Mid-term Periodicity of Coronal Mass Ejections during the Time Interval 1996-2022
Ouyang, Zhuolang1,2; Deng, Hui1,2; Wang, Feng1,2; Deng LH(邓林华)3,4; Mei, Ying1,2; Zhang, XiaoJuan1,2
发表期刊ASTROPHYSICAL JOURNAL
2024-07-01
卷号970期号:1
DOI10.3847/1538-4357/ad4d9f
产权排序第4完成单位
收录类别SCI
摘要Coronal mass ejections (CMEs) exhibit a wide range of quasiperiodic variations and are crucial for our understanding of the cyclical evolution of large-scale magnetic fields. However, the mid-term periodicities of different types of CMEs associated with different processes at the source location need to be clearly understood. Based on the CDAW catalog released by the Large Angle and Spectroscopic Coronagraph mission on the Solar and Heliospheric Observatory, we investigated the period of CMEs based on the speeds and accelerations using the continuous wavelet transformation method. Our results revealed that the distribution of CMEs over time is quite distinctly different for different speeds, and there are Rieger-type periods and quasi-biennial oscillations of the CMEs. The two types of periodic signals show significant differences in solar cycles 23 and 24. Furthermore, the periodicity patterns for the northern hemisphere differ from those in the southern hemisphere. The potential mechanisms and explanations of the results are also discussed.
资助项目National SKA Program of China, Guangzhou Science[2020SKA0110300]; National Natural Science Foundation of China[12373097]; Guangzhou Science,Technology Funds[2023A03J0016]; Major Key Project of Peng Cheng Laboratory; Basic and Applied Basic Research Foundation Project of Guangdong Province[2024A1515011503]; Yunnan Revitalization Talent Support Program Innovation Team Project; Yunnan Fundamental Research Project[202301AV070007]
项目资助者National SKA Program of China, Guangzhou Science[2020SKA0110300] ; National Natural Science Foundation of China[12373097] ; Guangzhou Science,Technology Funds[2023A03J0016] ; Major Key Project of Peng Cheng Laboratory ; Basic and Applied Basic Research Foundation Project of Guangdong Province[2024A1515011503] ; Yunnan Revitalization Talent Support Program Innovation Team Project ; Yunnan Fundamental Research Project[202301AV070007]
语种英语
学科领域天文学 ; 太阳与太阳系
文章类型Article
出版者IOP Publishing Ltd
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS记录号WOS:001270974200001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]SOLAR-CYCLES 23 ; QUASI-BIENNIAL OSCILLATIONS ; MAGNETIC-FIELD ; SUNSPOT AREA ; BEHAVIOR ; FLARES ; ACCELERATION ; 154-DAY ; SPEEDS
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文献类型期刊论文
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条目标识符http://ir.ynao.ac.cn/handle/114a53/27489
专题抚仙湖太阳观测和研究基地
作者单位1.Center for Astrophysics and Great Bay Center of National Astronomical Data Center, Guangzhou University, Guangzhou 510006, People's Republic of China; [email protected], [email protected], [email protected];
2.Peng Cheng Laboratory, Shenzhen 518000, People's Republic of China;
3.School of Mathematics and Computer Science, Yunnan Minzu University, Kunming 650504, People's Republic of China; [email protected];
4.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China
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Ouyang, Zhuolang,Deng, Hui,Wang, Feng,et al. Mid-term Periodicity of Coronal Mass Ejections during the Time Interval 1996-2022[J]. ASTROPHYSICAL JOURNAL,2024,970(1).
APA Ouyang, Zhuolang,Deng, Hui,Wang, Feng,邓林华,Mei, Ying,&Zhang, XiaoJuan.(2024).Mid-term Periodicity of Coronal Mass Ejections during the Time Interval 1996-2022.ASTROPHYSICAL JOURNAL,970(1).
MLA Ouyang, Zhuolang,et al."Mid-term Periodicity of Coronal Mass Ejections during the Time Interval 1996-2022".ASTROPHYSICAL JOURNAL 970.1(2024).
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