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Solar Cycle Variation of the Mass-loss Rate of Coronal Mass Ejections

文献类型：期刊论文

作者Tang, Yijia1; Zhang, Xiaojuan1; Deng, Hui1; Wang, Feng1; Deng LH(邓林华)2,3; Mei, Ying1
刊名ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
出版日期2025-05-01
卷号278期号:1
ISSN号0067-0049
DOI10.3847/1538-4365/adc257
产权排序第3完成单位
文献子类Article
英文摘要Coronal mass ejections (CMEs) are known as the main drivers of the most severe space weather disturbances. Usually, the most severe geomagnetic storms are caused by massive and fast CMEs. The latitudinal dependence of the mass loss of CMEs for different types (regular and specific events) and in different solar cycles is rarely studied. Based on the latest data acquired by the Coordinated Data Analysis Workshop catalog covering solar cycles 23 and 24, we investigated the solar cycle variation of their mass-loss rate in detail. The main results are shown as follows: (1) The temporal distribution of the mass-loss rate is noticeably different from the occurrence rate of CMEs, and this difference might be attributed to the different types. The mass-loss rate of regular CMEs significantly follows the pattern of the solar cycle. (2) The latitudinal evolutions of the mass-loss rate of regular CMEs are indeed different from those of specific CMEs during solar cycles 23 and 24, suggesting that the source region and configuration of regular and specific CMEs differ from each other. (3) Rieger-type periodicity and the quasi-biennial oscillations are found in the long-term evolution of the CME mass-loss rate, but they exhibit different temporal aspects in different subsamples of CMEs. Our results might provide new insight into the solar-cycle dependence of the mass-loss rate of CMEs at different latitudes, and have potential implications for our understanding of the long-term evolution of the mass-loss process on solar-type stars.
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QUASI-BIENNIAL OSCILLATION ; RIEGER-TYPE PERIODICITY ; NORTH-SOUTH ASYMMETRY ; MAGNETO-ROSSBY WAVES ; BEHAVIOR ; WIND ; FREQUENCY ; FLARE ; FIELD ; VARIABILITY
资助项目MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809; NOAA National Centers for Environmental Information
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001473345100001
出版者IOP Publishing Ltd
资助机构MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809 ; NOAA National Centers for Environmental Information
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/28281]  
专题云南天文台_抚仙湖太阳观测站
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; Zhangxiaojuan@gzhu.edu.cn, denghui@gzhu.edu.cn, fengwang@gzhu.edu.cn;
2.School of Mathematics and Computer Science, Yunnan Minzu University, Kunming 650504, People's Republic of China; linhua.deng@ymu.edu.cn;
3.Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan, 650216, People's Republic of China
推荐引用方式
GB/T 7714		 Tang, Yijia,Zhang, Xiaojuan,Deng, Hui,et al. Solar Cycle Variation of the Mass-loss Rate of Coronal Mass Ejections[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2025,278(1).
APA Tang, Yijia,Zhang, Xiaojuan,Deng, Hui,Wang, Feng,邓林华,&Mei, Ying.(2025).Solar Cycle Variation of the Mass-loss Rate of Coronal Mass Ejections.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,278(1).
MLA Tang, Yijia,et al."Solar Cycle Variation of the Mass-loss Rate of Coronal Mass Ejections".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 278.1(2025).

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来源：云南天文台

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