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Association of CMEs with solar surface activity during the rise and maximum phases of solar cycles 23 and 24
Gao PX(高朋鑫)1,2,3; Li, T2; Zhang, J2; Gao, PX (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
发表期刊RESEARCH IN ASTRONOMY AND ASTROPHYSICS
2014-10
卷号14期号:10页码:1289-1300
DOI10.1088/1674-4527/14/10/008
产权排序第1完成单位
收录类别SCI
关键词Sun: Coronal Mass Ejections (Cmes) Sun: Flares Sun: Filaments Sunspots Prominences
摘要The cyclical behaviors of sunspots, flares and coronal mass ejections (CMEs) for 54 months from 2008 November to 2013 April after the onset of Solar Cycle (SC) 24 are compared, for the first time, with those of SC 23 from 1996 November to 2001 April. The results are summarized below. (i) During the maximum phase, the number of sunspots in SC 24 is significantly smaller than that for SC 23 and the number of flares in SC 24 is comparable to that of SC 23. (ii) The number of CMEs in SC 24 is larger than that in SC 23 and the speed of CMEs in SC 24 is smaller than that of SC 23 during the maximum phase. We individually survey all the CMEs (1647 CMEs) from 2010 June to 2011 June. A total of 161 CMEs associated with solar surface activity events can be identified. About 45% of CMEs are associated with quiescent prominence eruptions, 27% of CMEs only with solar flares, 19% of CMEs with both active-region prominence eruptions and solar flares, and 9% of CMEs only with active-region prominence eruptions. Comparing the association of the CMEs and their source regions in SC 24 with that in SC 23, we notice that the characteristics of source regions for CMEs during SC 24 may be different from those of SC 23.
项目资助者National Natural Science Foundation of China [11203068, 11273057, 11303050, 11025315] ; National Basic Research Program of China (973 program) [2011CB811406, 2012CB957801] ; Chinese Academy of Sciences ; Foundation of Key Laboratory of Solar Activity of National Astronomical Observatories of Chinese Academy of Sciences [KLSA201302] ; Key Laboratory of Dark Matter and Space Astronomy of Purple Mountain Observatory of Chinese Academy of Sciences [DMS2012KT008]
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN1674-4527
URL查看原文
归档日期2014-11-27
WOS记录号WOS:000342804500008
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]CORONAL MASS EJECTIONS ; MISSION ; JET
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被引频次:1[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/6242
专题太阳物理研究组
通讯作者Gao, PX (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
作者单位1.National Astronomical Observatories/Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China
2.Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
3.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China
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Gao PX,Li, T,Zhang, J,et al. Association of CMEs with solar surface activity during the rise and maximum phases of solar cycles 23 and 24[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2014,14(10):1289-1300.
APA Gao PX,Li, T,Zhang, J,&Gao, PX .(2014).Association of CMEs with solar surface activity during the rise and maximum phases of solar cycles 23 and 24.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,14(10),1289-1300.
MLA Gao PX,et al."Association of CMEs with solar surface activity during the rise and maximum phases of solar cycles 23 and 24".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 14.10(2014):1289-1300.
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