YNAO OpenIR  > 太阳物理研究组
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
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: filaments, prominences Sun: flares sunspots
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.

资助项目National Natural Science Foundation of China[11203068] ; National Natural Science Foundation of China[11273057] ; National Natural Science Foundation of China[11303050] ; National Natural Science Foundation of China[11025315] ; National Basic Research Program of China (973 program)[2011CB811406] ; National Basic Research Program of China (973 program)[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]
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
学科领域天文学 ; 太阳与太阳系 ; 太阳物理学
学科门类理学 ; 理学::天文学
文章类型Article
出版者NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
出版地20A DATUN RD, CHAOYANG, BEIJING, 100012, PEOPLES R CHINA
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
引用统计
被引频次:6[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(高朋鑫)
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
第一作者单位中国科学院云南天文台
通讯作者单位中国科学院云南天文台
推荐引用方式
GB/T 7714
Gao PX,Li, T,Zhang, J. 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.(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.
条目包含的文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
Association of CMEs (557KB)期刊论文出版稿开放获取CC BY-NC-SA浏览 请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Gao PX(高朋鑫)]的文章
[Li, T]的文章
[Zhang, J]的文章
百度学术
百度学术中相似的文章
[Gao PX(高朋鑫)]的文章
[Li, T]的文章
[Zhang, J]的文章
必应学术
必应学术中相似的文章
[Gao PX(高朋鑫)]的文章
[Li, T]的文章
[Zhang, J]的文章
相关权益政策
暂无数据
收藏/分享
文件名: Association of CMEs with solar surface activity during the rise and maximum phases of solar cycles 23 and 24.pdf
格式: Adobe PDF
所有评论 (0)
暂无评论
 

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。