PMO OpenIR  > 暗物质和空间天文实验室
Association of CMEs with solar surface activity during the rise and maximum phases of solar cycles 23 and 24
Gao, Peng-Xin1,2,3; Li, Ting2; Zhang, Jun2
2014-10-01
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
ISSN1674-4527
Volume14Issue:10Pages:1289-+
AbstractThe 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.
KeywordSun: Coronal Mass Ejections (Cmes) Sun: Filaments, Prominences Sun: Flares Sunspots
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1088/1674-4527/14/10/008
WOS KeywordCORONAL MASS EJECTIONS ; MISSION ; JET
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000342804500008
Citation statistics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/10551
Collection暗物质和空间天文实验室
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China
2.Chinese Acad Sci, Key Lab Solar Act, Natl Astron Observ, Beijing 100012, Peoples R China
3.Chinese Acad Sci, Key Lab Dark Matter & Space Astron, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
Recommended Citation
GB/T 7714
Gao, Peng-Xin,Li, Ting,Zhang, Jun. 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-+.
APA Gao, Peng-Xin,Li, Ting,&Zhang, Jun.(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-+.
MLA Gao, Peng-Xin,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-+.
Files in This Item:
File Name/Size DocType Version Access License
2014006Association o(557KB) 限制开放CC BY-NC-SAView Application Full Text
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Gao, Peng-Xin]'s Articles
[Li, Ting]'s Articles
[Zhang, Jun]'s Articles
Baidu academic
Similar articles in Baidu academic
[Gao, Peng-Xin]'s Articles
[Li, Ting]'s Articles
[Zhang, Jun]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Gao, Peng-Xin]'s Articles
[Li, Ting]'s Articles
[Zhang, Jun]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: 2014006Association of CMEs with solar surface activity during the rise and maximum phases of solar cycles 23 and 24.pdf
Format: Adobe PDF
This file does not support browsing at this time
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.