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Kinetic properties of coronal mass ejections corrected for the projection effect in Cycle 23
Gao PX(高朋鑫)1,2; Li KJ(李可军)1; Li, QX3; Gao, PX (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2009-04-01
Volume394Issue:2Pages:1031-1036
DOI10.1111/j.1365-2966.2009.14390.x
Contribution Rank第1完成单位
Indexed BySCI
KeywordSun: Coronal Mass Ejections Sun: Filaments Sun: Flares
AbstractUsing Howard et al.s method, we investigate, before and after the projection correction, the speed and acceleration distributions for 1747 coronal mass ejections (CMEs) associated solely with flares (FL CMEs) and 631 CMEs associated solely with filament eruptions (FE CMEs) observed by the Large Angle and Spectrometric Coronagraph on board the Solar and Heliographic Observatory (SOHO/LASCO) from 1996 September to 2007 September, corresponding to almost an entire solar cycle. The results show the following. (1) Before the correction, the speed distributions for FL and FE CMEs are statistically different from each other; after the correction, the speed distributions for FL and FE CMEs should also be statistically different from each other. (2) Before the correction, the acceleration distributions for FL and FE CMEs are statistically different from each other. However, after the correction, FL and FE CMEs should have quite similar acceleration distributions.
Funding OrganizationNSFC [10573034, 40636031] ; National Key Research Science Foundation [2006CB806303] ; Chinese Academy of Sciences
Language英语
Subject AreaAstronomy & Astrophysics
SubtypeArticle
ISSN0035-8711
URL查看原文
Archive Date2009-03-17
WOS IDWOS:000264242000035
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordSPEEDS ; CMES ; TRANSIENTS ; EMISSION ; VELOCITY ; MINIMUM ; FLARES
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Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/6142
Collection太阳物理研究组
Corresponding AuthorGao, PX (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
Affiliation1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China
2.Graduate School of Chinese Academy of Sciences, Beijing 100049, China
3.Department of Physics, Chongqing University, Chongqing 400044, China
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Gao PX,Li KJ,Li, QX,et al. Kinetic properties of coronal mass ejections corrected for the projection effect in Cycle 23[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2009,394(2):1031-1036.
APA Gao PX,Li KJ,Li, QX,&Gao, PX .(2009).Kinetic properties of coronal mass ejections corrected for the projection effect in Cycle 23.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,394(2),1031-1036.
MLA Gao PX,et al."Kinetic properties of coronal mass ejections corrected for the projection effect in Cycle 23".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 394.2(2009):1031-1036.
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