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Distributions of Energy and Mass of Coronal Mass Ejections
Gao PX(高朋鑫)1,2; Li KJ(李可军)1,2; Xu JC(徐景晨)1,3; Gao, PX (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
发表期刊SOLAR PHYSICS
2011-10
卷号273期号:1页码:117-123
DOI10.1007/s11207-011-9853-z
产权排序第1完成单位
收录类别SCI
关键词Methods: Data Analysis Sun: Coronal Mass Ejections Sun: Filaments Sun: Flares
摘要The present study investigates the energy and mass distributions of all (11 322) coronal mass ejections (CMEs), 1406 CMEs associated solely with flares (FL CMEs), and 325 CMEs associated solely with filament eruptions (FE CMEs), all of which were observed by the Large Angle and Spectrometric Coronagraph on board the Solar and Heliospheric Observatory (SOHO/LASCO) from January 1996 to December 2009. The results show the following. i) The mean energy of FL CMEs is significantly lower than that of all CMEs. The mean energy of FE CMEs is significantly higher than those of FL CMEs and all CMEs. ii) The mean mass of FL CMEs is slightly larger than that of all CMEs. The mean mass of FE CMEs is significantly larger than those of FL CMEs and all CMEs. Our results suggest that CMEs should shed excess helicity stored in the corona and that the magnetic complexity determines the likelihood of CMEs.
项目资助者NSFC [10873032, 10921303, 40636031] ; National Key Research Science Foundation [2011CB811406] ; Chinese Academy of Sciences ; Foundation of Key Laboratory of Solar Activity of National Astronomical Observatories of Chinese Academy of Sciences [KLSA2011-03]
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0038-0938
URL查看原文
归档日期2011-11-11
WOS记录号WOS:000297125700008
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]KINETIC-PROPERTIES ; FLARES ; ERUPTIONS ; FILAMENTS ; CYCLE ; MODEL ; CMES
引用统计
被引频次:3[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/114a53/6170
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 Observatory, Chinese Academy of Sciences, Kunming, 650011, China
2.Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China
3.Graduate University of Chinese Academy of Sciences, Beijing, 100049, China
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GB/T 7714
Gao PX,Li KJ,Xu JC,et al. Distributions of Energy and Mass of Coronal Mass Ejections[J]. SOLAR PHYSICS,2011,273(1):117-123.
APA Gao PX,Li KJ,Xu JC,&Gao, PX .(2011).Distributions of Energy and Mass of Coronal Mass Ejections.SOLAR PHYSICS,273(1),117-123.
MLA Gao PX,et al."Distributions of Energy and Mass of Coronal Mass Ejections".SOLAR PHYSICS 273.1(2011):117-123.
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