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Phase Relationships Between the CME-Energy Cycle, the Sunspot-Area Cycle and the Flare-Index Cycle
Gao PX(高朋鑫)1,2,3; Xie JL(谢婧岚)1,4; Zhong, J5; Gao, PX (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China.
发表期刊SOLAR PHYSICS
2014-05
卷号289期号:5页码:1831-1841
DOI10.1007/s11207-013-0409-2
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 (Cmes) Sun: Flares Sun: Sunspots
摘要We study the phase relationships between the coronal-mass-ejection (CME) energy cycle, the sunspot-area cycle, and the flare-index cycle from 1996 to 2010. The results show the following: i) The activity cycle of the flare index significantly leads the activity cycle of the sunspot area. ii) The activity cycle of the CME energy is inferred to be almost in phase with the activity cycle of the sunspot area; the activity cycle of the CME energy at low latitudes slightly leads the activity cycle of the sunspot area; the CME energy at high latitudes is shown to significantly lag behind the sunspot area. iii) The CME energy is shown to significantly lag behind the flare index; the CME energy at low latitudes is shown to slightly lag behind the flare index; the CME energy at high latitudes is shown to significantly lag behind the flare index.
项目资助者Natural Science Funds of China [11273057, 11221063, 11203068, 11073010] ; 973 programs [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
ISSN0038-0938
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归档日期2014-02-21
WOS记录号WOS:000330985000024
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]CORONAL MASS EJECTIONS ; SOLAR-CYCLE ; POLAR FACULAE ; DISTRIBUTIONS ; INDICATORS ; HYSTERESIS ; ERUPTIONS
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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/114a53/6254
专题太阳物理研究组
通讯作者Gao, PX (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron 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, 100012, China
3.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210008, China
4.Graduate University of Chinese Academy of Sciences, Beijing, 100049, China
5.Kunming No. 3 Middle School, Kunming, 650011, China
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GB/T 7714
Gao PX,Xie JL,Zhong, J,et al. Phase Relationships Between the CME-Energy Cycle, the Sunspot-Area Cycle and the Flare-Index Cycle[J]. SOLAR PHYSICS,2014,289(5):1831-1841.
APA Gao PX,Xie JL,Zhong, J,&Gao, PX .(2014).Phase Relationships Between the CME-Energy Cycle, the Sunspot-Area Cycle and the Flare-Index Cycle.SOLAR PHYSICS,289(5),1831-1841.
MLA Gao PX,et al."Phase Relationships Between the CME-Energy Cycle, the Sunspot-Area Cycle and the Flare-Index Cycle".SOLAR PHYSICS 289.5(2014):1831-1841.
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