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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
Source PublicationSOLAR PHYSICS
2014-05
Volume289Issue:5Pages:1831-1841
DOI10.1007/s11207-013-0409-2
Contribution Rank第1完成单位
Indexed BySCI
KeywordMethods: Data Analysis Sun: Coronal Mass Ejections (Cmes) Sun: Flares Sun: Sunspots
Abstract

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.

Funding ProjectNatural Science Funds of China[11273057] ; Natural Science Funds of China[11221063] ; Natural Science Funds of China[11203068] ; Natural Science Funds of China[11073010] ; 973 programs[2011CB811406] ; 973 programs[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]
Funding OrganizationNatural 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]
Language英语
Subject Area天文学 ; 太阳与太阳系
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeArticle
PublisherSPRINGER,
Publication PlaceVAN GODEWIJCKSTRAAT 30, 3311 GZ DORDRECHT, NETHERLANDS
ISSN0038-0938
URL查看原文
Archive Date2014-02-21
WOS IDWOS:000330985000024
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordCORONAL MASS EJECTIONS ; SOLAR-CYCLE ; POLAR FACULAE ; DISTRIBUTIONS ; INDICATORS ; HYSTERESIS ; ERUPTIONS
Citation statistics
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/6254
Collection太阳物理研究组
Corresponding AuthorGao PX(高朋鑫)
Affiliation1.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
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Corresponding Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Gao PX,Xie JL,Zhong, J. 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.(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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