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Solar Cycle Variation of Interplanetary Coronal Mass Ejection Latitudes
Gao PX(高朋鑫)1,2; Li KJ(李可军)1,3; Gao, PX (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
Source PublicationJOURNAL OF ASTROPHYSICS AND ASTRONOMY
2010-09
Volume31Issue:3Pages:165-175
DOI10.1007/s12036-010-0014-9
Contribution Rank第1完成单位
Indexed BySCI
KeywordSun: Activity Coronal Mass Ejections (Cmes)
AbstractWith the use of interplanetary coronal mass ejections (ICMEs) compiled by Richardson and Cane from 1996 to 2007 and the associated coronal mass ejections (CMEs) observed by the Large Angle and Spectrometric Coronagraph (LASCO) onboard the Solar and Heliospheric Observatory (SOHO), we investigate the solar cycle variation of real ICME-associated CME latitudes during solar cycle 23 using Song et al.'s method. The results show the following: Although most of ICME-associated CMEs are distributed at low latitudes, there is a significant fraction of ICME-associated CMEs occurring at high latitudes. The latitudinal evolution of ICME-associated CMEs do not follow Sporer's sunspot law at low latitudes (thus, no 'butterfly diagram'); how-ever, at high latitudes, there may be a poleward motion and an equator-ward motion from the rise to the maximum to the declining phases.
Funding OrganizationNational Natural Science Foundation of China (NSFC) [10873032, 10921303, 40636031] ; National Key Research Science Foundation [2006CB806303] ; Chinese Academy of Sciences
Language英语
Subject AreaAstronomy & Astrophysics
SubtypeArticle
ISSN0250-6335
URL查看原文
Archive Date2010-09-10
WOS IDWOS:000282184900005
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordSOHO LASCO OBSERVATIONS ; REAL CME LATITUDES ; MAGNETIC CLOUDS ; WIND
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/6163
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, 650 011, China
2.Graduate University of Chinese Academy of Sciences, Beijing, 100 049, China
3.Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100 012, China
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Gao PX,Li KJ,Gao, PX . Solar Cycle Variation of Interplanetary Coronal Mass Ejection Latitudes[J]. JOURNAL OF ASTROPHYSICS AND ASTRONOMY,2010,31(3):165-175.
APA Gao PX,Li KJ,&Gao, PX .(2010).Solar Cycle Variation of Interplanetary Coronal Mass Ejection Latitudes.JOURNAL OF ASTROPHYSICS AND ASTRONOMY,31(3),165-175.
MLA Gao PX,et al."Solar Cycle Variation of Interplanetary Coronal Mass Ejection Latitudes".JOURNAL OF ASTROPHYSICS AND ASTRONOMY 31.3(2010):165-175.
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