Characteristics of Magnetic Clouds and Interplanetary Coronal Mass Ejections which Cause Intense Geomagnetic Storms

We present the results of a statistical data analysis of the geo-effectiveness of non-magnetic-cloud interplanetary coronal mass ejections (ICMEs) and compare them with those of magnetic-cloud (MC) interplanetary coronal mass ejections observed during solar cycle 23. (The term ICME as used here will...

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Prif Awduron:	Chin-Chun Wu, Natchimuthuk Gopalswamy, Ronld Paul Lepping, Seiji Yashiro
Fformat:	Artigo
Iaith:	Inglês
Cyhoeddwyd:	Springer 2013-01-01
Cyfres:	Terrestrial, Atmospheric and Oceanic Sciences
Pynciau:	Magnetic cloud Interplanetary coronal mass ejection Geomagnetic storm Solar flare Corotating interaction region
Mynediad Ar-lein:	http://tao.cgu.org.tw/images/attachments/v242p233.pdf
Tagiau:	Ychwanegu Tag Dim Tagiau, Byddwch y cyntaf i dagio'r cofnod hwn!