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

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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Bibliographic Details
Main Authors:	Chin-Chun Wu, Natchimuthuk Gopalswamy, Ronld Paul Lepping, Seiji Yashiro
Format:	Article
Language:	English
Published:	Chinese Geoscience Union 2013-01-01
Series:	Terrestrial, Atmospheric and Oceanic Sciences
Subjects:	Magnetic cloud Interplanetary coronal mass ejection Geomagnetic storm Solar flare Corotating interaction region
Online Access:	http://tao.cgu.org.tw/images/attachments/v242p233.pdf

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