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...

Ausführliche Beschreibung

Bibliografische Detailangaben

Hauptverfasser:	Chin-Chun Wu, Natchimuthuk Gopalswamy, Ronld Paul Lepping, Seiji Yashiro
Format:	Artigo
Sprache:	Inglês
Veröffentlicht:	Springer 2013-01-01
Schriftenreihe:	Terrestrial, Atmospheric and Oceanic Sciences
Schlagworte:	Magnetic cloud Interplanetary coronal mass ejection Geomagnetic storm Solar flare Corotating interaction region
Online-Zugang:	http://tao.cgu.org.tw/images/attachments/v242p233.pdf
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