Numerical modeling of interplanetary coronal mass ejections and comparison with heliospheric images

Interplanetary coronal mass ejections (ICMEs) have complex magnetic and density structures, which are the result of their interaction with the structured solar wind and with previous eruptions. ICMEs are revealed by in situ measurements and in the past five years, through remote-sensing observations...

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Veröffentlicht in:	Journal of atmospheric and solar-terrestrial physics 2011-06, Vol.73 (10), p.1187-1200
Hauptverfasser:	Lugaz, N., Roussev, I.I.
Format:	Artikel
Sprache:	eng
Schlagworte:	Coronal mass ejection (CME) Magnetohydrodynamics (MHD)
Online-Zugang:	Volltext
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