Signatures of two distinct driving mechanisms in the evolution of coronal mass ejections in the lower corona

We present a comparison between two simulations of coronal mass ejections (CMEs), in the lower corona, driven by different flux rope mechanisms presented in the literature. Both mechanisms represent different magnetic field configurations regarding the amount of twist of the magnetic field lines and...

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Veröffentlicht in:	Journal of Geophysical Research: Space Physics 2011-04, Vol.116 (A4), p.n/a
Hauptverfasser:	Loesch, C., Opher, M., Alves, M. V., Evans, R. M., Manchester, W. B.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Astrophysics coronal mass ejection Driving ability flux rope interplanetary shocks magnetic field configuration Magnetic fields magnetohydrodynamic simulations Planetology solar corona Space Sun
Online-Zugang:	Volltext
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