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Evolution of morphological features of CMEs deduced from catastrophe model of solar eruptions
DOI: 10.1016/j.newast.2004.04.004
Bibcode: 2004NewA....9..611L
Lin, J.; Soon, W.
We describe the evolution of morphological features of the magnetic configuration of CME according to the catastrophe model developed previously. For the parameters chosen for the present work, roughly half of the total mass is nominally contained in the initial flux rope, while the remaining plasma is brought by magnetic reconnection from the cor…
2004
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New Astronomy
SOHO
22