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Initiation and propagation of coronal mass ejections

โœ Scribed by P. F. Chen


Publisher
Springer-Verlag
Year
2008
Tongue
English
Weight
110 KB
Volume
29
Category
Article
ISSN
0250-6335

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Two thirds of the Ha flares associated in time and position with coronal mass ejections (CME) observed by the Coronagraph/Polarimeter (C/P) or by the coronagraph on Skylab lie within 30 ~ of the solar limb. Among type II flares (those with type II radio spectral bursts) with C/P observations, 10 are