Observation of Two Different Types of Coronal Mass Ejections

Details Observation of Two Different Types of Coronal Mass Ejections Observation of Two Different Types of Coronal Mass Ejections

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..325..421s&link_type=abstract

The Solar-B Mission and the Forefront of Solar Physics, ASP Conference Series, Vol. 325, Proceedings of the Fifth Solar-B Scienc

Physics

Scientific paper

For investigating the structure of Coronal Mass Ejections (CMEs), we classified them into two classes. One is defined as Type-A CMEs with loop-like configuration, and the other is defined as Type-B CMEs with halo structure. We examined the characteristics of both classes and found that they have distinctively different characteristics. Therefore, we claim that there are at least two basically different types among CMEs.

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