Relationship betwwen of Coronal Mass Ejections and EIT Post Flare Arcades

Details Relationship betwwen of Coronal Mass Ejections and EIT Post Flare Arcades Relationship betwwen of Coronal Mass Ejections and EIT Post Flare Arcades

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsh13b1551y&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #SH13B-1551

Physics

2134 Interplanetary Magnetic Fields, 7509 Corona, 7513 Coronal Mass Ejections (2101), 7524 Magnetic Fields, 7924 Forecasting (2722)

Scientific paper

Our recent study indicates the orientation of a halo CME elongation may correspond to the orientation of the underlying flux rope. This is a continuation of the research and here we compare orientation angles of elongated LASCO CMEs, both halo and partial to the EIT post eruption arcades (PEA). Data for 100 events had been analyzed and er report the following: i) it is further supported that majority of halo CMEs are elongated in the direction of the axial field of PEA arcades; ii) this relationship holds true for partial CME and those events that originate further from the disk center. There is also an indication that events in the northern hemisphere generally exhibit better correlation that those in the southern hemisphere.

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