Correlation between the parameters of coronal mass ejections and features of their propagation in the corona with the large-scale structure of the solar magnetic field

Details Correlation between the parameters of coronal mass ejections and features of their propagation in the corona with the large-scale structure of the solar magnetic field Correlation between the parameters of coronal mass ejections and features of their propagation in the corona with the large-scale structure of the solar magnetic field

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ge%26ae..49.1096i&link_type=abstract

Geomagnetism and Aeronomy, Volume 49, Issue 8, pp.1096-1100

Physics

Scientific paper

Correlation between the parameters of coronal mass ejections (CMEs) that
are detected on the LASCO coronographs and are associated with eruptive
prominences and the distances of CME axes from the coronal streamer belt
has been analyzed. The deviations of CME trajectories from the radial
direction have been investigated.

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