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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
Authors:E. V. Ivanov  G. V. Rudenko  V. G. Fainshtein
Affiliation:(1) The Catholic University of America, Washington, DC, USA;(2) NASA Goddard Space Flight Center, Greenbelt, MD, USA;(3) Plasma Physics Division, Naval Research Laboratory, Washington, DC, USA
Abstract: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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