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
DOI: 10.1134/S001679320908009X
Bibcode: 2009Ge&Ae..49.1096I
Ivanov, E. V.; Fainshtein, V. G.; Rudenko, G. V.
Russia
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.
2009
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Geomagnetism and Aeronomy
SOHO
2