The joint use of high-resolution data from SDO and PROBA2 satellites and LASCO/SOHO coronographs enabled us to examine early stages of initiation and propagation of six limb CMEs registered in June 2010 - June 2011. For five events under consideration, the CME initiation is marked by filament (prominence) eruption or by a loop-like structure having another nature. Subsequently, several loop-like structures having higher brightness and following each other at different velocities appear in the region of the CME initiation. The CME frontal structure is formed by these loop-like structures. The CME kinematics and such CME characteristics as angular size and longitudinal to latitudinal size ratio was found for considered all events. We have drawn a conclusion about the possible existence of two CME types dependent on the velocity profile.
Central European Astrophysical Bulletin
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- coronal mass ejections;
- initiation and propagation;