We investigate the kinematics of 13 solar energetic particle (SEP) related eruptive prominences (EPs) and SEP spectral indices (using SOHO/ERNE proton data) for well observed set of events in the SDO era. From the height-time profiles of the EPs, we measured their average velocities and eruptive phase velocities. Relationships between proton spectral index γ and properties of the other associated solar phenomena (flare peak flux, CME speed, EPs speeds) are investigated.
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