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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Research Article| February 26 2019
Filaments related to solar energetic particles
AIP Conf. Proc. 2075, 090013 (2019)
Tsvetan Tsvetkov, Rositsa Miteva, Nikola Petrov; Filaments related to solar energetic particles. AIP Conf. Proc. 26 February 2019; 2075 (1): 090013. https://doi.org/10.1063/1.5091227
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