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Coronal Propagation of Solar Protons during and after Their Stochastic Acceleration

Logachev, Yu. I.; Struminsky, A. B.; Grigorieva, I. Yu. +1 more

Solar protons in eruptive flares are stochastically accelerated in a wide spatial angle, and then they are effectively kept behind the expanding coronal mass ejection (CME) front, which can either bring protons to the magnetic-field line going to a remote observer or carry them away. We consider 13 solar proton events of cycle 24 in which protons …