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In the solar flare observed on June 3, 2012, high energy gamma-rays andneutrons were observed. The event includes a remarkable feature of a highneutron/gamma-ratio in the secondary particles. We have examined whether thishigh n/$\gamma$-ratio can be explained by simulation. As a result ofsimulations using the GEANT4 program, the high n/$\gamma$-ratio may bereproduced for the case that helium and other heavy ions were dominantlyaccelerated in the flare.

Angular and Abundance Distribution of High-energy Gamma Rays and Neutrons Simulated by GEANT4 Code for Solar Flares