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The energetic particle event that occurred on 314 DOY in 2000 is a good sample to investigate particle acceleration mechanisms because both the coronal mass ejection and the energetic particles were observed. We obtained energetic particles using the stochastic differential equation method with the velocity of the shock wave and the assumptions of the energy spectrum of the input pre-accelerated particles and the diffusion coefficient. The behavior of the shock wave produced at a point on thedoi:10.17706/ijapm.2015.5.1.8-17 fatcat:4lwr65dhxvbexnlejsanbxbdzq