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Observations of the interplanetary shock provide us with strong evidence ofparticle acceleration to multi-MeV energies, even up to GeV energy, in a solarflare or coronal mass ejection (CME). Diffusive shock acceleration is anefficient mechanism for particle acceleration. For investigating the shockstructure, the energy injection and energy spectrum of a CME-driven shock, weperform dynamical Monte Carlo simulation of the 14-Dec-2006 CME-driven shockusing an anisotropic scattering law. The simulated results of the shock finestructure, particle injection, and energy spectrum are presented. We find thatour simulation results give a good fit to the observations from multiplespacecraft.

A CME-driven shock analysis of the 14-Dec-2006 SEP event