Understanding the effect of turbulent magnetic fluctuations on the transport of energetic particles is a fundamental, still unanswered problem in astrophysics. In this paper we present a novel framework aimed at the study of cosmic rays transport and diffusion on the basis of test particle simulation in synthetic turbulent realizations. In particular, we make use of the BxC toolkit, integrating its output within the MPI-AMRVAC framework. We show that the two codes are successfully interfaced, paving the way for an extensive parameter study that could give insight into the role of turbulence in particle diffusion and scattering.