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Constraining the behavior of cosmic ray data observed at Earth requires aprecise understanding of how the cosmic rays propagate in the interstellarmedium. The interstellar medium is not homogeneous; although turbulent magneticfields dominate over large scales, small coherent regions of magnetic fieldexist on scales relevant to particle propagation in the nearby Galaxy. Guidedpropagation through a coherent field is significantly different from randomparticle diffusion and could be the explanation of spatial anisotropies in theobserved cosmic rays. We present a Monte Carlo code to propagate cosmicparticle through realistic magnetic field structures. We discuss the details ofthe model as well as some preliminary studies which indicate that coherentmagnetic structures are important effects in local cosmic-ray propagation,increasing the flux of cosmic rays by over two orders of magnitude atanisotropic locations on the sky. The features induced by coherent magneticstructure could be the cause of the observed TeV cosmic-ray anisotropy.

Explaining TeV Cosmic-Ray Anisotropies with Non-Diffusive Cosmic-Ray Propagation