  Recent studies have shown that the anisotropy is of great value to decipher
cosmic rays' origin and propagation. We have built an unified scenario to
describe the observations of the energy spectra and the large-scale anisotropy
and called attention to their synchronously evolution with energy. In this
work, the impact of of the local regular magnetic field (LRMF) and
corresponding anisotropic diffusion on large-scale anisotropy have been
investigated. When the perpendicular diffusion coefficient is much smaller than
the parallel one, the dipole anisotropy points to the LRMF and the
observational phase below $100$ TeV could be reproduced. Moreover we find that
the dipole phase above $100$ TeV strongly depends on the evolution of local
diffusion. But the current measurements at that energy are still scarce. We
suggest that more precise measurements at that energy could be carried out to
unveil the local diffusion and further the local turbulence.
