  The chiral magnetic wave from the interplay between the chiral magnetic
effect and the chiral separation effect is simulated in a box system with the
periodic boundary condition based on the chiral kinetic equations of motion.
Simulation results are compared with available limits from theoretical
derivations, and effects of the temperature, the magnetic field, and the
specific shear viscosity on the key properties of the chiral magnetic wave are
discussed. Our study serves as a baseline for further simulations of chiral
anomalies in relativistic heavy-ion collisions.
