  The structure of the cosmic ray electron halo of a starburst galaxy depends
strongly on the nature of galactic wind and the configuration of the magnetic
field. We have investigated these dependencies by solving numerically the
propagation of electrons originating in starburst galaxies, most likely in
supernova remnants. The calculations are made for several models for the
galactic winds and for the configuration of the magnetic fields for comparison
with observations. Our simulation of a quasi-radio halo reproduces both the
extended structure of ~ 9 kpc and the subtle hollow structure near the polar
region of the radio halo that are observed in the starburst galaxy NGC 253.
These findings suggest the existence of strong galactic wind in NGC 253.
