Ultra High Energy Cosmic Rays, propagation in the Galaxy and anisotropy

We considered propagation of Ultra High Energy Cosmic Rays (UHECR) through the galaxy. We extend our numerical code for calculation of the spectra of leptons, nucleons and $\gamma$-rays in case of uniform and isotropic source distribution for the case of spherically symmetric source distribution and magnetic field. We investigated models with sources of UHECR distributed in same way as Cold Dark Matter (CDM) in self-consistent way, taking into account both extra-galactic and Galactic contributions