  We predict energy spectra and angular distributions of nucleons above
10**(19) eV that originate from sources distributed in the Local Supercluster,
which is also supposed to contain a large scale magnetic field of strength
between 0.05 and 0.5 micro Gauss. We show that this model can explain all
present-day features of ultra-high energy cosmic rays, at least for field
strengths close to 0.5 micro Gauss. The large-scale anisotropy and the
clustering predicted by this scenario will allow strong discrimination against
other models with next generation experiments.
