  We report the discovery of two isolated radio pulsars having the largest
inferred surface dipole magnetic fields yet seen in the population: 4.1e10^13 G
and 5.5e10^13 G. These pulsars show apparently normal radio emission in a
regime of magnetic field strength where some models predict no emission should
occur. They have spin parameters and magnetic fields similar to those of some
magnetar candidates, but exhibit very different radiative properties. This
demonstrates that if the putative magnetars are indeed isolated neutron stars,
their unusual attributes cannot be only a consequence of their large inferred
magnetic fields.
