  Recent nucleosynthesis calculations of Type II supernovae using advanced
neutrino transport determine that the early neutrino winds are proton-rich.
However, a fraction of the ejecta emitted at the same time is composed of
neutron-rich pockets. In this paper we calculate the nucleosynthesis
contribution from the neutron-rich pockets in the hot convective bubbles of a
core-collapse supernova and show that they do not contribute significantly to
the total nucleosynthesis.
