  Nuclear transparency is calculated for high-energy, semi-inclusive $(e,e'p)$
reactions, by accounting for all orders of Glauber multiple-scattering and by
using realistic finite-range $p N$ interaction and (dynamically and
statistically) correlated nuclear wave functions. The nuclear correlation
effect is reduced due to the $p N$ finite-range effect. The net effect is
small, and depends sensitively on details of the nuclear correlations in finite
nuclei, which are poorly known at present.
