The Monte Carlo method was used to simulate particle segregation in gr
avitational fields. Systems containing one or two types of spherical p
articles were simulated, assuming that the particles interact accordin
g to a quasi-hard core potential. Systems with 1000 particles were sim
ulated, replicated by periodical boundary conditions in the directions
perpendicular to the gravitational field; at the top and bottom of th
e simulation box, the existence of rigid walls was assumed. Results fo
r local composition and local voidage as a function of the height of t
he solid sediment are presented. The results for binary systems show t
hat when very light particles are present in the mixture, it is possib
le, under certain conditions, to obtain configurations in which the pa
rticles with the smallest diameter concentrate at the top of the solid
sediment. In order to observe the three-dimensional system configurat
ions that result from the simulations, computational programs were dev
eloped in the virtual reality modeling language (VRML). (C) 1998 Elsev
ier Science S.A. AII rights reserved.