The widely accepted models for late stage clustering, the Lifshitz-Sly
ozov-Wagner theory for Ostwald ripening and the self-similar Monte Car
lo simulations by Family and Meakin for coalescence growth, are consis
tent with random spatial distributions of the clustered phase. Several
detailed investigations have revealed that cluster-cluster interactio
ns have to be further considered. Only one of these studies lead to pr
edictions of spatial ordering when long-range repulsive forces were in
cluded. In this paper we investigate nearest neighbor cluster distance
distributions for both late stage growth processes (coalescence for G
a on GaAs(001) and Ostwald ripening for Sn and In on SI(111)) and corr
elate the results with experimental and theoretical results for the cl
uster-cluster interaction in these systems. Non-random spatial distrib
utions are found for ripening even at rather low areal cluster densiti
es, indicating that (i) cluster-cluster interactions play a major role
in the morphological evolution of ripening structures at much smaller
areal fractions than previously assumed and (ii) the Gibbs-Thomson ef
fect, in combination with a diffusion controlled exchange of matter be
tween clusters, is sufficient as a driving force to obtain partially o
rdered structures.