The spatial resolution of three-dimensional atom probe is known to be mainl
y controlled by the aberrations of ion trajectories near the specimen surfa
ce. An analytical model accounting for the spatial overlaps that occur near
phase interfaces is described. This model makes it possible to correct the
apparent composition of small spherical precipitates in order to determine
the true composition. The prediction of the overlap rate as a function of
the particle size was found in remarkably good agreement with the simulatio
ns of ion trajectories that were made. The thickness of the mixed zone arou
nd beta precipitates was found to be of 0.3 nm for a normalised evaporation
field of beta phase of 0.8. Using simulations, the overlap rate could be p
arameterised as a function of the apparent atomic density observed in parti
cles. This model has been applied to copper precipitation in FeCu. (C) 2001
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