The work reported here represents significant advancement in the modeling o
f grain structure evolution in metallic systems. Utilizing computed tempera
ture fields from a well tested heat transfer and fluid flow model, the evol
ution of grain structure was simulated for the first time using a three dim
ensional (3D) Monte Carlo model of grain growth in the heat affected zone o
f commercially pure titanium welds. The computed weld geometry and the simu
lated mean prior beta grain size for different heat inputs;agreed well with
the corresponding experimental results when turbulence in the weld pool wa
s considered. The grain sizes at Various locations equidistant from the fus
ion line were different, indicating that the results of previous 2D calcula
tions need to be reexamined. The computed grain size distribution agreed we
ll with the corresponding experimental data. The agreement indicates signif
icant promise for understanding grain growth in the entire heat-affected zo
ne using a comprehensive phenomenological model. (C) 2000 Acta Metallurgica
Inc. Published by Elsevier Science Ltd. AII rights reserved.