The purpose of this paper is to analyse the crystal growth experiments perf
ormed under microgravity conditions in order to learn, with the help of the
existing theory, the degree to which residual convective level acts on che
mical segregation. A survey of the existing bibliography on chemical segreg
ation in crystal growth experiments in space is performed and the results a
re analysed with the help of the existing order of magnitude analysis. It a
ppears that useful data is restricted to the axial segregation in the cryst
als and that little attention has been paid to quantitative analysis of rad
ial or micro segregation under controlled growth conditions.
Restricting the analysis to the axial segregation results, they show a good
agreement with the theoretical prediction of the threshold between diffusi
on and convection dominated transport in the liquid. From the convection do
minated experiments, generally obtained onboard the space shuttle, it appea
rs that the effective gravity level acting on the fluid was or the order of
10(-5)g(0).
Considering this validation of the theoretical results, it is concluded tha
t the experimental parameters to apply in order to get diffusive transport
conditions during crystal growth from the melt in space can now be easily a
nd reliably computed. (C) 2000 Elsevier Science Ltd. All rights reserved.