The influence of weak convection, caused by surface tension forces, on radi
al dopant segregation occurring in crystals grown under microgravity condit
ions is studied numerically. The geometry considered corresponds to a float
ing-zone configuration with partially coated melt surfaces consisting of sm
all evenly distributed spots of free surfaces. In order to distinguish dopa
nt distribution due to weak convection clearly from distribution due to dif
fusion the spots only cover one quarter of the periphery. Thus, surface ten
sion-driven convection is allowed only over one quarter of the floating-zon
e configuration resulting in an asymmetric dopant distribution. The percent
age of free surfaces present is varied in order to alter the Marangoni flow
rates. The maximum dopant concentration due to radial segregation is plott
ed as a function of a certain convection level. The results of the present
numerical study are supposed to be used to design corresponding space exper
iments launched at the end of the year 2000. (C) 2000 Elsevier Science B.V.
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