Three of the four CdZnTe crystals grown on USML-1 and 2 have been analyzed with respect to hydrostatic and buoyant gravitational influences. Characterization was carried out using Synchrotron White Beam X-ray Topography, Fourier Transfer Infrared (FTIR) Spectroscopy and chemical etching. It was found that in the absence of hydrostatic pressure the liquid separated from the ampoule walls, depending on influences such as: volumetric fill-factor, level of constraint, residual g-vector, ampoule geometry and growth conditions. Regions solidified without wall contact were found to be virtually free from twinning, suggesting that these pervasive defects are surface nucleated. Further, these regions showed dramatic reductions in the density of dislocations, from 800,000 (l-g) to 800 (μ-g). This was attributed to thermo-mechanical stress reduction within the flight samples. Regions of partial wall contact showed defect gradients, high on the wall side and low on the free surface side. These results are consistent with our thermo and thermo-mechanical stress model.
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