In order to simulate the space environment for basic research into the crystal growth mechanism, Hgo.sCdo.2Te crystals were grown by the vertical Bridgman-Stockbarger method in the presence of an applied axial magnetic field. The influence of convection, by magneto hydrodynamic damping, on mass transfer in the melt and segregation at the solid-liquid interface was investigated by measuring the axial and radial compositional variations in the grown samples.The reduction of convective mixing in the melt through the application of the magnetic field is found to have a large effect on radial segregation and interface morphology in the grown crystals. Direct comparisons are made with a Hgo.sCdo.2Te crystal grown without field and also in the microgravity environment of space during the second United States Microgravity Payload Mission (USMP-2).