Special attention in the role of convection in vapor crystal growth has been paid since some single crystals under high gravity acceleration of <TEX>$10g_0$</TEX> appear considerably larger than those under normal gravity acceleration (<TEX>$1g_0$</TEX>). With increasing the gravity acceleration from <TEX>$1g_0$</TEX> up to <TEX>$10g_0$</TEX>, the total molar flux for <TEX>${\Delta}T$</TEX> = 30 K increases by a factor of 4, while for <TEX>${\Delta}T$</TEX> = 90, by a factor of 3. The maximum molar fluxes for three different gravity levels of <TEX>$1g_0$</TEX>, <TEX>$4g_0$</TEX> and <TEX>$10g_0$</TEX>, appear approximately in the neighborhood of y = 0.5 cm, and the molar fluxes show asymmetrical patterns, which indicate the occurrence of either one single or more than one convective cell. As the gravitational level is enhanced form <TEX>$1g_0$</TEX> up to <TEX>$10g_0$</TEX>, the intensity of convection is increased significantly through the maximum molar fluxes for <TEX>${\Delta}T$</TEX> = 30 K and 90 K. At <TEX>$10g_0$</TEX>, the maximum total molar flux is nearly invariant for for <TEX>${\Delta}T$</TEX> = 30 K and 90 K. The total molar flux increases with increasing the gravity acceleration, for <TEX>$1g_0{\leq}g_y{\leq}10g_0$</TEX>, and decreases with increasing the partial pressure of component B, a noble gas called as Kr (Krypton), <TEX>$P_B$</TEX>. The <TEX>${{\mid}U{\mid}}_{max}$</TEX> is directly proportional to the gravity acceleration for 20 Torr <TEX>$P_B{\leq}300$</TEX> Torr. As the partial pressure of <TEX>$P_B$</TEX> (Torr) decreases from 300 Torr to 20 Torr, the slopes of the <TEX>${{\mid}U{\mid}}_{max}s$</TEX> versus the gravity accelerations increase from 0.29 sec to 0.54 sec, i.e. by a factor of 2. The total molar flux of <TEX>$Hg_2Cl_2$</TEX> is first order exponentially decayed with increasing the partial pressure of component B, <TEX>$P_B$</TEX> (Torr) from 20 Torr up to 300 Torr.
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