Special attention in the role of convection in vapor crystal growth has been paid since some single crystals under high gravity acceleration of 10g 0 appear considerably larger than those under normal gravity acceleration (1g 0 ). With increasing the gravity acceleration from 1g 0 up to 10g 0 , the total molar flux for ∆T = 30 K increases by a factor of 4, while for ∆T = 90, by a factor of 3. The maximum molar fluxes for three different gravity levels of 1g 0 , 4g 0 and 10g 0 , 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 1g 0 up to 10g 0 , the intensity of convection is increased significantly through the maximum molar fluxes for ∆T = 30 K and 90 K. At 10g 0 , the maximum total molar flux is nearly invariant for for ∆T = 30 K and 90 K. The total molar flux increases with increasing the gravity acceleration, for 1g 0 ≤ g y ≤ 10g 0 , and decreases with increasing the partial pressure of component B, a noble gas called as Kr (Krypton), P B . The |U| max is directly proportional to the gravity acceleration for 20 Torr P B ≤ 300 Torr. As the partial pressure of P B (Torr) decreases from 300 Torr to 20 Torr, the slopes of the |U| max s 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 Hg 2 Cl 2 is first order exponentially decayed with increasing the partial pressure of component B, P B (Torr) from 20 Torr up to 300 Torr.