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Effect of accelerational perturbations on physical vapor transport crystal growth under microgravity environments
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  • Effect of accelerational perturbations on physical vapor transport crystal growth under microgravity environments
  • Effect of accelerational perturbations on physical vapor transport crystal growth under microgravity environments
저자명
Choi. Jeong-Gil,Lee. Kyong-Hwan,Kwon. Moo-Hyun,Kim. Geug-Tae
간행물명
한국결정성장학회지
권/호정보
2006년|16권 5호|pp.203-209 (7 pages)
발행정보
한국결정성장학회
파일정보
정기간행물|ENG|
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이 논문은 한국과학기술정보연구원과 논문 연계를 통해 무료로 제공되는 원문입니다.
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기타언어초록

For $P_B=50,;{Delta}T=10K$, Ar=5, Pr=2.36, Le=0.015, Pe=1.26, Cv=1.11, the intensity of solutal convection (solutal Grashof number $Grs=3.44x10^4$) is greater than that of thermal convection (thermal Grashof number $Grt=1.81x10^3$) by one order of magnitude, which is based on the solutally buoyancy-driven convection due to the disparity in the molecular weights of the component A($Hg_2Cl_2$) and B(He). With increasing the partial pressure of component B from 10 up to 200 Torr, the rate is decreased exponentially. The convective transport decreases with lower g level and is changed to the diffusive mode at 0.1 $g_0$. In other words, for regions in which the g level is 0.1 $g_0$ or less, the diffusion-driven convection results in a parabolic velocity profile and a recirculating cell is not likely to occur. Therefore a gravitational acceleration level of less than 0.1 $g_0$ can be adequate to ensure purely diffusive transport.