Phase and Microstructure Selection During Directional Solidification of Peritectic Alloy Under Convection Condition

2014 ◽  
Vol 27 (4) ◽  
pp. 585-592 ◽  
Author(s):  
Lingshui Wang ◽  
Jun Shen ◽  
Yilong Xiong ◽  
Yujun Du ◽  
Hengzhi Fu
2013 ◽  
Vol 112 (2) ◽  
pp. 363-370 ◽  
Author(s):  
Lei Wang ◽  
Jun Shen ◽  
Xiao Yin ◽  
Yujun Du ◽  
Yilong Xiong ◽  
...  

2016 ◽  
Vol 6 (1) ◽  
Author(s):  
Peng Peng ◽  
Xinzhong Li ◽  
Jiangong Li ◽  
Yanqing Su ◽  
Jingjie Guo ◽  
...  

2009 ◽  
Vol 79-82 ◽  
pp. 1655-1658
Author(s):  
Yan Qing Su ◽  
Dong Mei Liu ◽  
Xin Zhong Li ◽  
Liang Shun Luo ◽  
Jing Jie Guo ◽  
...  

Microstructure evolution of peritectic Al-25at.%Ni alloy during directional solidification with pulling velocity ranging from 2 to 500m/s is investigated. The directional solidified alloy is composed of Al3Ni2, Al3Ni phase and eutectic (Al3Ni+Al) phase. When pulling velocity ranges from 2 to 5m/s, Al3Ni phase grows into an integral matrix. Majority of primary Al3Ni2 is consumed by peritecti reaction and transformation behind the peritectic interface with pulling velocity ranging from 2 to 20 m/s. While pulling rate increases, major Al3Ni phase direct solidifies from liquid. With cooling rate increasing, Al3Ni2 phase content firstly decreases and then increases, while the Al3Ni phase content decreases throughout.


Rare Metals ◽  
2011 ◽  
Vol 30 (4) ◽  
pp. 424-431 ◽  
Author(s):  
Xiaowu Hu ◽  
Hong Yan ◽  
Wenjing Chen ◽  
Shuangming Li ◽  
Hengzhi Fu

2010 ◽  
Vol 312 (16-17) ◽  
pp. 2441-2448 ◽  
Author(s):  
Yanqing Su ◽  
Dongmei Liu ◽  
Xinzhong Li ◽  
Liangshu Luo ◽  
Jingjie Guo ◽  
...  

Author(s):  
H.J. Zuo ◽  
M.W. Price ◽  
R.D. Griffin ◽  
R.A. Andrews ◽  
G.M. Janowski

The II-VI semiconducting alloys, such as mercury zinc telluride (MZT), have become the materials of choice for numerous infrared detection applications. However, compositional inhomogeneities and crystallographic imperfections adversly affect the performance of MZT infrared detectors. One source of imperfections in MZT is gravity-induced convection during directional solidification. Crystal growth experiments conducted in space should minimize gravity-induced convection and thereby the density of related crystallographic defects. The limited amount of time available during Space Shuttle experiments and the need for a sample of uniform composition requires the elimination of the initial composition transient which occurs in directionally solidified alloys. One method of eluding this initial transient involves directionally solidifying a portion of the sample and then quenching the remainder prior to the space experiment. During the space experiment, the MZT sample is back-melted to exactly the point at which directional solidification was stopped on earth. The directional solidification process then continues.


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