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Phase Field Modeling of Columnar Grain Growth:Effect of Second-Phase Particles
LUO Zhirong, GAO Yingjun, MAO Hong, LU Chengjian, HUANG Shiye
CHINESE JOURNAL OF COMPUTATIONAL PHYSICS    2016, 33 (3): 367-373.  
Abstract392)   HTML5)    PDF (2450KB)(934)      
In a moving hot zone model with uniform temperature and an infinite temperature gradient under directional annealing, effect of second-phase particles (SPPs) on growth of columnar grain microstructure in polycrystalline materials was studied with phase field method. It shows that SPPs inhibit formation of columnar grain structure and inhibitory effect increases with increasing volume fraction of SPPs and decreasing size of SPPs. Effect of SPPs on final grain radius follows Zener relation under condition of directional annealing. Volume fraction of SPPs and their dispersive distribution at grain boundaries in materials should be reduced as far as possible to obtain better columnar grain structures during directional annealing.
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THE THEORETICAL SIMULATION AND COMPUTER SOFTWARE OF INFRARED RADIATION FIELDS OF TARGETS ON THE SEA
YANG Bao-cheng, SHEN Guo-tu, MAO Hong-xia, GAO Lan-xiang, HONG Zhen-qing, ZHU Wen-yong, GAO Jing
CHINESE JOURNAL OF COMPUTATIONAL PHYSICS    2001, 18 (3): 219-224.  
Abstract283)      PDF (234KB)(947)      
A theoretical model of the temperature field and infrared radiation field is presented,the physical characteristic of which is the separate treatment of the three wavelength regions of the radiation of the sun,the sea and atmosphere background,and the target,and based on the model the complete set of equations of the temperature field and radiation field for the ship in question are obtained that are then used to developed a computer software to obtain the field distribution and to simulate the thermal images of the target.The flow chart of the software is presented and key points concerning the programming are discussed.The numerical results and the simulated graphs for the infrared images of a ship are calculated using the software.The results are compared with the real infrared images of the ship and the main features of the two results are in good agreement.
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