scholarly journals Interaction between high-velocity gas and liquid in gas atomization revealed by a new coupled simulation model

2021 ◽  
pp. 110264
Author(s):  
Sheng Luo ◽  
Hongze Wang ◽  
Zhenyang Gao ◽  
Yi Wu ◽  
Haowei Wang
1999 ◽  
Vol 81 (1-3) ◽  
pp. 249-259
Author(s):  
Kenji Takagi ◽  
Motohiko Yamada ◽  
Yasushi Uematsu

2014 ◽  
Vol 960-961 ◽  
pp. 1442-1445
Author(s):  
Hui Meng ◽  
Zhi Tao Wang ◽  
Shu Ying Li ◽  
Ning Bo Zhao ◽  
Gang Jin

This paper establishes the COGAG system simulation model in the environment of SIMULINK and ADAMS with the method of coupled simulation based on multiple simulation platforms; simulates and analyses the COGAG engaging process with the simulation model. Dynamic change rules of some key parameters such as speed, moment, power are obtained and analysed detailed, which plays an important role in development and application of COGAG device.


2019 ◽  
Vol 66 ◽  
pp. 293-305 ◽  
Author(s):  
Hongyan Qu ◽  
Yan Peng ◽  
Zhejun Pan ◽  
Zhangxin Chen ◽  
Fujian Zhou ◽  
...  

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


1967 ◽  
Vol 31 ◽  
pp. 117-119
Author(s):  
F. D. Kahn ◽  
L. Woltjer

The efficiency of the transfer of energy from supernovae into interstellar cloud motions is investigated. A lower limit of about 0·002 is obtained, but values near 0·01 are more likely. Taking all uncertainties in the theory and observations into account, the energy per supernova, in the form of relativistic particles or high-velocity matter, needed to maintain the random motions in the interstellar gas is estimated as 1051·4±1ergs.


Author(s):  
S. Wisutmethangoon ◽  
T. F. Kelly ◽  
J.E. Flinn

Vacancies are introduced into the crystal phase during quenching of rapid solidified materials. Cavity formation occurs because of the coalescence of the vacancies into a cluster. However, because of the high mobility of vacancies at high temperature, most of them will diffuse back into the liquid phase, and some will be lost to defects such as dislocations. Oxygen is known to stabilize cavities by decreasing the surface energy through a chemisorption process. These stabilized cavities, furthermore, act as effective nucleation sites for precipitates to form during aging. Four different types of powders with different oxygen contents were prepared by gas atomization processing. The atomized powders were then consolidated by hot extrusion at 900 °C with an extrusion ratio 10,5:1. After consolidation, specimens were heat treated at 1000 °C for 1 hr followed by water quenching. Finally, the specimens were aged at 600 °C for about 800 hrs. TEM samples were prepared from the gripends of tensile specimens of both unaged and aged alloys.


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