disk shear
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2020 ◽  
Vol 85 (768) ◽  
pp. 251-261
Author(s):  
Yutaro ISHIDA ◽  
Hiroyasu SAKATA ◽  
Yuya TAKASE ◽  
Yusuke MAIDA ◽  
Takumi SATO ◽  
...  

2015 ◽  
Vol 80 (708) ◽  
pp. 297-307
Author(s):  
Yuya TAKASE ◽  
Takahide ABE ◽  
Takashi SATOH ◽  
Atsuyoshi ONAKA ◽  
Takaaki IKEDA
Keyword(s):  

2014 ◽  
Vol 79 (698) ◽  
pp. 507-515 ◽  
Author(s):  
Yuya TAKASE ◽  
Takahide ABE ◽  
Hidehiko ITADANI ◽  
Takashi SATOH ◽  
Atsuyoshi ONAKA ◽  
...  

2011 ◽  
Vol 422 ◽  
pp. 836-841
Author(s):  
Xian Jia ◽  
Qing Wang ◽  
Zhi Quan Huang ◽  
Qing Xue Huang

In this paper the main factors of impacting the quality in cutting the plate between the Shear blade clearance adjustment and control were analyzed, Focused on further analyzing all relevant factors on adjusting the Shear blade clearance , combined with the accumulated process parameters in production of one certain Thick Steel Plate Plant . Proposed for the first time the mathematical models of the best adjusting of Shear blade clearance of disk shear in cutting plate,and also make a imitate testing of finite element.


2010 ◽  
Vol 145 ◽  
pp. 26-30 ◽  
Author(s):  
Zhi Quan Huang ◽  
Qing Xue Huang

In this paper the main factors of impacting the quality in cutting the plate between the Shear blade clearance adjustment and control were analyzed, Focused on further analyzing all relevant factors on adjusting the Shear blade clearance , combined with the accumulated process parameters in production of Thick Steel Plate Plant of He Bei Wen Feng Iron and Steel Co., Ltd. Proposed for the first time the mathematical models of the best adjusting of Shear blade clearance of disk shear in cutting plate.


1995 ◽  
Vol 12 (2) ◽  
pp. 159-164 ◽  
Author(s):  
John F. Hawley ◽  
Steven A. Balbus

AbstractA long-standing problem in the theory of astrophysical accretion disks has been to determine the nature of the stress that transports orbital angular momentum outward. The discovery of a local MHD instability is strong evidence that transport occurs through turbulent Maxwell and Reynolds stresses. Using numerical simulations, we have demonstrated that a weak seed magnetic field in an accretion disk shear flow is unstable and leads to sustained MHD turbulence at dynamically important levels.


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