A Two-Fluid Simulation of Tailings Dam Breaching

Author(s):  
Gregor Petkovšek ◽  
Mohamed Ahmed Ali Mohamed Hassan ◽  
Darren Lumbroso ◽  
Marta Roca Collell
Particuology ◽  
2018 ◽  
Vol 38 ◽  
pp. 165-173 ◽  
Author(s):  
Atta Ullah ◽  
Iqra Jamil ◽  
Adnan Hamid ◽  
Kun Hong

2019 ◽  
Vol 2019 ◽  
pp. 1-10 ◽  
Author(s):  
Zhao Deng ◽  
Shiqiang Wu ◽  
Ziwu Fan ◽  
Zhikun Yan ◽  
Jingxiu Wu

The centrifugal model test system is utilized to reappear the breaching process of a tailings dam. The results show that there are significant differences in breaching processes between tailings dams and earth-rockfill dams. Influenced by the special physical and mechanical properties of tailings, the breaching processes of tailings dams are of short duration, and the flood flow through the breach increase rapidly. Based on the centrifugal test results, considering the special physical and mechanical properties of tailings, a mathematical model for tailings dam breaching is established. In the model, the vertical undercutting and horizontal expansion are simulated utilizing the erosion rate formula which is derived from shear stress principle of water flow; limit equilibrium method is used to analyze the breach slope stability. In addition, the model adopts iterative calculation method to simulate the whole breaching process. The analysis results show that, the proposed model is applicable in modeling the dam breaching process for tailings dam due to overtopping.


Energy ◽  
2021 ◽  
Vol 216 ◽  
pp. 119257
Author(s):  
Zihong Xia ◽  
Jisheng Long ◽  
Shuai Yan ◽  
Li Bai ◽  
Hailiang Du ◽  
...  

Fluids ◽  
2019 ◽  
Vol 4 (4) ◽  
pp. 189 ◽  
Author(s):  
Francesco Palermo

By means of the formation of vortices in the nonlinear phase, the Kelvin Helmholtz instability is able to redistribute the flux of energy of the solar wind that flows parallel to the magnetopause. The energy transport associated with the Kelvin Helmholtz instability contributes significantly to the magnetosphere and magnetosheath dynamics, in particular at the flanks of the magnetopause where the presence of a magnetic field perpendicular to the velocity flow does not inhibit the instability development. By means of a 2D two-fluid simulation code, the behavior of the Kelvin Helmholtz instability is investigated in the presence of typical conditions observed at the magnetopause. In particular, the energy penetration in the magnetosphere is studied as a function of an important parameter such as the solar wind velocity. The influence of the density jump at the magnetopause is also discussed.


2006 ◽  
Vol 167 (1) ◽  
pp. 26-32 ◽  
Author(s):  
Christian Costa Milioli ◽  
Fernando Eduardo Milioli

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