scholarly journals Controlling the Dynamics of Cloud Cavitation Bubbles through Acoustic Feedback

2021 ◽  
Vol 15 (3) ◽  
Author(s):  
Kazuki Maeda ◽  
Adam D. Maxwell
1999 ◽  
Vol 121 (4) ◽  
pp. 872-880 ◽  
Author(s):  
Yi-Chun Wang ◽  
Christopher E. Brennen

The nonlinear dynamics of a spherical cloud of cavitation bubbles have been simulated numerically in order to learn more about the physical phenomena occurring in cloud cavitation. A finite cloud of nuclei is subject to a decrease in the ambient pressure which causes the cloud to cavitate. A subsequent pressure recovery then causes the cloud to collapse. This is typical of the transient behavior exhibited by a bubble cloud as it passes a body or the blade of a ship propeller. The simulations employ the fully nonlinear continuum bubbly mixture equations coupled with the Rayleigh-Plesset equation for the dynamics of bubbles. A Lagrangian integral method is developed to solve this set of equations. It was found that, with strong bubble interaction effects, the collapse of the cloud is accompanied by the formation of an inward propagating bubbly shock wave. A large pressure pulse is produced when this shock passes the bubbles and causes them to collapse. The focusing of the shock at the center of the cloud produces a very large pressure pulse which radiates a substantial impulse to the far field and provides an explanation for the severe noise and damage potential in cloud cavitation.


2021 ◽  
pp. 101194
Author(s):  
Masataka Ijiri ◽  
Koji Yamaguchi ◽  
Shoichi Kikuchi ◽  
Fumihiro Kato ◽  
Yui Kunieda ◽  
...  

2021 ◽  
Vol 9 (7) ◽  
pp. 742
Author(s):  
Minsheng Zhao ◽  
Decheng Wan ◽  
Yangyang Gao

The present work focuses on the comparison of the numerical simulation of sheet/cloud cavitation with the Reynolds Average Navier-Stokes and Large Eddy Simulation(RANS and LES) methods around NACA0012 hydrofoil in water flow. Three kinds of turbulence models—SST k-ω, modified SST k-ω, and Smagorinsky’s model—were used in this paper. The unstable sheet cavity and periodic shedding of the sheet/cloud cavitation were predicted, and the simulation results, namelycavitation shape, shedding frequency, and the lift and the drag coefficients of those three turbulence models, were analyzed and compared with each other. The numerical results above were basically in accordance with experimental ones. It was found that the modified SST k-ω and Smagorinsky turbulence models performed better in the aspects of cavitation shape, shedding frequency, and capturing the unsteady cavitation vortex cluster in the developing and shedding period of the cavitation at the cavitation number σ = 0.8. At a small angle of attack, the modified SST k-ω model was more accurate and practical than the other two models. However, at a large angle of attack, the Smagorinsky model of the LES method was able to give specific information in the cavitation flow field, which RANS method could not give. Further study showed that the vortex structure of the wing is the main cause of cavitation shedding.


2021 ◽  
Vol 913 ◽  
Author(s):  
Peng Xu ◽  
Shuhong Liu ◽  
Zhigang Zuo ◽  
Zhao Pan

Abstract


2018 ◽  
Vol 3 (10) ◽  
Author(s):  
Outi Supponen ◽  
Danail Obreschkow ◽  
Mohamed Farhat
Keyword(s):  

2014 ◽  
Vol 184 (9) ◽  
pp. 947-960 ◽  
Author(s):  
Robert I. Nigmatulin ◽  
R.T. Lahey ◽  
R.T. Taleyarkhan ◽  
C. West ◽  
R.C. Block
Keyword(s):  

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