Unsteady RANS simulation of the ship forward speed diffraction problem

2006 ◽  
Vol 35 (6) ◽  
pp. 545-570 ◽  
Author(s):  
Pablo M. Carrica ◽  
Robert V. Wilson ◽  
Fred Stern
2021 ◽  
Vol 372 ◽  
pp. 110978
Author(s):  
Mubashir Hassan ◽  
Jinbiao Xiong ◽  
Xu Cheng

2016 ◽  
Vol 56 ◽  
pp. 79-91 ◽  
Author(s):  
Siamak Alimirzazadeh ◽  
Saeed Zabihzade Roshan ◽  
Mohammad Saeed Seif

2015 ◽  
Vol 117 ◽  
pp. 183-195 ◽  
Author(s):  
F. Noh-Pat ◽  
J. Xamán ◽  
G. Álvarez ◽  
M. Gijón-Rivera ◽  
I. Hernández-Pérez ◽  
...  

1998 ◽  
Vol 42 (02) ◽  
pp. 99-112 ◽  
Author(s):  
F. T. Korsmeyer ◽  
H. B. Bingham

This paper examines the theory and computational methods behind predicting the linear unsteady motion of a ship with steady forward speed in waves. The focus is on the wave exciting force impulse-response function as computed via the transient free-surface Green function. The linear equation of motion for a ship in waves was first written in a rational form, using the concept of the impulse-response function, by Cummins (1962). Some years later King et al (1988) added the corresponding wave exciting force in its appropriate convolution form. We extend this work by clarifying the definition of the impulsive incident wave in following seas, and show it to be easily computable. Continuing truncated calculations towards infinite time becomes especially important in following waves, and the method suggested by Bingham et al (1994) is employed here. A novel filtering scheme is also introduced to prevent short wave contamination of the solution. These developments allow calculations in following waves to be presented for the first time using this approach. The integral equation formulation of the linear seakeeping problem is reviewed in some detail, and the relevant equations derived. Transient Haskind relations for bodies with forward speed are also derived although, like their frequency-domain counterparts, these are only approximate. Computed, first-order exciting forces and response-amplitude operators for real ship geometries, in head and following seas, are presented that demonstrate the usefulness of the transient approach for the diffraction problem.


1985 ◽  
Vol 29 (02) ◽  
pp. 105-111
Author(s):  
P. D. Sclavounos

Expressions are derived for the heave and pitch exciting force and moment on a ship advancing in waves. They are obtained in the form of an integral over the ship axis of the outer source strength of the reverse-flow radiation problem multiplied by the value of the incident-wave velocity potential. Their performance is tested for two slender spheroids. Comparisons are made with predictions obtained from a three-dimensional numerical solution at zero speed—the expression common to strip-theory programs which uses the ship hull as the integration surface—and the direct solution of the diffraction problem.


Author(s):  
Takashi Yamane ◽  
Yuhi Tanaka

The conjugate heat transfer simulation is expected to simulate precise temperature distributions of turbine cooling structures and contribute to the reduction of cooling air usage. This method has mainly been used to predict steady state temperature because of the large difference of time scale between RANS flow simulation and thermal conduction in solid materials, thus the accuracy of temperature estimation depends on the modeling of the turbulence. Despite many efforts to improve turbulence models, an inherent limitation of RANS and turbulence modeling and the necessity of unsteady simulation for better accuracy in heat transfer simulations have been pointed out. The aim of this study is to combine the unsteady RANS simulation with the steady thermal conduction of solid materials. The “Time Smoothing” method was introduced to compensate the large time scale difference between fluid and solid, then the effectiveness of the method was confirmed through conjugate heat transfer simulations around a pipe shape object where strong flow unsteadiness prevails.


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