Flow around a ship-hull

 

Surface model for a RANSE computation of a propeller behind a ship hull

 
 
Introduction

 

The HSVA test case involves the flow around the submerged hull of a single-propeller ship. Initially, the ship model is tested without the propeller, during which many aspects of the hull performance are measured.


One such aspect is the flow through the propeller plane. The propeller is located behind the ship hull and hence it rotates in water that has been already disturbed by the passage of the hull. The velocity in the wake of the ship is not uniform but changes with radial and angular positions of the propeller. The wake velocity consists of axial, radial, tangential components.


The propeller rotates at a constant speed, and the blades are fixed-pitch propellers. Through a single revolution, the blades pass through regions of differing flow velocities. This results in varying angles of attack for any given propeller section, and consequently, a cyclic, oscillating propeller thrust is generated. Minimizing this oscillation is critical. Vibration and noise can be intolerable to crew and passengers. They may also reduce propulsion efficiency, leading to higher fuel costs, or even cause structural damage to the ship in extreme cases.


HSVA performs both numerical computations and model testing to measure this flow disruption. These measurements serve as a baseline, against which the effects of a propeller are compared. The results can be used to verify a propeller performance, and to indicate areas of improvement during the design phase. For the computations, it is of importance to the HSVA and the client to obtain these results quickly, accurately, and reliably.


FlowGrid will be tested not only to verify and benchmark against currently used methods, but also demonstrate its use with extreme computing methods. In this test case, two methods for computation will be computed and evaluated. The first method, using wall functions, is the commonly used computational method at the HSVA. It uses a moderately sized grid, and provides acceptable results in a short computing time. FlowGrid is to be used to compare with experimental model measurements and other CFD software for wall function computing method. The second, a non-wall function computing method, provides higher accuracy compared to the more commonly used method. However, due to the large grid and long computing times necessary, it is not practical to use this computing method with conventional computing software and hardware configurations. FlowGrid will demonstrate its superiority for the application of this more complex, unconventional computing method.

 
 
Detailed descriptions

 

The computations are based on the Napa geometry description of the model (HSVA model-2962) for the containership “Sydney Express”. An experimental model was constructed according to this geometry description. From the Napa description, an IGES file was generated, to be used as the basis for grid generation using the commercial grid generation software ICEM-CFD. The ship profile is shown in the figure below.

.

Profile view of “Sidney Express”


The ship is symmetrically shaped, and uses a single propeller for propulsion. The test case simulates full ahead travel, thus the flow is parallel to the ship’s length. Under these conditions, it is only necessary to compute one half of the ship, with the plane of symmetry along the longitudinal centerline of the ship. The actual ship is 210.00 meters long, but the computational grid was scaled to match the 7.50 meter length of the experimental model, in order to conduct a direct comparison with experiment measurements. The table below gives the main ship characteristics.

Full Scale Ship Dimensions
Lpp 210.00 Length between perpendiculars (m)
B 30.50 Breadth (m)
T 11.00 Design draught (m)
Vs 10.5 Ship speed (m/s)
Rn 1.859*109 Reynolds number based on Lpp and Vs
Fn 0.231 Froude number based on Lpp and Vs
 
Model measurement
lambda 28.0 Model scale factor
Vm 1.97 Model speed (m/s)
Rn 1.246*107 Reynolds number based on Lm and Vm
Fn 0.230 Froude number based on Lm and Vm

 

With the model testing, similarity laws come into conflict. Reynolds scaling is based on the viscous effects, and dictates the speed of the model should increase inversely as the model size decreases. Froude scaling, however, is based on gravity effects, and dictates that the model speed should decrease as the model size decreases. In model testing, the gravity effects at the free surface are dominant, and the model speed is defined according to Froude’s Law for similarity as


.


This test case uses two frames of reference: a global frame and a propeller-based frame of reference. The global frame of reference is right-handed Cartesian coordinate system. Typical to shipbuilding practices, the origin of the global reference frame is along the longitudinal plane of symmetry at the rudder shaft centerline. The x-axis is centered at the ruder shaft centerline and points forward. From this frame of reference, the free-stream fluid flow is defined as flowing in the negative x-direction. The z-axis is centered at the baseline of the ship, pointing positive upward. By default, the y-axis points in the port direction.


The secondary frame of reference is a cylindrical coordinate system, coinciding with the rotation of the ship propeller. Most of the plots depicting computation results are in this frame of reference.



Computational domain bounding edges


The computational domain is often either cylindrical or rectangular shaped; in this test case it is cylindrical, as shown in the figure above It is important, that the side and bottom boundaries are far enough from the ship hull as to avoid shallow water and channel wall effects; ½ ship length is sufficient in this case. The inlet is at ½ ship length ahead of the ship, and the outlet is placed 1 ship length behind the ship. The top of the computational domain is at the design waterline of the ship, 0.393 meters (11.00 meters, full scale). This type of computation does not take the free surface into account, and thus the top of the computation domain is a solid surface. These are generally known as „double body“ computations. The focus of the computations is the flow through the propeller plane, as indicated in tne figure below.



Propeller plane location


Based on the ship hull geometry and the computational domain bounding surfaces, two grids were generated using ICEM-CFD. The first grid had 868,465 cells and the second had 1,302,966 cells. Mainly, the cell height in the region at and near the hull surface changed the most from the first grid to the second. The initial cell height at the hull surface in the second grid was set to 2.86*10-3 m. For the second grid, the initial cell height at the hull was reduced to 1.79*10-4 m. Subsequently, to keep the aspect ratios in these cells within reason, the cell sizes in the other two directions, i.e. tangential to the hull surface, were also reduced. Further, the cell heights in the next several surrounding layers were also reduced, to maintain smooth continuity of cell sizes. Outside a 1 meter (full scale) region, the cell spacing for both grids were very similar. A cross-sectional slice from the same location of both grids is shown in the next figure.


These two grids were generated for application of two computational methods for resolving the boundary layer at and near the hull surface. At the hull surface, a no-slip boundary condition was applied. The no-slip condition implies that the velocity of the fluid is equal to that of the adjacent solid surface. However, if the flow is turbulent and the grid elements are too coarse to resolve this large velocity variation in the region near the wall, then a special interpolation of the velocity and shear stress is necessary. This interpolation is based on so-called “wall functions”.


For finer grids, the cell height in the region near the hull is sufficiently small that wall functions are not necessary to represent the distributions of velocity, temperature, turbulence, energy, etc. within the boundary layer that forms adjacent to the hull surface. With the size of the ships computed, a grid fine enough to fulfill this criterion is impractical for computing on the current HSVA hardware/software configuration. Using FlowGrid would provide the opportunity to perform such computations effectively and competitively.


Grid comparison: wall function coarse grid, left; non-wall function fine grid, right

Description of relevant parameters to be observed

In this test case, the relevant parameters to be observed are as follows:


• Pressure along the hull surface
• Shear stress along the hull surface
• Flow velocity near the hull surface
• Flow velocity components on the propeller plane
• y+ values along the hull surface
• k and e values for the turbulence model


The pressure and shear stress are integrated along the hull surface to compute the resistance of the hull. The flow velocity near the hull surface gives an indication of where flow problems may occur. The flow velocity components- u,v,w- on the propeller plane are used extensively for propeller design and evaluation.


The y+ values provide information to whether wall functions are used or not. Comet sets a limit; for y+ <11, non-wall function method is applied, otherwise wall functions are used for resolving the boundary layer.
The turbulence values k and e affect nearly all of the parameters mentioned above.

Available experimental data

Experimental data was gathered from model tests in the HSVA’s 300 meter towing tank. The model tests used force gauges to measure the longitudinal force required to tow the model, and 5-hole pitot tubes to measure the flow velocity in the propeller plane. The pitot tubes were arranged on a small armature, spaced from 30% propeller radius to 110% propeller radius, in 10% increments. The armature could be rotated through the entire propeller revolution in 10º increments. See figure for details.

Pitot tube arrangement for measuring flow


 
 
FlowGrid evaluation

 

The HSVA has identified several comparison characteristics, with which the FlowGrid system is to be evaluated. This consists of visual comparison of the computation results, as well as numerical evaluation. The following table summarizes these characteristics and corresponding values:

Complete “turn-around” time
1-1 ½ days
Computation convergence times
1-2 hours

Global Ship hull resistance (CFD computations only)

Within 10% of Comet computations
Nominal wake fraction value
Appx. 5% of Comet and model values
Axial velocity component error
Under 10% of model values
Flow velocity distribution
Visual survey


The term “turn-around” time describes the time needed to deliver results to the customer for a given problem. This includes preparation time for the solver, as well as post-processing of the results. Since this is still the developmental phase of FlowGrid, this turn-around time is not expected to be comparable to the process currently in use at the HSVA. However, it will become an important factor, once the process has been established, and the learning curve has been passed. Currently, turn-around times in the order of 1 to 1 ½ days is acceptable for the coarse grid computation using Comet. FlowGrid should meet or exceed this once the learning curve has passed. For the finer grid computation, an acceptable turn-around time is difficulty to determine, as the Comet calculations are impractical with HSVA’s current computing power.


The computation convergence time shows how quickly the calculations can arrive at a solution. Unlike the aforementioned turn-around time, the computational convergence time is not so strongly dependent of user experience and, therefore, can be compared against the computations performed on the HSVA’s parallel cluster. The computing times for the coarse grid computation using FlowGrid should be comparable to within 1 to 2 hours, comparable to those for Comet.


The global ship hull resistance compares the representation of the no-slip boundary condition of the ship hull. It is the sum of the integrated pressure component of the ship surface and the integrated shear stress acting on the hull surface. The resulting longitudinal, x-direction, forces should be comparable to Comet computations and experimental results by 5 to 10%.

The nominal wake fraction is the average deficiency in the axial flow through the propeller plane, caused by the wake of the ship hull. This value is calculated by the integration of the normalized axial velocity component over area enclosed by the propeller-bounding circle. The equation is in the form of a summation, based on the integral:

where ux is the normalized computed axial component of velocity.
The HSVA propeller expert uses the following formula to compute the velocity axial component error,


where Vi A_measured is the measured axial component, Vi A_computed is the computed axial component, and V0 is the free stream velocity (1.97 m/s). This formula may be applied to a single radius, or to the entire set of measurement points in the propeller disk.


Other aspects for evaluation of FlowGrid performance are not specific to this test case. These are the characteristics of FlowGrid that cannot be quantified. FlowGrid should be easy to use; learning to use FlowGrid should not be laborious. The HSVA has experience with at least three other RANSE solvers, and expects similar features to be found in FlowGrid as in the other solvers. Of course, not all features can be available initially. This is not a primary concern for HSVA, as it is understood that FlowGrid will be further improved beyond this developmental stage.

 

Copyright © 2004 FlowGrid Consortium | Please send questions or comments to Norberto.Fueyo@posta.unizar.es, or to any other FlowGrid partner | Last modified on 02/04/2004