2.1. CFD Numerical Setup for RDT Simulation
Numerical simulations based on the RANS method are carried out to investigate the viscous flow fields of a 30 kW rim-driven thruster under two operating conditions: open water and behind-hull wake. Since the temperature variation in underwater flow is negligible and heat exchange can be ignored, the continuity equation and Reynolds-averaged momentum equations are adopted as the governing equations to resolve complex viscous flow characteristics, including propeller blade rotation, rim gap leakage, and non-uniform stern wake. The complete details of the solver configuration are elaborated as follows.
- (1)
Core solver and coupling algorithm
A pressure-based transient solver is selected to solve the viscous flow field. The SIMPLEC algorithm is adopted for pressure–velocity coupling, which provides stable convergence for narrow-rim clearance flow and rotating-blade flow. For spatial discretization, a second-order upwind scheme is applied to the convection terms of momentum, turbulent kinetic energy, and specific dissipation rate; a central differencing scheme is used for all diffusion terms to reduce numerical dissipation.
- (2)
Turbulence model and wall treatment
The two-equation turbulence model is utilized, which balances the near-wall boundary-layer prediction and far-field wake capture for ducted propulsors. To match the target Y+ range of 30–60 on all solid walls, the scalable wall function is activated instead of low-Reynolds wall treatment, avoiding extra mesh refinement inside the viscous sublayer and guaranteeing calculation efficiency.
- (3)
Transient sliding mesh settings
The sliding mesh interface is defined between the rotating domain and stationary domain. The rotational speed of the moving zone is assigned according to working conditions, with variable time steps configured to control the blade rotation angle per time step. Three step sizes are tested for uncertainty quantification: ( per step), ( per step), ( per step). For all formal simulations, the time step of is adopted to balance accuracy and computational cost.
- (4)
Boundary condition configuration
The far-field inlet boundary is set as a velocity inlet, where axial flow velocity is input according to the target advance coefficient J; initial turbulence intensity is fixed at 5% and turbulent viscosity ratio at 10, consistent with the water tunnel environment. The outlet boundary is defined as a pressure outlet with relative static pressure equal to zero gauge pressure. All surfaces of the blades, rim, and duct are set to no-slip stationary walls, except the rotating region assigned rigid-body rotation motion. Symmetry boundary conditions are applied to the lateral cylindrical faces of the outer computational domain to eliminate far-field boundary interference.
2.2. Numerical Simulation of Rim-Driven Thruster
The research object of this paper is a large, hundred-ton heavy-load autonomous underwater vehicle (AUV), which is mainly applied to long-duration operations in shallow and medium seas, with the capacity to undertake emergency deep-water tasks. Its main body adopts a streamlined revolving hull similar to the SUBOFF standard model. Such a streamlined configuration can effectively reduce frictional resistance and form resistance during navigation. The main propulsion system is mounted at the stern propulsion section of the AUV, providing core power for forward, backward, and depth-keeping cruising motions.
The overall length of the full-scale vehicle model is 36 m, its maximum hull radius is 1.5 m, and its three-dimensional geometric model is shown in
Figure 1.
The blade tip of the rim-driven thruster is rigidly connected to the rim while the blade root is free, resulting in the maximum bending moment occurring at the blade tip. Therefore, a reverse thickness distribution design with thick blade tips and thin blade roots is adopted to meet the strength requirements. The main geometric parameters of the thruster are as follows: blade diameter of 800 mm, 5 blades, disk area ratio of 0.7, and duct length of 687.5 mm. The geometric parameters and model of the rim-driven thruster are shown in
Table 1 and
Figure 2.
To calculate the thrust of the designed rim-driven thruster, the design speed of 4 kn , propeller diameter of 0.8 m, fluid density (fresh water) and design power of 30 kW are adopted as basic parameters. The thrust under ideal inviscid conditions and the actual thrust after viscous correction are calculated, respectively. The detailed calculation procedures and results are presented as follows:
- (1)
Thrust Calculation under Ideal Inviscid Conditions
Referring to ducted propellers, the relationship between thrust T and power P for a constant-area ducted propeller is derived based on the momentum theory and energy conservation principle:
where P denotes power, T is thrust,
represents sailing speed, and A is the propeller disk area. Substitute the known parameters into the formula:
This is a nonlinear equation requiring numerical solution. Define the function:
The root of
is solved, and the final thrust is obtained as
. Verification is conducted by substituting the result back into the formula:
The actual thrust is corrected from the ideal value via the overall propulsion efficiency:
where
denotes the overall propulsion efficiency, which consists of two components:
Hydraulic efficiency : accounts for losses caused by fluid viscosity, including friction, vortex flow, and flow separation;
Mechanical efficiency : accounts for losses induced by mechanical motion such as friction and vibration.
The hydraulic efficiency is determined by the thrust loading coefficient
Substituting the target thrust which corresponds to a medium loading condition. According to marine propulsion experience, the typical hydraulic efficiency range of ducted rim-driven thrusters under this load coefficient is 0.75 to 0.85.
Adopting representative characteristic values, where the mechanical efficiency
and hydraulic efficiency
, the overall propulsion efficiency is calculated as 0.8245. The actual thrust is expressed as
Therefore, the propeller with a diameter of can generate a thrust of 6807 N at the sailing speed of 4 kn.
A cylindrical full-flow computational domain is adopted for simulation, which is divided into a rotating domain and a stationary domain. The diameter of the stationary domain is 4D, with an inlet length of 3D and an outlet length of 6D (D refers to the blade diameter). The diameter of the rotating domain is 2 mm larger than the outer diameter of the rim. For the complex curved walls within the duct region and propeller rotating domain, to accurately resolve the near-wall flow characteristics, the dimensionless wall distance Y+ is controlled within the range of 30–60 for all solid walls. This target range is deliberately selected in accordance with the standard practice for wall-function-based simulations. In the present study, the scalable wall function is employed in conjunction with the turbulence model. This Y+ range ensures that the first near-wall cell lies safely within the log-law region, where the wall function is theoretically valid, while avoiding the buffer layer (5 < Y+ < 30) and the viscous sublayer (Y+ < 5), where the standard wall function would lose accuracy.
To accurately capture critical flow details, including pressure gradients, flow field variations, and tip clearance vortices within the gap, local mesh refinement is implemented for the clearance region with a refined mesh size of 0.05 mm. The first layer thickness of the boundary layer inflation adjacent to the blade and hub surfaces in the rotating domain is set to 0.01 mm, with a total of 15 inflation layers generated. Given the narrow clearance between the propeller blades and the duct, the maximum gap dimension is specified as 0.1 mm, and the mesh size on the blade surfaces is limited to 1 mm. The Reynolds-Averaged Navier–Stokes (RANS) method and
SST turbulence model are employed. The inlet is set as a velocity inlet and the outlet as a pressure outlet. The walls of the propeller and duct are defined as no-slip walls, and the rotating domain adopts a rotating coordinate system. The computational domain and surface mesh of the rim-driven thruster are illustrated in
Figure 3.
In CFD numerical simulations, mesh quality and cell count directly govern the solution accuracy of flow fields, while exerting notable impacts on computational efficiency and convergence performance. To eliminate the interference of mesh density on numerical results and balance simulation precision with computational efficiency, six sets of computational cases with total mesh cells increasing gradually from 1 million to 8 million are designed in this study for grid independence verification. The advance coefficient
and rotational speed of 240 rpm are selected as the validation conditions, with thrust coefficient
adopted as the primary evaluation indicator. The mesh cell numbers corresponding to each case are listed in
Table 2.
With all other computational conditions maintained identical, numerical simulations are conducted on six rim-driven thruster models with distinct mesh cell counts. The calculated thrust coefficients and corresponding relative errors under each mesh scheme are acquired, and the computational results for various mesh quantities are illustrated in
Figure 4.
As indicated by the grid independence verification results, the numerical predictions gradually converge without obvious fluctuations once the total mesh cell count exceeds 5.2 million. This demonstrates that adopting a mesh size of approximately 5.2 million cells for subsequent calculations can effectively reduce hardware resource consumption and computational costs while guaranteeing numerical accuracy. Accordingly, all follow-up numerical simulations of the rim-driven thruster model are performed with mesh quantities ranging from 5.2 million to 6.8 million cells.
To systematically investigate the open-water performance of the rim-driven thruster, the rotational speed is set to 240 rpm, and the advance coefficient is adjusted by changing the axial incoming flow velocity. The open-water performance results of the thruster at the advance coefficient
are listed in
Table 3.
Taking the inlet section of the thruster (0 D) as the starting point and defining the flow direction at the outlet as the positive axial direction, the velocity distributions at six characteristic axial sections of 0 D, 0.25 D, 0.5 D, 0.75 D, 1 D, and 1.25 D are extracted to analyze the axial evolution characteristics of the flow field. The contour plots of different sections are shown in
Figure 5.
In terms of the axial evolution of the flow field, the incoming flow remains uniform in the upstream region of the thruster (0 D~−0.55 D). A slight rise in flow velocity occurs near the duct inlet, which reflects the suction effect of the rim-driven thruster. At the propeller disk (0.5 D), the flow field is disturbed by rotating blades, resulting in obvious circumferential non-uniformity of velocity distribution, where the high-velocity regions correspond exactly to the positions of the blades. In the downstream area of the rim-driven thruster (0.75 D~1 D), the swirling flow generated by blade rotation gradually diffuses, and the flow velocity decreases along the axial direction until the flow field returns to a uniform state. The intensity of swirling flow at sections downstream of 0.5 D decays by more than 40%. The flow field basically restores an axisymmetric distribution at the sections of 1 D and 1.25 D.
According to the simulation results for axial velocity contours (
Figure 6) and global pressure and flow field contours (
Figure 6), the pressure on the outer wall of the duct is distributed uniformly and is roughly equal to the ambient pressure of the incoming flow. Pressure variation is mainly concentrated inside the duct passage. Divided by the propeller disk, the interior of the duct presents a distinct three-stage pressure distribution: the area ahead of the propeller disk is a low-pressure zone, the middle throat section serves as a medium-pressure transition zone, and the area behind the propeller disk is a high-pressure zone. The axial pressure difference between the inlet and outlet of the duct produces positive thrust on the duct itself, indicating that the duct can achieve an obvious thrust-augmentation effect under heavy-load and low advance-coefficient conditions.
2.3. CFD Uncertainty Quantification Analysis
The CFD uncertainty quantification analysis in this paper covers three independent components: grid discretization uncertainty, temporal discretization uncertainty, and iterative convergence uncertainty. A full set of uncertainty quantification analyses is carried out for the benchmark open-water condition of the single thruster with advance coefficient (J = 0.6) and rotational speed (
n = 240 rpm). The calculation of grid discretization uncertainty in this study strictly complies with the ITTC standard for CFD verification. Meanwhile, the systematic procedure proposed by Eça for estimating numerical uncertainties of CFD computations via grid refinement studies is also adopted [
28,
29].
2.3.1. Mesh Discretization Uncertainty Quantification
Three sets of unstructured meshes with identical topology and systematic uniform refinement are adopted. Only the mesh size is changed proportionally, while all other boundary conditions, discretization schemes, and turbulence models remain exactly the same. The basic mesh parameters are listed in
Table 4.
Based on Richardson extrapolation theory, the actual convergence order p is first solved using the target physical quantity (thrust coefficient ) obtained from the three sets of meshes, and then the Grid Convergence Index (GCI) of the fine mesh is calculated. The formulas are given as follows:
Convergence Order Calculation:
where
are the target physical quantities under coarse, medium, and fine meshes, respectively; r denotes the mesh refinement ratio.
Grid Convergence Index (GCI):
where
represents the safety factor, which takes a standard value of 1.25 for three mesh sets;
denotes the relative mesh discretization uncertainty
of the fine mesh.
- (3)
Quantification Results
The thrust coefficients calculated from the three mesh sets are: , , . Substituting these values into the formulas yields:
The actual convergence order is approximately , which falls within the monotonic asymptotic convergence range and conforms to the law of numerical convergence.
The Grid Convergence Index of the fine mesh is , meaning the mesh discretization uncertainty .
This result indicates that for the computational meshes of 5.20 million~6.80 million cells adopted in this work, the discretization error falls within the engineering-acceptable range (the generally accepted industry threshold is less than 3%), and the mesh resolution satisfies the requirement for computational accuracy.
The computational domain of the AUV-thruster coupled system includes the complete AUV hull, X-shaped rudders, and thruster. The total mesh count is approximately three times that of the single-thruster model, which brings a considerable rise in transient computational cost. Limited by computational resources, the full three-mesh GCI analysis was not repeated for the coupled system. However, the coupled system adopts exactly the same mesh-generation strategy, boundary-layer growth ratio, local refinement criteria, and Y+ control range as the single-thruster model throughout the simulation. Convergence has been verified via mesh-refinement comparisons in key regions. Consequently, its mesh discretization uncertainty is the same order of magnitude as that of the single-thruster model, laying a consistent foundation for the reliability of numerical results.
2.3.2. Temporal Discretization Uncertainty Quantification
A transient sliding-mesh approach is adopted in this paper to simulate the rotation of propeller blades. The discretization error induced by time-step size constitutes an essential component of numerical uncertainty, and its quantification method shares the same origin as the mesh-based GCI.
Three sets of proportionally scaled time-step sizes are selected. The corresponding propeller blade rotation angles per time step are , , and . At a rotational speed of 240 rpm, the corresponding time-step sizes are , , and , respectively. All other computational settings remain identical.
- (2)
Quantification Results
Adopting the same calculation method as the mesh-based GCI, the time-step convergence order is obtained, and the temporal convergence index for the fine time-step , namely, the temporal discretization uncertainty .
The results demonstrate that the time-step setup adopted in this work is sufficiently convergent. The temporal discretization error is very small and contributes little to the overall numerical uncertainty.
2.3.3. Iterative Convergence Uncertainty Quantification
Iteration error refers to the fluctuation error induced by iterative solving within each time step, which is quantified by a statistical method in this work:
1. After the computation is fully converged, the thrust coefficient is continuously monitored over 20 complete propeller-blade rotation cycles, and sample data in the steady-state segment are extracted.
2. The relative standard deviation within the 95% confidence interval is taken as the iterative uncertainty:
where S denotes the sample standard deviation, and
represents the mean value of the physical quantity.
The calculated relative iterative-convergence uncertainty under the baseline condition is . This indicates that the dual convergence criteria for residuals and physical quantities are reasonably set, and the iteration error can be neglected.
2.3.4. Synthesis of Total Numerical Uncertainty
The three types of errors, i.e., mesh discretization error, temporal discretization error, and iterative convergence error, are mutually independent. The root-sum-square method is adopted to synthesize the total numerical uncertainty:
Substituting each component for calculation yields that the total relative numerical uncertainty under the baseline condition. The overall result achieves a relatively high-accuracy level and satisfies the engineering accuracy requirements for CFD numerical prediction of marine propulsors.