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Formulations of Hydrodynamic Force in the Transition Stage of the Water Entry of Linear Wedges with Constant and Varying Speeds

Xueliang Wen [email protected] Peiqing Liu [email protected] Alessandro Del Buono [email protected] Qiulin Qu [email protected] Alessandro Iafrati [email protected] School of Aeronautic Science and Engineering, Beihang University, Beijing, 100191, China CNR-INM, Via di Vallerano 139, 00128 Rome, Italy
Abstract

There is an increasing need to develop a two-dimensional (2D) water entry model including the slamming and transition stages for the 2.5-dimensional (2.5D) method being used on the take-off and water landing of seaplanes, and for the strip theory or 2D+t theory being used on the hull slamming. Motivated by that, this paper numerically studies the transition stage of the water entry of a linear wedge with constant and varying speeds, with assumptions that the fluid is incompressible, inviscid and with negligible effects of gravity and surface tension, and the flow is irrotational. For the constant speed impact, the similitude of the declining forces of different deadrise angles in the transition stage are found by scaling the difference between the maximum values in the slamming stage and the results of steady supercavitating flow. The formulation of the hydrodynamic force is conducted based on the similitude of the declining forces in the transition stage together with the linear increasing results in the slamming stage. For the varying speed impact, the hydrodynamic force caused by the acceleration effect in the transition stage is formulated by an added mass coefficient with an averaged increase of 27.13%27.13\% compared with that of slamming stage. Finally, a general expression of the hydrodynamic forces in both the slamming and transition stages is thus proposed and has good predictions in the ranges of deadrise angles from 55^{\circ} to 7070^{\circ} for both the constant and varying speed impacts.

keywords:
water entry, wedge, hydrodynamic force, transition stage
journal: Journal of Fluids &\& Structures Templates

Nomenclature

𝐚\bf a = Accelerations of body
awa_{w} = Acceleration of body in vertical direction
AA = Dimensionless variable of the theory of steady supercavitating flow
A2A_{2}, B2B_{2} = Dimensionless variables of approximate solution
A2MeiA_{2\rm Mei}, B2MeiB_{2\rm Mei} = Dimensionless variable of Mei et al.’s model
cc = Effective wetted length
CaC_{a} = Added mass coefficient
Ca0C_{a0} = A2(k2tanβ)2A_{2}(k_{2}\tan\beta)^{2} Added mass coefficient in the slamming stage
CconstC_{\rm const} = Dimensionless coefficient of constant speed impact
CKorobkinC_{\rm Korobkin} = CconstC_{\rm const} of Korobkin’s model
CpC_{p} = Pressure coefficient
Cp0C_{p0} = Pressure coefficient of constant speed impact
cqc_{q} = Volume fraction of qthq^{th} fluid
CsC_{s} = Slamming coefficient
Cs0C_{s0} = Slamming coefficient of constant speed impact
Cs0C_{s0}^{*} = (Cs0Cs)/(CsmaxCs)({C_{s0}-C_{s\infty}})/({C_{s\rm max}-C_{s\infty}})
CsmaxC_{s\rm max} = Maximum Slamming coefficient
CsC_{s\infty} = Slamming coefficient of steady supercavitating flow
f3Df_{\rm 3D} = Force coefficient of 3D effect
FF = Force acting on bodies in vertical direction
𝐅\mathbf{F} = Total hydrodynamic forces acting on the body surface
F0F_{0} = Force acting on bodies of constant speed impact
FrFr = U0/glU_{0}/\sqrt{{\rm g}l} Froude number of the freefall motion case
g\rm g = Gravitational acceleration
𝐠\mathbf{g} = Body forces in Euler equations
GG = Core function of the second Green identity
hh = Penetration depth
h0h_{0} = ltanβl\tan\beta Height of wedge
h2h_{2} = Penetration depth corresponding to CsmaxC_{s\rm max}
hh^{*} = (hh2)/h2cotλβ({h-h_{2}})/{h_{2}}\cot^{\lambda}\beta
kk = Parameter of curved FBC
k1k_{1} = h2/h0h_{2}/h_{0} Dimensionless penetration depth of the maximum Cs0C_{s0}
k2k_{2} = Cs0(h/h0)\frac{\partial C_{s0}}{\partial(h/h_{0})} Dimensionless derivative of Cs0C_{s0} with respect to hh
ll = Half width of a finite body
LL = Thickness of a 3D wedge
mm = Mass of the wedge
m0m_{0} = Added mass of wedge in half model
𝐧\bf n = Unit vector of normal to the wall surface
nyn_{y} = Projection in vertical direction yy of 𝐧\bf n
NN = Number of nodes to calculate parameter nn
pp = Pressure
p0p_{0} = Pressure of constant speed impact
pap_{a} = Atmosphere pressure
P¯\bar{P} = Vertices of the lower side in jet region
P¯\bar{P} = Vertices of the upper side in jet region
rr = Ratio between the normal distance between the two side
of the jet in proximity of the spray root and the minimun panel size
tt = Time
𝐮\mathbf{u} = ϕ\nabla\phi Velocities of fluid
unu_{n}, usu_{s} = Normal and tangential projections of fluid velocity on the body surface
U0U_{0} = Initial speed of wedge
UwU_{w} = Instantaneous speed of wedge
vv = Fluid velocity of the theory of steady supercavitating flow
v0v_{0} = Incoming velocity of water of steady supercavitating flow
𝐕q{\bf V}_{q} = Velocities of the qthq^{th} fluid
vnv_{n} = Vertical velocity on the free surface
𝐕\bf V = Velocities of fluid
wnw_{n}, wsw_{s} = Normal and tangential projections of body speeds on the body surface
𝐖\bf W = Body speeds
𝐱\bf x = Position of particles lying on the free surface
xx, yy, = Cartesian coordinates
zz = x+iyx+{\rm i}y Complex coordinates
α\alpha, χ\chi, μ\mu, = Coefficients of the velocity potential expression in the jet region
β\beta = Deadrise angle of wedge bodies
βL\beta_{L} = Deadrise angle of linear FBC
Δp\Delta p = Difference of pressure between the constant and varying speed impacts
ΔF\Delta F = Difference of force between the constant and varying speed impacts
η\eta = 1Ni=1Nσi2\frac{1}{N}\sum\limits_{i=1}^{N}{\sigma_{i}^{2}} Mean σ\sigma of all the nodes in h[0,  7]h^{*}\in[0,\,\,7]
γ\gamma = Correction factor of wetted length
γMei\gamma_{\rm Mei} = Correction factor of wetted length for Mei et al.’s model
κ\kappa = Growth factor of BEM-FEM panels
λ\lambda = Auxiliary variable to model the Cs0C_{s0} in the transition stage
ω\omega = Parameter complex plane
ϕ\phi = Velocity potential
ϕ0\phi_{0} = Velocity potential at C and C’ in the theory of steady supercavitating flow
Φ\Phi = Dimensionless velocity potential of similarity solution
ρ\rho = Density of water
σ\sigma = Standard deviation of Cs0C_{s0}^{*} between different deadrise angles
τ\tau = Parameter complex plane
θ\theta = Argument of the velocity of fluid
SuperscriptSuperscript
JJ = Panel in the jet region
* = Variables at the centroid of fluid control volume
SubscriptSubscript
qq = Phase of fluid
ii = Index of vertices in the jet region or index of node

1 Introduction

Refer to caption

Fig. 1: The free surfaces of different cross-sections of a hull during the high speed planning.

The take-off and water-landing of seaplanes had been studied since 1920s and the procedures to assess the structural crashworthiness of airframe is mainly based on a 2.5-dimensional (2.5D) method [1, 2, 3], which is similar to the formulations of slamming forces of the strip theory for the hull slamming. Every individual cross-section normal to the longitudinal direction of hull independently experiences a single process of water entry (see Fig. 1), where the 2D water entry model is formulated by the added mass method [4, 1, 2] or the Wagner theory [5, 3]. The traditional procedures had been identified to be less accurate as the numerical methods have fast developed in recent decades, and make it possible to conduct numerical simulations of water-landing of seaplanes [6] and transport airplanes [7, 8]. Although a whole-time history of water entry of aircraft can be reproduced, massive computational resources are required and several days of calculations are taken. This could not be treated as a practical method for the engineers to complete the initial designs of seaplanes or high-speed planning hulls [9, 10]. The alternative method is to improve the 2D model of the 2.5D methods because the errors of early 2.5D methods are mainly resulted from the transverse pressure distribution, especially for that with chine immersion. For the cross-section C Fig. 1 without chine immersion, they used the Wagner theory; For the cross-sections A and B in Fig. 1 with chine immersion, they adopted the pressure distribution of a steady supercavitating flow [11, 12] to formulate the transverse flow. However, the pressure distribution of Wagner theory is quite different from that of steady supercavitating flow. How the pressure distribution continuously changes from that of Wager theory to that of steady supercavitating flow is missing in the early 2.5D methods.

Refer to caption

Fig. 2: The cross-sections (normal to the keels) of the hull of seaplanes.

From the perspective of a 2D transverse flow in a constant speed, the cross-section without chine immersion is corresponding to a slamming stage in which the hydrodynamic force increases linearly with the increasing wetted length, and the cross-section with chine immersion is corresponding to a transition stage in which the body experiences a fast drop of hydrodynamic force when the spray root leaves the chine. The pressure distribution and the hydrodynamic force gradually decline and finally approach those of steady supercavitating flow, as the experimental results of Zhao et al. [13] indicated. The poor accuracy of original 2.5D methods is due to the weakness of their 2D model for the transverse flow and lack of involvement of the hydrodynamic forces acting on afterbody of hull (see Fig. 2). Since there is no effective theoretical method to formulate the transition stage, Sun and Faltinsen [14, 15] directly adopted a boundary element method (BEM) as the 2D water entry model to develop another similar method called 2D+t theory for the high speed hulls. Their BEM [16, 13] can address both the slamming and transition stages with increasing accuracy of predictions, but at the same time greatly increases the computational cost, which undermines the efficiency of the 2D+t theory. Therefore, there is an increasing need to improve the efficiency of the 2.5D methods and the 2D+t theory by proposing an analytical solution as accurate as the numerical methods to predict the hydrodynamic forces in both slamming and transition stages. For the slamming stage, many researchers had contributed to the formulations of hydrodynamic force by added mass methods [4, 5, 17], asymptotic theories [18, 19, 20] and approximate solution [21]. Among them, the approximate solution of Wen et al.[21] provided the most accurate model for the constant and varying speed cases by a similarity solution of Dobrovol1’skaya[22]. For the transition stage, due to the different hydrodynamic characteristics, the formulation of hydrodynamic force is more difficult and is yet to be fully addressed. In this paper, by following the formulation work of our previous research [21], the transition stage of the water entry of linear wedges with constant and varying speeds, as shown in Fig. 3, is formulated to complete the 2D water entry model.

Refer to caption

Fig. 3: The description of the water entry of a 2D wedge with a speed of UwU_{w}, hh being the penetration depth.

There are three different formulations of the hydrodynamic forces in the transition stage in literature. The first one was proposed by Logvinovich[18] based on the boundary condition at the separation (point C in Fig. 3). The pressure at C is required to be same with the atmospheric pressure, which is denoted as zero pressure condition. Logvinovich derived an ordinary differential equation (ODE) to obtain a virtual wetted length but integrated the pressure to obtain the hydrodynamic force on the real wetted surface AC. Tassin et al. [23] improved the Logvinovich’s model by introducing the correction of 1+tan2β\tan^{2}\beta (β\beta being the deadrise angle) to the pressure expression on the wall surface and re-derived the ODE of virtual wetted length. The predictions are in better agreement with BEM results of Iafrati and Battistin [24] than the original one. The second way is called fictitious body continuation (FBC) and was also developed by Tassin et al. [23] based on a modified Logvinovich’s model (MLM) of Korobkin [20] who addressed the formulation of the slamming stage. The FBC is a virtual wall surface extended from the separation C with an angle of βL\beta_{L} with respect to the horizonal line (see Fig. 3). The wetted length is solved from the combination of the real wall surface AC and FBC, while the hydrodynamic force is only integrated on AC as it does in the Logvinovich’s model of the zero pressure condition. Tassin et al. [23] had to compare with the numerical results to identify the parameter βL\beta_{L}. Although the agreement with the numerical results is better than the Logvinovich’s model with correction 1+tan2β\tan^{2}\beta, there is still some discrepancy and the FBC needs more improvement. Wen et al. [25] proposed the curved FBC to improve the accuracy of linear FBC of Tassin et al. [23] based on a modified Wagner’s model (MWM). They introduced another parameter kk and provided explicit equations to determine βL\beta_{L} and kk. Their predictions were in better agreement with the numerical results than the linear FBC of Tassin et al. [23]. Since these methods are all based on the Wagner theory [5], their predictions will become less accurate when the deadrise angle is larger than 30. The last and the most sophisticated formulation was conducted by Semenov and Wu [26] by extending their integral hodograph method (IHM) [27, 28] from the slamming stage to transition stage. Their results show a larger declining force than the BEM simulations of Iafrati and Battistin [24] because they imposed a self-similar solution onto a non-self-similar flow in the transition stage. In general, the fully analytical solutions as accurate as the numerical results and with a range of deadrise angle [15,  45][15^{\circ},\,\,45^{\circ}] for the applications of take-off and water landing of seaplanes are currently unavailable. In contrast to formulate the hydrodynamic force by the asymptotic analysis and self-similar solution, a semi-analytical solution for both the slamming and transition stages can be probably built by summarizing the numerical results and exploring the possible patterns of the hydrodynamic forces.

The failures of the abovementioned theoretical methods to formulate the hydrodynamic forces in the transition stage is caused by inaccurate modelling of free surface, which is the main difference between the numerical methods and the theoretical methods. There are two broad categories of the numerical methods: BEM and computational fluid dynamics (CFD). The free surface problems of water entry for the BEM include the modelling of jet and the new free surface AC. Zhao et al. [13] provided the first fully nonlinear BEM results, using a model of jet-cut to avoid the high-speed thin jet, and the lowest-order expansion of the Kutta condition (the flow leaves the body tangentially at the separation point C) to simplify the new free surface AC. Iafrati and Battistin [24] proposed a different approach to switch boundary conditions (BCs) of the panels from a wall panel to a free surface panel when the center of panel leaves the separation point C. Instead of using the jet cutting strategy as Zhao and Faltinsen [16] and their previous method [29] did, they combined the use of a BEM solver in the bulk of fluid and a simplified finite element method (FEM) in the thin jet developing along the body contour. The hybrid method was denoted as a hybrid BEM-FEM (HBF) approach and can provide a detailed description of the flow and free surface dynamics, together with an improved prediction of the separation, while keeping the computational effort still reasonable. The HBF method was recently extended by Del Buono et al. [30] to deal with the water entry with varying speed and the water exit problems. Considering the good application of the BCs switching, Wang and Faltinsen [31] also develop their BEM of jet cutting replacing the lowest-order expansion of the Kutta condition with the BCs switching for the water entry problems. In contrast to the BCs switching and FEM solver, Bao et al. [32] used the least orders of equations to update the normal velocity of the free surface AC and a shallow water assumption for the jet region in the transition stage. The abovementioned BEM methods have different strategies for the jet region and new free surface AC, but are basically consistent with each other. They can reduce the computational cost and provide the velocity potential distribution on the wedge surface, which is important for the varying speed impact. Different from the complexity of the free surface modelling of BEM, the CFD methods are more flexible to deal with the modelling of free surface. The most widely used method for the free surface problems, volume of fraction (VOF), was first proposed by Hirt and Nichols [33] based on the framework of finite volume method (FVM). A modified high-resolution interface capturing scheme (Modified HRIC) was developed by Muzaferija et al. [34] to solve volume fraction equations and has good applications to the water entry problems [8, 35, 36]. Compared with the BEM approaches, the CFD methods provide more information about the distributions of pressure and velocities in the whole region which intuitively picture the rapid changes of flow field in the transition stage of the constant speed impact. The FVM with VOF has been the most successful method to deal with the water entry problems and will be adopted in this paper to produce the numerical results of constant speed impact. In order to study the distribution of velocity potential on the wall surface for the varying speed impact, the HBF of Iafrati and Battistin [24] will also be used to provide the required data.

In this paper, the slamming and transition stages of water entry of linear wedges with constant and varying speeds are numerically studied by the FVM with VOF [36] and the HBF of Iafrati and Battistin [24]. To propose a semi-analytical solution of a combination of numerical results and theoretical results to address the high speed impact problems, the fluid is considered to be incompressible, non-viscous, weightless and with negligible surface tension effects and the flow is to be irrotational. The hydrodynamic forces in the slamming and transition stages during the water entry of a wedge with constant and varying speeds will be formulated. The arrangements of this paper are as follows. The computational approaches of FVM with VOF and HBF are detailed in Sec. 2 and the validations of the two methods are given in Sec. 3. For the constant speed impact, the formulation of forces in both slamming and transition stages of the water entry of linear wedges with the deadrise angles varying from 55^{\circ} to 7070^{\circ} is proposed based on the CFD results in Sec. 4. For the varying speed impact, the acceleration effect is addressed based on the HBF results in Sec. 5. The general formulations of hydrodynamic force of both the slamming and transition stages will be provided and can address the constant speed impact and the acceleration effect.

2 Computational Approaches

A CFD method of FVM with VOF technique is adopted to provide the detailed results of flow field of water entry in a constant speed and the HBF [24, 37] is used to calculate the velocity potential (the CFD method can’t provide the velocity potential) and the pressure distributions on the wedge surface during the water entry in a varying speed.

2.1 CFD method

2.1.1 Flow solver

The unsteady incompressible Euler equations ignoring the surface tension force are solved using ANSYS FLUENT as follows

𝐕t+𝐕𝐕=1ρp𝐠,\frac{{\partial{\bf V}}}{{\partial t}}+{\bf V}\cdot\nabla{\bf V}=-\frac{1}{\rho}{\bf\nabla}p-\mathbf{g}, (1)

where 𝐕\bf V is the velocity of fluid, ρ\rho is the density, pp is the pressure and 𝐠=(0,g)\mathbf{g}=(0,-\rm g) representing the gravity of fluid (the gravity of fluid can be neglected for the high speed impact). The semi-implicit method for pressure linked equation consistent algorithm (SIMPLEC) is used to deal with the pressure-velocity coupling. The unsteady terms are discretized by first order implicit scheme, the convention terms are discretized by second order upwind scheme, and the pressure term is discretized by body force weighted scheme.

2.1.2 VOF method

The VOF method was firstly proposed by Hirt and Nichols [33], which can capture the free interfaces between two or more immiscible fluids by introducing a variable, called volume fraction, for each phase. If the volume fraction of the qthq^{th} fluid in a certain cell is denoted as cqc_{q}, cq=0c_{q}=0 represents the cell is empty of the qthq^{th} fluid; cq=1c_{q}=1 represents the cell is full of the qthq^{th} fluid; and 0<cq<10<c_{q}<1 represents the cell contains the interface between the qthq^{th} fluid and other fluids. The sum of the volume fractions of all phases must be 1 in each cell. The volume fraction equation of the qthq^{th} fluid is written as follows:

t(cqρq)+(cqρq𝐕q)=0,\frac{\partial}{{\partial t}}({c_{q}}{\rho_{q}})+\nabla\cdot({c_{q}}{\rho_{q}}{\bf V}_{q})=0, (2)

where 𝐕q{\bf V}_{q} is the velocity of qq fluid. The first term in the left hand is discretized by one order implicit scheme, and the second term is discretized by modified high resolution interface capturing (Modified HRIC) scheme [34].

2.1.3 GMM method and VOF boundary conditions

In this paper, the global moving mesh method (GMM) [38] is used to deal with the motion of wedge. The whole computational domain (including the cells and boundaries) moves together with the wedge like a rigid body. The volume fraction boundary conditions can ensure that the free water surface keeps a given level when the computational domain moves. This condition is set according to the cell coordinates of the boundaries in the earth fixed coordinate system, i.e., the volume fraction of water cq=0.5c_{q}=0.5 for the cell located on the interface between air and water; cq=0c_{q}=0 for the cells located above the interface; cq=1c_{q}=1 for the cells located below the interface.

2.2 HBF approach

In this section, the fully nonlinear potential flow model based the hybrid BEM-FEM approach is presented. The method is mainly based on the studies of Refs. [24, 37], where full details are provided.

2.2.1 Governing Equations

The water entry problem of rigid bodies is faced under the hypotheses of an inviscid and incompressible fluid. The flow is assumed irrotational and the problem is formulated in terms of the velocity potential ϕ\phi. Surface tension effects are neglected. The flow is therefore governed by the following initial-boundary value problem:

2ϕ=0inwaterdomainΩ,\nabla^{2}\phi=0\quad{\rm{in\,\,water\,\,domain}}\,\,\Omega, (3)
ϕn=𝐖𝐧=UwnyonwallsurfaceSB,\frac{\partial\phi}{\partial n}={\bf W}\cdot{\bf n}=-U_{w}n_{y}\quad{\rm on\,\,wall\,\,surface\,\,}S_{\rm B}, (4)
DϕDt=|ϕ|22gy,D𝐱Dt=ϕ,onfreesurfaceSS,\frac{{{\rm{D}}\phi}}{{{\rm{D}}t}}=\frac{{{{\left|{\nabla\phi}\right|}^{2}}}}{2}-{\rm g}y,\quad\frac{{{\rm{D}}{\bf{x}}}}{{{\rm{D}}t}}=\nabla\phi,\quad{\rm on\,\,free\,\,surface\,\,}S_{\rm S}, (5)

where 𝐧\bf n is the unit vector of normal to the wall surface, nyn_{y} is the projection of 𝐧\bf n in the vertical direction yy, 𝐖{\bf W} is the entering speed of the body, and 𝐱\bf x is the position of the particle lying on the free surface. At each time step, the solution of the boundary-value problem for the velocity potential is solved in the form of the boundary integral representation provided by the second Green’s identity

12ϕ(P)=SBSS[ϕn(Q)G(P,Q)ϕ(Q)Gn(P,Q)]dS(Q),PSBSS\frac{{\rm{1}}}{{\rm{2}}}\phi\left(P\right)=\int_{{S_{\rm B}}\cup{S_{\rm S}}}{\left[{{\phi_{n}}\left(Q\right)G\left({P,Q}\right)-\phi\left(Q\right){G_{n}}\left({P,Q}\right)}\right]{\rm{d}}S\left(Q\right)},\,\,P\in S_{\rm B}\cup S_{\rm S} (6)

where G(P,Q)=12πlog(|PQ|)G\left({P,Q}\right)=\frac{1}{{2\pi}}\log\left({\left|{P-Q}\right|}\right). According to Eqs. (4)-(5), the velocity potential is known on the free surface while its normal derivative is assigned on the body contour, which belongs to a boundary integral equation of mixed first and second kind. Once Eq. (6) is solved, the velocity potential and its normal derivative are known on the body contour and the free surface. The solution of the boundary integral equation Eq. (6), providing the normal derivative of the velocity potential on the free surface, allows the determination of the velocity field on the free surface, which is integrated in time through a two-step Runge-Kutta scheme to update the position of particle of the free surface.

2.2.2 Pressure distribution

The pressure distribution along the body contour is obtained through the Bernoulli’s equation:

ppa=ρ(ϕ˙+|ϕ|22+gy),p-{p_{a}}=-\rho\left({\dot{\phi}+\frac{{{{\left|{\nabla\phi}\right|}^{2}}}}{2}+{\rm g}y}\right), (7)

and the total hydrodynamic load is obtained by integration of the pressure field along the wetted part of the body

𝐅=SB(ppa)𝐧dS.\mathbf{F}=-\int_{{S_{B}}}{\left({p-{p_{a}}}\right){\mathbf{n}}{\rm d}S}. (8)

ϕ˙\dot{\phi} has to be provided before the pressure distribution on the wall surface is given. The calculation of ϕ˙\dot{\phi} is similar to ϕ\phi. On the free surface, the ϕ˙\dot{\phi} is known as ϕ˙=|ϕ|22gy\dot{\phi}=-\frac{{{{\left|{\nabla\phi}\right|}^{2}}}}{2}-{\rm g}y according to Eq. (5). On the wall surface, the normal derivative of ϕ˙\dot{\phi} is known and calculated as

ϕ˙n=𝐚𝐧wsunswnuss+ks𝐖𝐮,\frac{{\partial\dot{\phi}}}{{\partial n}}={\bf a\cdot n}-{w_{s}}\frac{{\partial{u_{n}}}}{{\partial s}}-{w_{n}}\frac{{\partial{u_{s}}}}{{\partial s}}+{k_{s}}{\bf W\cdot\mathbf{u}}, (9)

where 𝐚\bf a is the body acceleration, wsw_{s} and wnw_{n} are the tangential and normal projections of 𝐖{\bf W} on the wall surface, usu_{s} and unu_{n} are the tangential and normal projections of 𝐮=ϕ\mathbf{u}=\nabla\phi on the wall surface and ksk_{s} denotes the curvature of the wall surface. The normal derivative of ϕ˙\dot{\phi} on free surface and the ϕ˙\dot{\phi} on the wedge surface can be solved by a similar boundary integral equation of Eq. (6). it is worth noting that the gravitational acceleration g\rm g is only used for the validations of freefall cases in Figs. 10 and 25, and is never included in other cases.

2.2.3 Jet model

Refer to caption

Fig. 4: The description of the jet model of the simplified FEM solver.

In the simplified FEM solver used for the description of the thin jet, a part of the jet region is divided in control volumes in which the vertices corresponding to the panel centroids (P¯i1\bar{P}_{i-1}, P¯i\bar{P}_{i}, P^i1\hat{P}_{i-1}, P^i\hat{P}_{i}), as shown in Fig. 4. In each control volume, the velocity potential is written in the form of a harmonic polynomial expansion, up to second order. Details about the approach in the slamming stage can be found in Battistin and Iafrati [24] and Del Buono et al. [30]. For the transition stage, the harmonic polynomial expansion, ϕiJ\phi_{i}^{J} is reduced to first orders and reads

ϕiJ(x,y)=αi+χi(xxi)+μi(yyi).\phi_{i}^{J}\left({x,y}\right)={\alpha_{i}}+{\chi_{i}}\left({x-x_{i}^{*}}\right)+{\mu_{i}}\left({y-y_{i}^{*}}\right). (10)

The corresponding normal derivative is

ϕn,iJ(x,y)=χinx,i+μiny,i\phi_{n,i}^{J}\left({x,y}\right)={\chi_{i}}{n_{x,i}}+{\mu_{i}}{n_{y,i}} (11)

where (xi,yj)(x_{i}^{*},\,y_{j}^{*}) is the centroid of the fluid control volume PiP_{i}^{*}, nx,i{n_{x,i}} and ny,i{n_{y,i}} are the unit vector of the ithi^{th} panel which are directed along the xx-axis and yy-axis, αi\alpha_{i}, χi\chi_{i} and μi\mu_{i} are new unknown variables and can be determined by enforcing the free surface condition

ϕiJ(P¯i1)=ϕ(P¯i1),ϕiJ(P¯i)=ϕ(P¯i),\phi_{i}^{J}\left({{{\bar{P}}_{i-1}}}\right)=\phi\left({{{\bar{P}}_{i-1}}}\right),\quad\phi_{i}^{J}\left({{{\bar{P}}_{i}}}\right)=\phi\left({{{\bar{P}}_{i}}}\right), (12)

and by enforcing the continuity of the ϕn\phi_{n} at adjacent elements

ϕn,iJ(P¯i1)=ϕn,i1J(P¯i).\phi_{n,i}^{J}\left({{{\bar{P}}_{i-1}}}\right)=\phi_{n,i-1}^{J}\left({{{\bar{P}}_{i}}}\right). (13)

3 Validations of numerical methods

3.1 Grid independence

Refer to caption

Fig. 5: Grid independence validation of the CFD simulations for the water entry of a wedge with β=30\beta=30^{\circ} in a constant speed: (aa) Slamming coefficient CsC_{s}; (bb) CpC_{p} distribution of h/h0=0.8h/h_{0}=0.8; Free surface of h/h0=0.8h/h_{0}=0.8.

Figure 5 shows the grid independence validation of the CFD simulations for the water entry of a wedge with β=30\beta=30^{\circ} in a constant speed, where the slamming coefficient CsC_{s} and pressure coefficient CpC_{p} are defined as follows

Cs=F12ρUw2l,C_{s}=\frac{F}{\frac{1}{2}\rho U_{w}^{2}l}, (14)
Cp=ppa12ρUw2,C_{p}=\frac{p-p_{a}}{\frac{1}{2}\rho U_{w}^{2}}, (15)

where UwU_{w} is the entering speed of the body. Three grids of cell numbers of 50,000, 100,000 and 200,000 are adopted to simulate the impact flow with adaptive time steps. The courant number is set to be 0.95 during the adaptive time steps. The CsC_{s} of the whole time-history between the three grids match well. The CpC_{p} distribution and free surface of h/h0=0.8h/h_{0}=0.8 (h0=ltanβh_{0}=l\tan\beta) are also consistent between the three grids except for some discrepancies at the tip of jet. The grid independence of CFD method is successfully validated. Therefore, the CFD grid with cell number of 100,000 is adopted for further simulations by balancing both the accuracy of spatial resolution and the computational cost.

Refer to caption

Fig. 6: Description of the BEM panels and FEM panels in the BEM.
Grids κ\kappa of BEM panels κ\kappa of FEM panels rr
Coarse 1.04 1.05 1.5
Normal 1.03 1.04 2.0
Fine 1.02 1.03 4.0
Tab. 2: The grid details of BEM panels: κ\kappa being the growth factor; rr being the ratio between the normal distance between the two side of the jet in proximity of the spray root and the minimun panel size.

Figure 6 shows the description of the HBF model in which the fluid boundary is divided into three parts: (1) free surface panels; (2) wall surface panels and (3) jet panels. The free surface and wall surface panels are solved by BEM solver while the jet panels are solved by the FEM solver. The panel distribution is determined by three parameters in Tab. 2: growth factors κ\kappa of BEM panels and FEM panels, as well as the ratio rr between the normal distance between the two side of the jet in proximity of the spray root and the minimun panel size. The CsC_{s} and CpC_{p} at the tip of wedge of the three distributions of HBF for the constant speed case in Fig. 7 match well with each other. Here, a normal grid is adopted for most of the HBF calculations in present study.

Refer to caption

Fig. 7: The grid independence of the HBF simulations for the water entry of a wedge with β=30\beta=30^{\circ} in a constant speed: (aa) the slamming coefficient CsC_{s}; (bb) the pressure coefficient CpC_{p} at the tip of wedge.

3.2 Comparisons between different methods

For the slamming stage of constant speed impact in which the self-similar flow is satisfied, the present CFD and HBF methods are compared with the similarity solution of Dobrovol’skaya[22, 36]. For the varying speed impact of both the slamming and transition stages, the present CFD and HBF methods are compared with the predictions of Bao et al.’s BEM [32] for the freefall motion case. In this case, the impact speed is small and the gravity effect will become significant in the transition stage. In the simulations of Bao et al.’s case [32], the gravity of fluid is included. For the other cases, the gravity of fluid is excluded.

Refer to caption

Fig. 8: The comparisons of the pressure coefficient CpC_{p} on the wedge surface and the free surface profiles of h/h0=0.6h/h_{0}=0.6 between the predictions of CFD, HBF and similarity solution [36] during the water entry of a wedge with β=30\beta=30^{\circ} in a constant speed.

For the slamming stage with h/h0=0.6h/h_{0}=0.6 in the case of the water entry of a wedge with β=30\beta=30^{\circ} in a constant speed, Fig. 8 shows the comparisons of the pressure coefficient CpC_{p} on the wedge surface and the free surface profiles between the predictions of CFD, HBF and similarity solution [36]. The spray root of the jet remains under the knuckle of the wedge, which means the self-similar flow is still satisfied and thereby the similarity solution can be used for a validation. The good agreement between the present methods and the similarity solution is excellent.

For the transition stage, Fig. 9 shows the comparisons of the force (aa), pressure distribution (bb) and free surface (cc) between the present CFD and HBF for the water entry of a wedge with β=30\beta=30^{\circ} in a constant speed. The CFD results are all consistent with those of HBF, except for the jet tip of free surface. Since the jet tip is of little relevance with the pressure and force acting on the wedge surface, the mutual validations between the present CFD and HBF are properly conducted. Fig. 10 shows the comparisons of the acceleration (aa), pressure distribution (bb) and free surface (cc) between the CFD method, HBF and BEM of Bao et al. [32] for the water entry of wedges of β=30\beta=30^{\circ} in a freefall motion. The CFD and HBF results are in good agreement with those of the BEM of Bao et al. [32], while there are still minor discrepancies of the jet tip of free surface and the pressure distribution near the apex of wedge. These differences are acceptable for the validations of CFD and HBF methods.

Refer to caption

Fig. 9: Comparisons of the force (aa), pressure distribution (bb) and free surface (cc) between the present CFD and HBF for the water entry of a wedge with β=30\beta=30^{\circ} in a constant speed.

It can be concluded that the CFD method and HBF method are consistent with each other and can deal with the slamming and transition stages of the constant and varying speed impacts. In this paper, the CFD method is mainly used to produce the numerical results of constant speed impact, while the HBF method is to used produce those of varying speed impact.

Refer to caption

Fig. 10: Comparisons of the acceleration (aa), pressure distribution (bb) and free surface (cc) between the CFD, HBF and BEM of Bao et al. [32] for the water entry of wedges of β=30\beta=30^{\circ} in a freefall motion.

4 Constant speed impact

In this section, the constant speed impacts of wedges with different deadrise angles are studied based on the CFD method. The hydrodynamic forces of the three stages are formulated based on a combination of the results of similarity solution of slamming stage, the CFD results of transition stage and the theoretical results of steady supercavitating flow. The steady supercavitating flow is an approximation of the flow around the wedge at a very large penetration depth and is theoretically formulated in Appendix 7.1 based on the theoretical method of Gurevich [12].

4.1 Pressure distributions of β=30\beta=30^{\circ} caused by the constant speed impact

Refer to caption

Fig. 11: The pressure distributions and free surface of different penetration depths in the transition stage during the water entry of a wedge with β=30\beta=30^{\circ} in a constant speed [25].

The pressure distributions and free surface of different penetration depths in the transition stage during the water entry of a wedge with β=30\beta=30^{\circ} in a constant speed are shown in Fig. 11. It is clearly observed that the high pressure region located at the spray root rapidly vanishes after the spray root leaves the knuckle of the wedge. In the slamming stage, the high pressure region is formed because the water under the wedge has to accumulate in the spray root and turns into a jet with high speed, as the wetted area of wedge keeps increasing. In the transition stage, the wetted length of the wedge stops increasing and the wall surface of the spray root no longer exists, and thus the high pressure region disappears. Fig. 12 shows the pressure distributions on the wedge surface. With the increasing penetration depth, the pressure on the whole wedge surface decreases and finally approaches the distribution of steady supercavitating flow. It is difficult to figure out the way how the pressure drops from the original distribution of slamming stage. In this paper, we focus on the formulation of the force and expect to find a general expression of slamming and transition stages .

Refer to caption

Fig. 12: The pressure distributions on the wedge surface in the transition stage of the water entry of a wedge with β=30\beta=30^{\circ} in a constant speed. The result of steady supercavitating flow is calculated by the potential theory in Appendix 7.1.

4.2 Hydrodynamic force caused by the constant speed impact

Refer to caption

Fig. 13: The slamming coefficient Cs0C_{s0} (aa) and the new variables Cs0C_{s0}^{*} (bb) of different deadrise angles varying from 2525^{\circ} to 4545^{\circ} calculated by the CFD method.

Figure 13 (aa) shows the slamming coefficient Cs0C_{s0} of different deadrise angles varying from 2525^{\circ} to 4545^{\circ}. The Cs0C_{s0} of a single β\beta increases linearly to the maximum CmaxC_{\rm max} and declines to a steady value CsC_{s\infty}. The CsC_{s\infty} of different deadrise angles are shown in Fig. 32 in Appendix 7.1, which is calculated by a potential theory [12]. In order to formulate the slamming coefficient Cs0C_{s0} in the transition stage, new variables are adopted:

h=hh2h2cotλβ,h^{*}=\frac{h-h_{2}}{h_{2}}\cot^{\lambda}\beta, (16)
Cs0=Cs0CsCsmaxCs,C_{s0}^{*}=\frac{C_{s0}-C_{s\infty}}{C_{s\rm max}-C_{s\infty}}, (17)

where h2h_{2} is the penetration depth corresponding to the maximum slamming coefficient CsmaxC_{s\rm max}. The new parameter λ\lambda is determined by a gradient algorithm enforcing on the following function

η(λ)=1Ni=1Nσi2(λ),{\eta}(\lambda)=\frac{1}{N}\sum\limits_{i=1}^{N}{\sigma_{i}^{2}(\lambda)}, (18)

where σi(λ)\sigma_{i}(\lambda) is the standard deviation of Cs0C_{s0}^{*} between different deadrise angles for the ithi^{th} node in the range of h[0,  7]h^{*}\in[0,\,\,7] and thereby becomes a function of λ\lambda. An uniform distribution with NN=7001 nodes in the range of h[0,  7]h^{*}\in[0,\,\,7] is adopted, and the initial values are chosen as λ=1.4\lambda=1.4 and 1.351.35. After 35 steps, the gradient algorithm is convergent with λ=1.3075\lambda=1.3075 (Δλ<\Delta\lambda<1e-6). The Cs0C_{s0}^{*} of different deadrise angles with λ=1.3075\lambda=1.3075 are also shown in Fig. 13 (bb), and it can be seen that the Cs0C_{s0}^{*} of different deadrise angles in the transition stage coincide well with each other.

Refer to caption

Fig. 14: Description of the formulation for the whole process of water entry.

Owing to the linear increasing slamming coefficient in the slamming stage and the coinciding results in the transition stage, the hydrodynamic force of both the slamming and transition stages of water entry can be formulated as shown in Fig. 14, where the slamming stage is in the range of [h1,  0][h_{1}^{*},\,\,0] and the transition stage is in that of [0,+][0,+\infty]. The coinciding Cs0C_{s0}^{*} of Fig. 13 (bb) in the transition stage is formulated by a rational function in h[0,  7]h^{*}\in[0,\,\,7] based on the mean results of the Cs0C_{s0}^{*} of different deadrise angles

Cs0=1.539h+2.618h2+8.081h+2.169.C_{s0}^{*}=\frac{{1.539{h^{*}}+2.618}}{{{h^{*2}}+8.081{h^{*}}+2.169}}. (19)

Due to the fitting errors, Cs0C_{s0}^{*} in Eq. (19) is larger than 1 when h[0,  0.067]h^{*}\in[0,\,\,0.067]. In order to deal with the continuity between Eq. (19) and the linear increasing Cs0C_{s0}^{*} of slamming stage, Cs0C_{s0}^{*} of is approximately as 1 in h[0,  0.067]h^{*}\in[0,\,\,0.067]. The linear increasing Cs0C_{s0}^{*} appears the following form

Cs0=1+Cs0hh.C_{s0}^{*}={1+\frac{{\partial C_{s0}^{*}}}{{\partial{h^{*}}}}{h^{*}}}. (20)

By taking the derivative of Cs0C_{s0}^{*} with respect to hh^{*}, the slope of the linear expression of Eq. (20) in [h1,  0][h_{1}^{*},\,\,0] appears to be

dCs0dh=k1k2tanλβCsmaxCs,\frac{{{\rm d}C_{s0}^{*}}}{{{\rm d}{h^{*}}}}=\frac{{{k_{1}}{k_{2}}{{\tan}^{\lambda}}\beta}}{{{C_{s\max}}-{C_{s\infty}}}}, (21)

where k1=h2/h0k_{1}=h_{2}/h_{0}, k2=dCs0d(h/h0)k_{2}=\frac{{\rm d}C_{s0}}{{\rm d}(h/h_{0})}. Csmax=k1k2C_{s\max}=k_{1}k_{2} according to the definations of k1k_{1} and k2k_{2}. Fig. 15 shows the k1k_{1} and k2k_{2} of various deadrise angles from 15 to 45, which are calculated by the present CFD method. In the Wagner theory, k1=2/πk_{1}={2}/{\pi}. k1k_{1} from CFD results match 2/π2/\pi when β30\beta\leq 30^{\circ}. Thus, k1=2/πk_{1}=2/\pi can be adopted for small deadrise angle. k2k_{2} appears to be equal to B2tanβB_{2}\tan\beta of the similarity solution [22, 39, 21]. The CFD results of k2k_{2} are in good agreement with the similarity solution. In this paper, the results of k1k_{1} and k2k_{2} for an arbitrarily deadrise angle within the range of [15,  45][15^{\circ},\,\,45^{\circ}] are given by a least square fitting method (LSF) of a quadratic function k1=0.2027β20.1295β+0.655{k_{1}}=0.2027{\beta^{2}}-0.1295\beta+0.655 and a quadratic function multiplying cotβ\cot\beta, e.g., k2=(1.585β26.856β+7.764)cotβ{k_{2}}=\left({1.585{\beta^{2}}-6.856\beta+7.764}\right)\cot\beta from the CFD results, and the maximum fitting errors are 0.62%0.62\% and 1.91%1.91\% respectively. Therefore

Cs0={1+Cs0hh,h01,1.539h+2.618h2+8.081h+2.169,0<h0.067h>0.067C_{s0}^{*}=\left\{{\begin{array}[]{*{20}{c}}{1+\frac{{\partial C_{s0}^{*}}}{{\partial{h^{*}}}}{h^{*}},}&{{h^{*}}\leq 0}\\ {\begin{array}[]{*{20}{c}}{1,}\\ {\frac{{1.539{h^{*}}+2.618}}{{{h^{*2}}+8.081{h^{*}}+2.169}},}\end{array}}&{\begin{array}[]{*{20}{c}}{0<{h^{*}}\leq 0.067}\\ {{h^{*}}>0.067}\end{array}}\end{array}}\right. (22)

By combining the Eqs. (16) - (17) and (22), it is possible to find the Cs0C_{s0} value and then the hydrodynamic force acting on the wedge surface (half model) for the cases in a constant speed is given

F=12ρUw2lCs0.F=\frac{1}{2}\rho U_{w}^{2}l{C_{s0}}. (23)

Refer to caption

Fig. 15: The k1k_{1} and k2k_{2} of various deadrise angles from 15 to 45, which are calculated by the present CFD method.

4.3 Comparisons with CFD results

In Sec. 4.2, the formulation of slamming stage in the slamming and transition stages is set up by Eqs. (16)-(17) and (22), and the hydrodynamic force is finally calculated by Eq. (23). The formulation is based on the CFD results in a range of deadrise angles from 1515^{\circ} to 4545^{\circ}. In order to explore its application range of deadrise angles, this section compares the predictions of Eq. (23) and the CFD results in the range of β[5,70]\beta\in[5^{\circ},70^{\circ}].

For the comparisons in β[15,  45]\beta\in[15^{\circ},\,\,45^{\circ}], Fig. 16 shows the comparisons between the predictions of Eq. (23), the modified Wagner’s model (MWM) [25] and the CFD method for the cases of β=15\beta=15^{\circ}, 2525^{\circ} and 4545^{\circ}. The agreement between the present model and the CFD results is good except that a tiny discrepancy occurs at the maximum CsC_{s} for the case of β=45\beta=45^{\circ}. The WMW can only work in the range of β[15,  35]\beta\in[15^{\circ},\,\,35^{\circ}]. For the cases of β=15\beta=15^{\circ} and 2525^{\circ}, the accuracy of the present model and MWM is close.

The comparisons in the ranges of small and large deadrise angles are also provided in Figs. 17 and  18. The agreement between the predictions of Eq. (23) and the CFD results is generally good, though with some discrepancies. Eq. (23) slightly underestimates the force at a large penetration depth for the case of β=5\beta=5^{\circ} and overestimates the forces for the cases of large deadrise angles at an early period of the transition stage. But the agreement becomes better as the penetration depth increases. Therefore, it can be concluded that the present formula can provide accurate predictions for the slamming coefficients of various deadrise angles from 55^{\circ} to 7070^{\circ}.

Since there exists entrainment of air when the deadrise angle is smaller than 55^{\circ} [40, 41], the predictions of force without involvement of the effect of air cushion may be inaccurate. Thus, this paper does not consider the validations of a smaller deadrise angle, and 5β705^{\circ}\leq\beta\leq 70^{\circ} will be a proper range of deadrise angle for most of the engineering applications.

Refer to caption

Fig. 16: The comparisons between the predictions of Eq. (23), the modified Wagner’s model (MWM) [25] and the CFD method for the water entry of linear wedges with deadrise angles of β=15\beta=15^{\circ}, 2525^{\circ} and 4545^{\circ}.

Refer to caption

Fig. 17: The comparisons between the predictions of Eq. (23) and the CFD method for water entry of linear wedges with small deadrise angles of β=5\beta=5^{\circ} and 1010^{\circ}.

Refer to caption

Fig. 18: The comparisons between the predictions of Eq. (23) and the CFD method for water entry of linear wedges with high deadrise angles of β=50\beta=50^{\circ}, 6060^{\circ} and 7070^{\circ}.

5 Varying speed impact

In this section, the varying speed impact of a linear wedge is numerically studied by the HBF method described in Sec. 2.2. The varying speed cases are shown in Tab. 3. The wedges have the same half-width of 1m. All the cases start the varying speed motions at the start time in the slamming stage, which makes sure that the impacts in the transition stage are all in varying speed motions. Cases 1 and 4 have constant decelerations and the other have linear decelerations. In the following simulations of HBF, the growth factor of BEM and FEM panels are 1.03 and 1.04 respectively and the ratio between the normal distance between the two side of the jet in proximity of the spray root (to be honest where the jet model start) and the minimun panel size is 2. The pressure distributions and the force acting on the wedge body are discussed by comparing the results of the constant and varying speed impacts. The formulation of the acceleration effect in the transition stage is proposed and the new expression will be validated by numerical and experiment results and compared with other theories.

β()\beta\,\rm(^{\circ}) U0(m/s)U_{0}\,\rm(m/s) start time (s) aw(m/s2)a_{w}\,\rm(m/s^{2})
Case 1 30 1 0.25 1-1
Case 2 30 1 0.25 -2t+0.2
Case 3 30 1 0.25 2t22t-2
Case 4 15 2 0.06 5-5
Case 5 20 1 0.15 2t+0.3-2t+0.3
Case 6 45 1 0.63 0.5t+0.315-0.5t+0.315
Tab. 3: Details of the cases of varying speed impacts in forced motions. The cases remains the impacts in a constant speed of U0U_{0} before the start time and turn into those of a varying speed with the above accelerations after that. Cases 1 and 4 have constant decelerations and the other have linear decelerations.

5.1 Pressure distributions of β=30\beta=30^{\circ} caused by the acceleration effect

Refer to caption

Fig. 19: The CpC_{p} distributions on the wedge surface in the transition stage of Case 1 (see Tab. 3) (aa) and the distributions of Δp/(0.5ρawc)\Delta p/(0.5\rho a_{w}c), where Δp\Delta p is the difference of the pressure between the varying and constant speed impacts in a same penetration depth and with a same instantaneous speed (bb). The result of similarity solution k1tanβ(2Φ)k_{1}\tan\beta(-2\Phi) is also given for comparisons[36]. The result of h/h0=0.502h/h_{0}=0.502 remains in the slamming stage.

Figure 19 (aa) shows the CpC_{p} distributions on the wedge surface in the transition stage of Case 1 (see Tab. 3). For the case of β=30\beta=30^{\circ}, the transition stage starts at h/h0=0.639h/h_{0}=0.639 and thus the result of h/h0=0.502h/h_{0}=0.502 is still in the slamming stage while the other are in the transition stage. As can be seen in Fig. 19 (aa), the CpC_{p} distributions along the wedge surface decline with the increasing penetration depth. The reasons of the pressure drop includes two different aspects: the vanishing of high pressure region at spray root (see Sec. 3.1) and the deceleration of wedge. In order to distinguish these two kinds of influence, the pressure is split into two parts: (1) the pressure only related to the constant speed impact p0=0.5ρUw2Cp0p_{0}=0.5\rho U_{w}^{2}C_{p0} (see Fig. 12); (2) the pressure changing Δp=pp0\Delta p=p-p_{0} caused by the acceleration of wedge, where p0p_{0} and pp are the pressure of the constant and varying speed impacts respectively in a same penetration depth and with a same instantaneous speed. Fig. 19 (bb) shows the distributions of Δp/(0.5ρawc)\Delta p/\left(0.5\rho a_{w}c\right), where the effective wetted length (half length) is c=min{hcotβ/k1,l}c=\min\left\{{h\cot\beta/{k_{1}},\,\,l}\right\}. The Δp/(0.5ρawc)\Delta p/\left(0.5\rho a_{w}c\right) of different penetration depths show similar distributions and have a small increase along the whole wedge surface with the increasing penetration depth. The result of similarity solution k1tanβ(2Φ)k_{1}\tan\beta(-2\Phi) [36] in the slamming stage is well consistent with the result h/h0=0.502h/h_{0}=0.502 in the slamming stage. It can be concluded that the distribution of Δp/(0.5ρawc)\Delta p/\left(0.5\rho a_{w}c\right) remains as k1tanβ(2Φ)k_{1}\tan\beta(-2\Phi) in the slamming stage and then has a small increase in the transition stage. The results become steady as the penetration depth continues to increase. The small increase pressure will also result in the small increase of slamming coefficient, which will be further discussed in Sec. 5.2.

Refer to caption

Fig. 20: The dimensionless velocity potential 2ϕ/(Uwc)-2\phi/(U_{w}c) on the wedge surface of Case 1 in the transition stage. The result of h/h0=0.502h/h_{0}=0.502 remains in the slamming stage.

From the studies of slamming stage [36, 21], the pressure changing caused by the acceleration of wedge can be quantified by the dimensionless velocity potential 2Φ-2\Phi. Fig. 20 shows the dimensionless velocity potential 2ϕ/(Uwc)-2\phi/\left(U_{w}c\right) (a similar dimensionless variable like 2Φ-2\Phi) on the wedge surface of Case 1 in the transition stage. The 2ϕ/(Uwc)-2\phi/(U_{w}c) distribution of h/h0=0.502h/h_{0}=0.502 is identical to 2Φ-2\Phi of the similarity solution [21] since it still remains in the slamming stage. The other distributions show large differences with 2Φ-2\Phi of the similarity solution and the Δp/(0.5ρawc)\Delta p/\left(0.5\rho a_{w}c\right) distributions in Fig. 19 (bb). It can be concluded that the pressure changing caused by the acceleration of wedge can not be quantified by the velocity potential in the transition stage as it does in the slamming stage. Although the Δp/(0.5ρawc)\Delta p/\left(0.5\rho a_{w}c\right) distributions have a similar distribution and small increase as the penetration depth increases, there is still some challenging problems to formulate the pressure changing caused by the acceleration effect. In this paper, we focus on the formulation of the hydrodynamic force caused by the acceleration effect and hope to find an effective method to formulate the hydrodynamic force caused by the acceleration effect.

5.2 Hydrodynamic force caused by the acceleration effect

Refer to caption

Fig. 21: The time histories of ΔF/(0.5ρc2aw)\Delta F/(0.5\rho c^{2}a_{w}) of different prescribed speeds (Case 1, Case 2 and Case 3 in Tab. 3), where ΔF\Delta F is difference of force between the varying and constant speed impacts in a same penetration depth and with a same instantaneous speeds. The results of Ca0=A2(k1tanβ)2C_{a0}=A_{2}(k_{1}\tan\beta)^{2} from the similarity solution [36] and Eq. (26) from Tassin et al. [23] are also given for comparisons.

Similar to the pressure distribution on the wedge surface, the force can also be divided into two part: (1) the force caused by the constant speed impact F0=0.5ρUw2lCs0F_{0}=0.5\rho U_{w}^{2}lC_{s0}, where Cs0C_{s0} can be given by Eqs. (16) - (17) and (22); (2) the force caused by the acceleration effect ΔF=FF0\Delta F=F-F_{0}, where F0F_{0} and FF are the forces of constant and varying speed impacts respectively in a same penetration depth and with a same instantaneous speed. Fig. 21 shows the ΔF/(0.5ρc2aw)\Delta F/(0.5\rho c^{2}a_{w}) of different prescribed speeds (Cases 1,2 and 3 in Tab. 3). All of the cases are decelerating with different decelerations. Case 1 has a constant deceleration, Case 2 has an increasing deceleration and Case 3 has a decreasing deceleration. The ΔF/(0.5ρc2aw)\Delta F/(0.5\rho c^{2}a_{w}) show good consistence between different cases in the transition stage of h/h0[0.639  1.0]h/h_{0}\in[0.639\,\,1.0], though with some numerical fluctuations. Therefore, Ca=ΔF/(0.5ρc2aw)C_{a}=\Delta F/(0.5\rho c^{2}a_{w}) is defined as an added mass coefficient, and independent of awa_{w} in h/h0[0.639  1.0]h/h_{0}\in[0.639\,\,1.0]. It can be concluded that the effects of acceleration on the hydrodynamic force have a fixed pattern in the transition stage as it does in the slamming stage [21]. In the slamming stage, the acceleration effect on the hydrodynamic force is given as ΔF=ρA2awh2\Delta F=\rho A_{2}a_{w}h^{2} from the similarity solution [36], indicating an added mass coefficient Ca0=A2(k1tanβ)2C_{a0}=A_{2}(k_{1}\tan\beta)^{2}. The CaC_{a} in the slamming stage can be given as Ca0=1.0459C_{a0}=1.0459, and in the transition stage, CaC_{a} has an averaged result of 1.3297 in h/h0[0.639  1.0]h/h_{0}\in[0.639\,\,1.0], which is ξ=27.13%\xi=27.13\% larger than the result of similarity solution Ca0C_{a0}. In this paper, a hybrid added mass coefficient is adopted to formulate the acceleration effect corresponding to Eq. (22)

Ca={Ca0,h0(1+ξh/0.067)Ca0,(1+ξ)Ca00<h0.067h>0.067{C_{a}}=\left\{{\begin{array}[]{*{20}{c}}{{C_{a0}},}&{{h^{*}}\leq 0}\\ {\begin{array}[]{*{20}{c}}{(1+\xi{h^{*}}/0.067){C_{a0}},}\\ {(1+\xi){C_{a0}}}\end{array}}&{\begin{array}[]{*{20}{c}}{0<{h^{*}}\leq 0.067}\\ {{h^{*}}>0.067}\end{array}}\end{array}}\right. (24)

The results of h[0, 0.067]h^{*}\in[0,\,0.067] are given by a linear distribution from Ca0C_{a0} to (1+ξ)Ca0(1+\xi)C_{a0}. For the case of β=30\beta=30^{\circ}, the approximation of CaC_{a} in the transition stage is summarized from the HBF results of h/h0[0.639, 1.0]h/h_{0}\in[0.639,\,1.0], corresponding to h[0, 1.1586]h^{*}\in[0,\,1.1586]. However, further validations of Eq. (24) by the numerical results in Sec. 5.3 indicates that Eq. (24) can work in a larger range of hh^{*} and deadrise angles. Therefore, for the water entry of linear wedges with an acceleration, the hydrodynamic force can be predicted by Eq. (24) together with Eqs. (16) - (17) and (22), and the final expression of the force (half model) has the following form:

F=12ρUw2lCs0+12ρc2awCa,F=\frac{1}{2}\rho U_{w}^{2}l{C_{s0}}+\frac{1}{2}\rho{c^{2}}{a_{w}}{C_{a}}, (25)

where c=min{hcotβ/k1,l}c=\min\left\{{h\cot\beta/{k_{1}},\,\,l}\right\}.

In the linear FBC of Tassin et al. [23] based on MLM, the acceleration effect was addressed by the following form of CaC_{a} of in the slamming and transition stages

Ca={π2+(14π)tanβ,hh02ππ2+(12hh0)tanβ,π2tanβ.2π<hh01hh0>1{C_{a}}=\left\{{\begin{array}[]{*{20}{c}}{\frac{\pi}{2}+\left({1-\frac{4}{\pi}}\right)\tan\beta,}&{\frac{h}{{{h_{0}}}}\leq\frac{2}{\pi}}\\ {\begin{array}[]{*{20}{c}}{\frac{\pi}{2}+\left({1-\frac{{2h}}{{{h_{0}}}}}\right)\tan\beta,}\\ {\frac{\pi}{2}-\tan\beta.}\end{array}}&{\begin{array}[]{*{20}{c}}{\frac{2}{\pi}<\frac{h}{{{h_{0}}}}\leq 1}\\ {\frac{h}{{{h_{0}}}}>1}\end{array}}\end{array}}\right. (26)

As can be seen in Fig. 21, the present model has a different CaC_{a} from that of Tassin et al. [23].

5.3 Validations by numerical and experiment results

Figure 22 shows the comparisons of the forces acting on the wedge surface between the present predictions and the HBF results for Case 1, 2 and 3. The results of Eq. (23) only include the effect of constant speed impact while those of Eqs. (25) include the effect of constant speed impact and the acceleration effect. The predictions of Eqs. (25) are in good agreement with the HBF results, while those of Eqs. (23) show much discrepancies with the HBF results. Fig. 23 shows comparisons for Case 4, 5 and 6 of different deadrise angles and different ways of decelerations. The same CaC_{a} correction of ξ=27.13%\xi=27.13\% is adopted for the cases of different deadrise angles, and the good agreement is also obtained. It indicates that the CaC_{a} correction of ξ=27.13%\xi=27.13\% also works for other deadrise angles.

Refer to caption

Fig. 22: The comparisons of the forces acting on the wedge surface between the present predictions and the HBF results for Case 1, 2 and 3.

Refer to caption

Fig. 23: The comparisons of the forces acting on the wedge surface between the present predictions and the HBF results for Case 4, 5 and 6.

To explore the application ranges of deadrise angles and of different ways of wedge motions for the present model, Fig. 24 shows the comparisons of the forces acting on the wedge surface between the present predictions and the CFD results for the freefall cases of (aa) β=5\beta=5^{\circ} and β=70\beta=70^{\circ}. The wedges are in freefall motions with masses of m=1.5ρl2m=1.5\rho l^{2}. For the small and high deadrise angles, the present model can provide good predictions for the hydrodynamic forces, even for the freefall motions where the acceleration of wedge is unknown before the predictions.

Refer to caption

Fig. 24: The comparisons of the forces acting on the wedge surface between the present predictions and the CFD results for the freefall cases of (aa) β=5\beta=5^{\circ} and (bb) β=70\beta=70^{\circ} with masses of m=1.5ρl2m=1.5\rho l^{2}.

The case in Fig. 10 is also used for a validation for the present model. Fig. 25 shows the comparisons of the predictions of accelerations of wedge with β=30\beta=30^{\circ} between the CFD without gravity of fluid, BEM of Bao et al. [32] with gravity of fluid, theory of Wen et al. [21] without considering the transition stage, Eq. (23) and Eq. (25) during the water entry in freefall motion. The agreement between the CFD result and the present model with acceleration effect, e.g., Eq. (25), is good in both slamming and transition stages, while the theory of approximate solution without considering the transition stage [21] can only address the slamming stage. The present model without acceleration effect, e.g., Eq. (23), also shows large differences compared with the CFD result. The gravity effect has small influence on the hydrodynamic force in the transition stage for the cases of Fr=1.9587Fr=1.9587. For the high speed impact of higher FrFr, the gravity of fluid can be neglected and the present model will have better predictions.

Refer to caption

Fig. 25: The comparisons of the predictions of accelerations of wedge with β=30\beta=30^{\circ} between the CFD without gravity of fluid, BEM of Bao et al. [32] with gravity of fluid, theory of Wen et al. [21] without considering the transition stage, Eqs. (23) and  (25) during the water entry in freefall motion.

Refer to caption


Fig. 26: The comparisons between the present predictions of forces and the experimental result of Zhao et al. [13] for the water entry of a wedge of β=30\beta=30^{\circ}. The vertical velocity of the wedge is given by the experimental result of an optical sensor. The force coefficient of 3D effect is approximately formulated as a parabolic f3D=10.80(c/l)2f_{\rm 3D}=1-0.80(c/l)^{2} by using Meyerhoff’s results [42].

A comparison of the forces between an experimental test of Zhao et al. [13] and the present model is shown in Fig. 26. The case is a three-dimensional water entry with deadrise angle of β=30\beta=30^{\circ}. The half width of wedge is l=0.25ml=0.25\,\rm m and the thickness is L=1mL=1\,\rm m. The vertical speed of the wedge is given by the experimental result of an optical sensor. The acceleration of wedge is given by the derivative of vertical speed. The present 2D model has large discrepancies compared with the experimental result. As Zhao et al. indicated, the reason is due to the three dimensional (3D) effect and the force should be corrected by a force coefficient f3Df_{\rm 3D} (a function of c/Lc/L). They used Meyerhoff’s results [42] of f3D(0.25)=0.95f_{\rm 3D}(0.25)=0.95, f3D(0.4)=0.87f_{\rm 3D}(0.4)=0.87, f3D(0.5)=0.8f_{\rm 3D}(0.5)=0.8 from the added masses of thin rectangular plates with a generalization of Wagner theory to formulate the 3D effect. In this paper, a parabolic f3D=10.80(c/L)2f_{\rm 3D}=1-0.80(c/L)^{2} is approximately formulated by fitting from the above results. After using the 3D correction, the present model with 3D effect can predict the force of the experimental test.

To sum up, Eq. (25) together with Eqs. (16), (17), Eq. (24) and (22) can be used for both the predictions of hydrodynamic force in slamming and transition stages for the water entry of wedges with different deadrise angles in constant and varying speeds.

5.4 Comparisons with other theories

For the slamming stage, the traditional added mass methods have the forms of added mass and the hydrodynamic force (half model)

m0=12ρc2Ca,m_{0}=\frac{1}{2}\rho{c^{2}}{C_{a}}, (27)
F=d(m0Uw)dt=12ρUw2hcot2βCconst+12ρc2awCa,F=\frac{{{\rm{d}}({m_{0}}{U_{w}})}}{{{\rm{d}}t}}=\frac{1}{2}\rho U_{w}^{2}h{\cot^{2}}\beta{C_{{\rm{const}}}}+\frac{1}{2}\rho{c^{2}}{a_{w}}{C_{a}}, (28)

where c=γhcotβc=\gamma h\cot\beta for the traditional methods. Tab. 4 shows the correction factor γ\gamma of the wetted length, the dimensionless coefficient of constant speed impact CconstC_{\rm const} and the added mass coefficient CaC_{a} of slamming stage for different theories [4, 5, 17, 19, 23]. The Wagner’s new model [5] was proposed to improve the predictions of forces of constant speed impact for different deadrise angles, but the acceleration term remained unchanged. γMei\gamma_{\rm Mei} can be found in Refs.  [19, 21]. B2MeiB_{2\rm Mei} and A2MeiA_{2\rm Mei} are calculated by direct pressure and velocity potential integrations of Mei et al.’s model [19]. CKorobkinC_{\rm Korobkin} is from the theoretical results of Korobkin [20]. B2B_{2} and A2A_{2} of the present model were calculated from the similarity solution [22], and the results are shown in Ref. [21].

Model γ\gamma CconstC_{\rm const} CaC_{a}
Von Karman [4] 1 π\pi 1
Wagner’s original model [5] π2\frac{\pi}{{2}} π34\frac{\pi^{3}}{4} π2\frac{\pi}{{2}}
Wagner’s new model [5] π2\frac{\pi}{{2}} π(π2β1)2tan2β\pi{\left({\frac{\pi}{{2\beta}}-1}\right)^{2}}\tan^{2}\beta π2\frac{\pi}{{2}}
Faltinsen [17] π2\frac{\pi}{{2}} π34(1β2π)2\frac{\pi^{3}}{4}(1-\frac{\beta}{{2\pi}})^{2} π2(1β2π)2\frac{\pi}{2}(1-\frac{\beta}{{2\pi}})^{2}
Mei et al. [19] γMei\gamma_{\rm Mei} B2Meitan2βB_{2\rm Mei}\tan^{2}\beta A2Mei(tanβ/γMei)2A_{2\rm Mei}(\tan\beta/\gamma_{\rm Mei})^{2}
Tassin et al. [23] π2\frac{\pi}{{2}} CKorobkinC_{\rm Korobkin} π2(4π1)tanβ\frac{\pi}{2}-\left({\frac{4}{\pi}-1}\right)\tan\beta
Present model 1k1\frac{1}{k_{1}} B2tan2βB_{2}\tan^{2}\beta A2(k1tanβ)2A_{2}(k_{1}\tan\beta)^{2}
Tab. 4: The correction factor γ\gamma of the wetted length, the dimensionless coefficient of constant speed impact CconstC_{\rm const} and the added mass coefficient CaC_{a} of slamming stage for different theories.

Refer to caption

Fig. 27: The comparisons of the dimensionless coefficient of (aa) constant speed impact CconstC_{\rm const} and (bb) added mass coefficient CaC_{a} of the slamming stage between the present model and other theories [4, 5, 17, 19, 23].

In early researches of Refs. [4, 5, 17, 19, 20] for the slamming stage, the hydrodynamic force of constant speed impact received the most attention and the researchers proposed their models by comparing the results of similarity solution [22, 16] to correct the underestimated results of Von Karman [4] and overestimated results of Wagner’s original model [5], as shown in Fig. 27 (aa). The models of Mei et al. [19], Tassin et al. [23] and Wagner’s new model [5] have been approximately close to the results of similarity solution, but these models actually violate the framework of added mass methods. Their CconstC_{\rm const} are no longer 2Caγ22C_{a}\gamma^{2}, which are different from the models of Von Karman [4], Wagner [5] (original model) and Faltinsen [17]. Although these models [19, 23, 5] brought good predictions for the constant speed impact, they still can not properly model the acceleration effect, as shown in Fig. 27 (bb). The Faltinsen’s model cannot properly address both the constant speed impact and acceleration effect. The present model formulates the models of constant speed impact and acceleration effect directly from the approximate solution [21] based on the similarity solution of Dobrovol’skaya [22], regardless of the framework of added mass methods and the consistency of CconstC_{\rm const} and CaC_{a}. The validations by numerical results in Ref. [21] and Figs. 22 and 23 have completely verified the present model.

For the transition stage, Tassin et al.’s model [23], the MWM of Wen et al. [25] and the present model can address both the slamming and transition stages, while the models of Ref. [4, 5, 17, 19] can only work in the slamming stage. Wen et al. had greatly improved the predictions of hydrodynamic forces for the constant speed impact in the range of β[15,  35]\beta\in[15^{\circ},\,\,35^{\circ}] compared with the linear FBC of Tassin et al. and the improved model of zero pressure condition [18, 23]. The accuracy of present model is close to Wen et al.’s MWM, but with a much larger range of deadrise angle. Besides, the acceleration effect in the transition stage is missing in MWM. Tassin et al.’s model provided the formulation of acceleration effect and the CaC_{a} is given by Eq. (26). The comparison of CaC_{a} of β=30\beta=30^{\circ} between the present model and Tassin et al.’s model is shown in Fig. 27 (bb). In contrast to an increase of CaC_{a} in the transition stage, the CaC_{a} of Tassin et al.’s model declines and finally reaches a constant value lower than Ca0C_{a0}, which is inconsistent with the HBF results in Fig. 27 (bb).

In general, we rewrite the formula of hydrodynamic force and extend it to the transition stage for the constant and varying speed impacts. Although the present model is more sophisticated, it works better than the traditional added mass methods and the asympotic theories and can work in a larger range of deadrise angle.

6 Conclusions

In this paper, the transition stage of the water entry of a linear wedge with constant and varying speeds is numerically studied by FVM with VOF and HBF. The hydrodynamic force acting on the wedge is formulated by a combination of the numerical results and theoretical results of the steady supercavitating flow. The fluid is assumed to be incompressible, inviscid, weightless and with negligible surface tension, and the flow is irrotational for the high speed impact. For the constant speed impact, the similitude of the slamming coefficients of different deadrise angles in the transition stage is found by scaling the difference between the maximum values in the slamming stage and the results of steady supercavitating flow. The formulation of the hydrodynamic force is conducted based on the similitude of the declining forces in the transition stage together with the linear increasing results in the slamming stage. For the varying speed impact, the acceleration effects on the pressure distribution and force acting on the wedge surface are revealed. The hydrodynamic force caused by the acceleration effect in the transition stage is formulated by an added mass coefficient with an averaged increase of 27.13%27.13\% compared with that of slamming stage. A general expression of the slamming coefficient with the deadrise angles from 55^{\circ} to 7070^{\circ} in both the slamming and transition stages is thus proposed for the constant and varying speed impacts, and its predictions are in good agreement with the numerical and experiment results. Thus, it can be treated as a 2D water entry model the 2.5D method being used on the take-off and water landing of seaplanes, and for the strip theory or 2D+t theory being used on the hull slamming.

Acknowledgements

This work was partially supported by the National Natural Science Foundation of China (No. 12072014 and No. 11721202).

7 Appendix

7.1 The theory of steady supercavitating flow

The water entry in the infinite penetration depth becomes a steady supercavitating flow with an incoming currency with velocity v0v_{0}. The theory can be extended from the water entry on a plate by the theory of Gurevich [12]. The free surface CD and CD\rm C^{\prime}D^{\prime} of impact flow is shown in Fig. 28 after the solution is solved. The direction of incoming flow is upward and the stream-function on the streamline passing A is 0. The velocity potential at A is chosen as 0. A parameter plane τ\tau mapping to the geometry in Fig. 28 is shown in Fig. 29 and thus the complex velocity potential of impact flow can be calculated as

w=ϕ0τ2,w=\phi_{0}\tau^{2}, (29)

Refer to caption

Fig. 28: Free surface of the steady supercavitating flow for a 2D wedge of β=30\beta=30^{\circ}.

Refer to caption

Fig. 29: The τ\tau plane of the steady supercavitating flow.

where ϕ0\phi_{0} is the velocity potential at C and CC^{\prime}. Another parameter plane ω=v0dzdw=v0eiθ/v\omega=v_{0}\frac{{\rm d}z}{{\rm d}w}=v_{0}e^{{\rm i}\theta}/v (i\rm i being the imaginary unit) mapping to the velocity is shown in Fig. 30 and can be formulated by the Schwarz-Christoffel formula as

ω(τ)=(12βπ)ln(11/τ2+iτ)+iπ2.\omega\left(\tau\right)=\left({1-\frac{{2\beta}}{\pi}}\right)\ln\left({\sqrt{1-1/{\tau^{2}}}+\frac{{\rm{i}}}{\tau}}\right)+{\rm{i}}\frac{\pi}{2}. (30)

The complex coordinate can be derived

z=dzdwdwdτdτ=2ϕ0v0i(11/τ2+iτ)12βπτdτ.z=\int{\frac{{{\rm{d}}z}}{{{\rm{d}}w}}}\frac{{{\rm{d}}w}}{{{\rm{d}}\tau}}{\rm{d}}\tau=\frac{{2{\phi_{0}}}}{{{v_{0}}}}{\rm{i}}\int{{{\left({\sqrt{1-1/{\tau^{2}}}+\frac{{\rm{i}}}{\tau}}\right)}^{1-\frac{{2\beta}}{\pi}}}}\tau{\rm{d}}\tau. (31)

By considering the distance from A to C, the velocity potential at C and CC^{\prime} can be determined

2ϕ0v0=lAcosβ,\frac{{2{\phi_{0}}}}{{{v_{0}}}}=\frac{l}{{A\cos\beta}}, (32)

where

A=01(1+1τ2τ)12βπτdτA={\int_{0}^{1}{\left({\frac{{1+\sqrt{1-{\tau^{2}}}}}{\tau}}\right)}^{1-\frac{{2\beta}}{\pi}}}\tau{\rm{d}}\tau (33)

Refer to caption

Fig. 30: The ω\omega plane of the steady supercavitating flow.

Therefore, the xx on AC is given as

x(τ)=lA0τ(1+1τ2τ)12βπτdτ,x\left(\tau\right)=\frac{l}{A}{\int_{0}^{\tau}{\left({\frac{{1+\sqrt{1-{\tau^{2}}}}}{\tau}}\right)}^{1-\frac{{2\beta}}{\pi}}}\tau{\rm{d}}\tau, (34)

and the velocity on AC is

v=v0(11τ2τ)12βπv={v_{0}}{\left({\frac{{1-\sqrt{1-{\tau^{2}}}}}{\tau}}\right)^{1-\frac{{2\beta}}{\pi}}} (35)

The pressure coefficient CpC_{p} has the form

Cp=1(11τ2τ)2(12βπ).{C_{p}}=1-{\left({\frac{{1-\sqrt{1-{\tau^{2}}}}}{\tau}}\right)^{2\left({1-\frac{{2\beta}}{\pi}}\right)}}. (36)

Refer to caption

Fig. 31: The CpC_{p} distributions of different deadrise angles for the steady supercavitating flow.

The CpC_{p} distributions of different deadrise angles β\beta are shown in Fig. 31. The CpC_{p} is 1 at the stagnation A and 0 at the separation C for a steady supercavitating flow. The free surface profile in Fig. 28 is given by the following xx and yy expressions

x(τ)=llAcosβRe[i1τ(11/τ2+iτ)12βπτdτ],x\left(\tau\right)=l-\frac{l}{{A\cos\beta}}{\rm{Re}}\left[{{\rm{i}}{{\int_{1}^{\tau}{\left({\sqrt{1-1/{\tau^{2}}}+\frac{{\rm{i}}}{\tau}}\right)}}^{{}^{1-\frac{{2\beta}}{\pi}}}}\tau{\rm{d}}\tau}\right], (37)
y(τ)=ltanβ+lAcosβIm[i1τ(11/τ2+iτ)12βπτdτ].y\left(\tau\right)=l\tan\beta+\frac{l}{{A\cos\beta}}{\rm{Im}}\left[{{\rm{i}}{{\int_{1}^{\tau}{\left({\sqrt{1-1/{\tau^{2}}}+\frac{{\rm{i}}}{\tau}}\right)}}^{{}^{1-\frac{{2\beta}}{\pi}}}}\tau{\rm{d}}\tau}\right]. (38)

The force acting on the wedges is calculated by integrating the pressure with the CpC_{p} expression Eq. (36). The slamming coefficient CsC_{s\infty} of different deadrise angles is shown in Fig. 32. The result of β=0\beta=0 is equal to 0.88, which is consistent with that of water entry on a plate derived by Gurevich [12]. The CsC_{s\infty} decreases with the increasing deadrise angle and reaches 0 at β=90\beta=90^{\circ}.

Refer to caption

Fig. 32: The slamming coefficient CsC_{s\infty} of the steady supercavitating flow.

Korvin-Kroukovsky and Chabrow [11] in 1948 had already presented the calculation of pressure distribution on the wedge surface. The present theory is consistent with their model.

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