Wave Forces on a Body

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Wave Forces on a Body

 U = \omega A \,
 R_e = \frac{U\ell}{\nu} = \frac{\omega A \ell}{\nu} \,
 K_C = \frac{UT}{\ell} = \frac{A\omega T}{\ell} = 2 \pi \frac{A}{\ell} \,
 C_F = \frac{F}{\rho g A \ell^2} = f \left( \frac{}{} \right.  \underbrace{\frac{A}{\lambda}} \,,  \underbrace{\frac{\ell}{\lambda}} \, ,  R_e \, ,  \frac{h}{\lambda} \, , roughness,  \ldots \left. \frac{}{} \right) \,
Wave Diffraction
steepness parameter

Type of Forces

1. Viscous forces Form drag, viscous drag  = f ( R_e, K_c, \, roughness,  \ldots ) .

  • Form drag  ( C_D ) \,

Associated primarily with flow separation -normal stresses.

  • Friction drag  ( C_F ) \,
Associated with skin friction  \tau_w, \ i.e., \ \,  \vec{F} \sim \iint \tau_w \,  dS \, .
body
(wetted surface)

2. Inertial forces Froude-Krylov forces, diffraction forces, radiation forces.

Forces arising from potential flow wave theory,

 \vec{F} = \iint p \hat{n} \,  dS \, , where  \ p = - \rho \left( \frac{\partial\phi}{\partial t} + g y \right. \,  + \left. \underbrace{ \frac{1}{2} \left| \nabla \phi \right|^2} \right) \,
body  =0 \, , for linear theory,
(wetted surface) small amplitude waves

For linear theory, the velocity potential  \phi \, and the pressure  p \, can be decomposed to

 \phi = \,  \underbrace{\phi_I} \,  + \,  \underbrace{\phi_D} \,  + \,  \underbrace{\phi_R} \,
Incident wave Scattered wave Radiated wave
potential  (a) \, potential  (b.1) \, potential  (b.2) \,
 - \frac{p}{\rho} = \,  \frac{\partial\phi_I}{\partial t} \,  + \,  \frac{\partial\phi_D}{\partial t} \,  + \,  \frac{\partial\phi_R}{\partial t} \,  + \,
 g y \,

(a) Incident wave potential

  • Froude-Krylov Force approximation When  \ell \ll \lambda \, , the incident wave field is not significantly modified by the presence of the body, therefore ignore  \phi_D \, and  \phi_R \, . Froude-Krylov approximation:
 \left. \begin{matrix} & \phi \approx \phi_I \\ & p \approx - \rho \left( \frac{\partial\phi_I}{\partial t} + g y \right) \end{matrix} \right\}  \Rightarrow \vec{F}_{FK} = \,  \iint \underbrace{- \rho \left( \frac{\partial\phi_I}{\partial t} + g y \right)}  \hat{n} dS \leftarrow \, can calculate knowing (incident)
wave kinematics (and body geometry)
body  . \qquad \equiv p_I \,
surface
  • Mathematical approximation After applying the divergence theorem, the  \vec{F}_{FK} \, can be rewritten as
 \vec{F}_{FK} \,   = - \iint p_I \hat{n} \,  dS = - \iiint \nabla p_I d\forall \,
body
surface
body
volume

If the body dimensions are very small comparable to the wave length, we can assume that  \nabla_{p_I} \, is approximately constant through the body volume  \forall \, and 'pull' the  \nabla_{p_I} \, out of the integral. Thus, the  \vec{F}_{FK} \, can be approximated as

 \vec{F}_{FK} \cong \left( - \nabla_{p_I} \right) \left. \frac{}{} \right| \, at body  \iiint d\forall = \,  \underbrace{\forall} \,  \left( - \nabla_{p_I} \right) \left. \frac{}{} \right| \, at body
center body
volume
body
volume
center

The last relation is particularly useful for small bodies of non-trivial geometry for 13.021, that is all bodies that do not have a rectangular cross section.

(b) Diffraction and Radiation Forces

(b.1) Diffraction or scattering force When  \ell \not\ll \lambda \, , the wave field near the body will be affected even if the body is stationary, so that no-flux B.C. is satisfied.

 \vec{F}_D \ = \  \iint - \rho \left( \frac{\partial\phi_D}{\partial t} \right) \hat{n} dS
body surface

(b.2) Radiation Force -added mass and damping coefficient Even in the absence of an incident wave, a body in motion creates waves and hence inertial wave forces.

 \vec{F}_R = \,  \iint - \rho \left( \frac{\partial\phi_R}{\partial t} \right) \hat{n} dS = -  \underbrace{m_{ij}} \,  \dot{U}_j \ - \,  \underbrace{d_{ij}} \,  U_j \,
body surface added mass wave radiation damping

Important parameters

 (1) K_C = \frac{UT}{\ell} = 2 \pi \frac{A}{\ell} \,  \left. \begin{matrix}  \\  \\ \\ \\ \\ \\ \end{matrix} \right\} \, Interrelated through maximum wave steepness
 \frac{A}{\lambda} \leq 0.07 \,
(2)diffraction parameter  \frac{\ell}{\lambda} \,  \left( \frac{A}{\ell} \right) \left( \frac{\ell}{\lambda} \right) \leq 0.07 \,
  • If  K_c \leq 1 \, : no appreciable flow separation, viscous effect confined to boundary layer (hence small), solve problem via potential theory. In addition, depending on the value of the ratio  \frac{\ell}{\lambda} \, ,
  • If  \frac{\ell}{\lambda} \ll 1 \, , ignore diffraction , wave effects in radiation problem (i.e.,  d_{ij} \approx 0, \ m_{ij} \approx m_{ij} \, infinite fluid added mass). F-K approximation might be used, calculate  \vec{F}_{FK} \, .
  • If  \frac{\ell}{\lambda} \gg 1/5 \, , must consider wave diffraction, radiation  \left( \frac{A}{\ell} \leq \frac{0.07}{\ell / \lambda} \leq 0.035 \right) \, .
  • If  K_C \gg 1 \, : separation important, viscous forces can not be neglected. Further on if  \frac{\ell}{\lambda} \leq \frac{0.07}{A/\ell} \, so 
\frac{\ell}{\lambda} \ll 1 \, ignore diffraction, i.e., the Froude-Krylov approximation is valid.
 F = \frac{1}{2} \rho \ell^2 \,  \underbrace{U(t)} \,  \left| U(t) \right| C_D \left( R_e \right) \,
relative velocity
  • Intermediate  K_c - \, both viscous and inertial effects important, use Morrison's formula.
 F= \frac{1}{2} \rho \ell^2 U(t) \left| U(t) \right| C_D \left( R_e \right) + \rho \ell^3 \dot{U} C_m \left( R_e, K_C \right)
  • Summary

I. Use:  C D \, and  F - K \, approximation.

II. Use:  C F \, and  F - K \, approximation.

III.  C D \, is not important and  F - K \, approximation is not valid.



This article is based on the MIT open course notes and the original article can be found here.

Marine Hydrodynamics

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