Difference between revisions of "Green Function Solution Method"

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boundary conditions at infinite ([[Sommerfeld Radiation Condition]])
 
boundary conditions at infinite ([[Sommerfeld Radiation Condition]])
  
= [[Standard Linear Scattering Problem]] =
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= [[Standard Linear Wave Scattering Problem]] =
  
We begin with the [[Standard Linear Scattering Problem]]  
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We begin with the [[Standard Linear Wave Scattering Problem]]  
 
<center><math>
 
<center><math>
 
\nabla^{2}\phi=0, \, -\infty<z<0,\,\,\,\mathbf{x}\notin \Omega
 
\nabla^{2}\phi=0, \, -\infty<z<0,\,\,\,\mathbf{x}\notin \Omega
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</math></center>
 
</math></center>
  
We then use Green's Forumla
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We then use [http://en.wikipedia.org/wiki/Green's_identities Green's second identity]
 
[[Category:Linear Water-Wave Theory]]
 
[[Category:Linear Water-Wave Theory]]

Revision as of 12:01, 12 March 2007

Introduction

The use of the Free-Surface Green Function to solve the Standard Linear Wave Scattering Problem has proved one of the most powerful methods, primarily because of its very general nature so that it can deal with complicated boundary conditions. It also solves explicity for the boundary conditions at infinite (Sommerfeld Radiation Condition)

Standard Linear Wave Scattering Problem

We begin with the Standard Linear Wave Scattering Problem

[math]\displaystyle{ \nabla^{2}\phi=0, \, -\infty\lt z\lt 0,\,\,\,\mathbf{x}\notin \Omega }[/math]
[math]\displaystyle{ \frac{\partial\phi}{\partial z}=0, \, z=h, }[/math]
[math]\displaystyle{ \frac{\partial\phi}{\partial z} = k_{\infty}\phi,\,z=0,\,\,\mathbf{x}\notin\Omega, }[/math]
[math]\displaystyle{ \frac{\partial\phi}{\partial z} = L\phi, \, z\in\partial\Omega, }[/math]

We then use Green's second identity