next up previous [pdf]

Next: Finite-difference approach Up: Fomel: Velocity continuation Previous: Introduction

Numerical velocity continuation in the post-stack domain

The post-stack velocity continuation process is governed by a partial differential equation in the domain, composed by the seismic image coordinates (midpoint $x$ and vertical time $t$) and the additional velocity coordinate $v$. Neglecting some amplitude-correcting terms (Fomel, 2003), the equation takes the form (Claerbout, 1986)

\begin{displaymath}
{\frac{\partial^2 P}{\partial v  \partial t}} +
{v t \frac{\partial^2 P}{\partial x^2}} = 0\;.
\end{displaymath} (1)

Equation (1) is linear and belongs to the hyperbolic type. It describes a wave-type process with the velocity $v$ acting as a propagation variable. Each constant-$v$ slice of the function $P(x,t,v)$ corresponds to an image with the corresponding constant velocity. The necessary boundary and initial conditions are
\begin{displaymath}
\left.P\right\vert _{t=T} = 0\;\quad \left.P\right\vert _{v=v_0} = P_0 (x,t)\;,
\end{displaymath} (2)

where $v_0$ is the starting velocity, $T=0$ for continuation to a smaller velocity and $T$ is the largest time on the image (completely attenuated reflection energy) for continuation to a larger velocity. The first case corresponds to ``modeling'' (demigration); the latter case, to seismic migration.

Mathematically, equations (1) and (2) define a Goursat-type problem (Courant and Hilbert, 1989). Its analytical solution can be constructed by a variation of the Riemann method in the form of an integral operator (Fomel, 2003,1994):

\begin{displaymath}
P(t,x,v) = {\frac{1}{(2 \pi)^{m/2}}} \int 
{\frac{1}{(...
...2}
P_0\left(\frac{\rho}{\sqrt{v^2-v_0^2}},x_0\right) dx_0\;,
\end{displaymath} (3)

where $\rho = \sqrt{(v^2-v_0^2) t^2 + (x - x_0)^2}$, $m=1$ in the 2-D case, and $m=2$ in the 3-D case. In the case of continuation from zero velocity $v_0=0$, operator (3) is equivalent (up to the amplitude weighting) to conventional Kirchoff time migration (Schneider, 1978). Similarly, in the frequency-wavenumber domain, velocity continuation takes the form
\begin{displaymath}
\hat{P} (\omega,k,v) = \hat{P}_0 (\sqrt{\omega^2+k^2 (v^2-v_0^2)},k)\;,
\end{displaymath} (4)

which is equivalent (up to scaling coefficients) to Stolt migration (Stolt, 1978), regarded as the most efficient constant-velocity migration method.

If our task is to create many constant-velocity slices, there are other ways to construct the solution of problem (1-2). Two alternative approaches are discussed in the next two subsections.


Subsections
next up previous [pdf]

Next: Finite-difference approach Up: Fomel: Velocity continuation Previous: Introduction

2013-03-03