previous up next print clean
Next: Inverse problem Up: THEORY Previous: THEORY

Forward problem

To begin, I define a forward model for a ``generalized'' PP reflectivity, $R_{_{P\!P}}$, which combines elements of Zoeppritz plane wave reflection (e.g., Aki and Richards, 1980), and Rayleigh-Sommerfeld diffraction (e.g., Goodman, 1968). I define a differential volume element $R_{_{P\!P}}$ as

 
 \begin{displaymath}
R_{_{P\!P}}= \frac{iw}{\alpha} \grave{P}\!\acute{P}\cos\phi_s\cos\phi_r \;,\end{displaymath} (1)

for $\vert \phi_s, \phi_r \vert \le \pi/2$, and zero otherwise. Here, w is angular frequency, $\alpha$ is compressional velocity, $\grave{P}\!\acute{P}$ is the Zoeppritz PP plane wave reflection coefficient and $\phi_s$ ($\phi_r$) is the angle between the incident source (receiver) ray and the specular ray in Figure [*]. The specular ray is defined as the reflection raypath for which the incident angle $\Theta$ is equal to the angle of reflection, with respect to the normal to the reflecting surface. The specular angle $\Theta$ is related to $\phi_s$ and $\phi_r$ in that $\Theta = \vert\theta_s-\phi_s\vert = \vert\theta_r-\phi_r\vert$, where $\theta_s$ is the angle between an arbitrary source ray and the reflector normal, and $\theta_r$ is the angle between an arbitrary receiver ray and the reflector normal. Frazer and Sen (1985, eqn. 9b) derive an analogous expression to (1) for elastic Kirchhoff-Helmholtz surface integrals.

 
geom
geom
Figure 1
Ray geometry for generalized reflection and diffraction.
view

Equation (1) can be integrated over the subsurface volume to forward model the reflected scalar wavefield:

 
 \begin{displaymath}
U({\bf x}_r,{\bf x}_s,w) = \int_V A_s A_r R_{_{P\!P}}e^{iw\tau} dV \;,\end{displaymath} (2)

where ${\bf x}_s$ (${\bf x}_r$) is the shot (receiver) coordinate, and $\tau$ is the total traveltime from source to reflection point to receiver. As (Ar) is the WKBJ amplitude factor along the source (receiver) leg of the raypath to the subsurface reflection point ${\bf x}$, and incorporates the amplitude effects of source (receiver) directivity, geometric spreading, transmission loss, and intrinsic high-frequency Q attenuation. All of these quantities are readily available by raytracing through the background migration velocity model. The scalar U may be the wave pressure measured in a hydrophone, the magnitude of the displacement vector measured at a geophone, or an individual (e.g. vertical) component of the displacement vector if the appropriate component directivity is introduced into Ar.

It is important to note that the volume integration (2) models a single trace for any arbitrary source and receiver location. There is no ``preferred'' acquisition geometry for this synthesis; it works for shot gathers as well as random trace orientations. In particular, (2) is perfectly adequate for constant offset survey data, which will be the focus of this work.


previous up next print clean
Next: Inverse problem Up: THEORY Previous: THEORY
Stanford Exploration Project
11/17/1997