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In the case of zero-offset reflection, the ray travel distance,
l, from the source to the reflection point is related to the
two-way zero-offset time, t, by the simple equation
where vg is the half of the group velocity, best expressed in
terms of its components, as follows:
![\begin{displaymath}
v_g = \sqrt{v_{gx}^2 + v_v^2 v_{g\tau}^2}.\end{displaymath}](img8.gif)
Here vgx denotes the horizontal component of group velocity,
vv is the vertical P-wave velocity, and
is the
vv-normalized vertical component of the group velocity. Under the
assumption of zero shear-wave velocity in VTI media, these components
have the following analytic expressions:
| ![\begin{displaymath}
v_{gx} =
{\frac{{v^2}\,{p_x}\,\left( -1 - 2\,\eta + 2\,\eta ...
...left( 1 + 2\,\eta \right) \,{{{p_x}}^2} +
{{{p_{\tau }}}^2}}},\end{displaymath}](img10.gif) |
(4) |
and
| ![\begin{displaymath}
v_{g\tau} = {\frac{\left(1- 2\,{v^2}\,\eta \,{{{p_x}}^2} \ri...
...eft( 1 + 2\,\eta \right) \,
{{{p_x}}^2} + {{{p_{\tau }}}^2}}},\end{displaymath}](img11.gif) |
(5) |
where px is the horizontal component of slowness, and
is the normalized (again by the vertical P-wave velocity vv)
vertical component of slowness. The two components of the slowness
vector are related by the following eikonal-type equation
Alkhalifah (1997):
| ![\begin{displaymath}
p_{\tau} = \sqrt{1 - {\frac{{v^2}\,{{{p_x}}^2}}
{1 - 2\,{v^2}\,\eta \,{{{p_x}}^2}}}}.\end{displaymath}](img13.gif) |
(6) |
Equation (6) corresponds to a normalized version of the
dispersion relation in VTI media.
If we consider v and
as imaging parameters (migration
velocity and migration anisotropy coefficient), the ray length l can
be taken as an imaging invariant. This implies that the partial
derivatives of l with respect to the imaging parameters are zero.
Therefore,
| ![\begin{displaymath}
\frac{\partial l}{\partial v} = \frac{\partial
v_{g}}{\partial v} t+ v_{g} \frac{\partial t}{\partial v} = 0,\end{displaymath}](img14.gif) |
(7) |
and
| ![\begin{displaymath}
\frac{\partial l}{\partial \eta} = \frac{\partial v_{g}}{\partial \eta} t+
v_{g} \frac{\partial t}{\partial \eta} = 0.\end{displaymath}](img15.gif) |
(8) |
Applying the simple chain rule to equations (7) and
(8), we obtain
| ![\begin{displaymath}
\frac{\partial t}{\partial v} = \frac{\partial t}{\partial \...
...partial t}
{\partial \tau} \frac{\partial \tau}{\partial \eta},\end{displaymath}](img16.gif) |
(9) |
where
, and the two-way vertical traveltime is
given by
![\begin{displaymath}
\tau = v_{g\tau} t.\end{displaymath}](img18.gif)
Combining equations (7-9) eliminates the two-way
zero-offset time t, which leads to the equations
| ![\begin{displaymath}
\frac{\partial
\tau}{\partial v} = \frac{\partial v_{g}}{\partial v} {\frac{\tau }
{{p_{\tau }}\,{v_{g\tau }}{v_{g}}}}, \end{displaymath}](img19.gif) |
(10) |
and
| ![\begin{displaymath}
\frac{\partial
\tau}{\partial \eta} = \frac{\partial v_{g}}...
...rtial \eta}
{\frac{\tau } {{p_{\tau }}\,{v_{g\tau }}{v_{g}}}}. \end{displaymath}](img20.gif) |
(11) |
After some tedious algebraic manipulation, we can transform
equations (5) and (6) to the general form
| ![\begin{displaymath}
\frac{\partial \tau}{\partial v} = \tau F_v\left(p_x,v,\eta \right),\end{displaymath}](img21.gif) |
(12) |
and
| ![\begin{displaymath}
\frac{\partial \tau}{\partial \eta} = \tau F_{\eta}\left(p_x,v,\eta \right).\end{displaymath}](img22.gif) |
(13) |
Since the residual migration is applied to migrated data, with the
time axis given by
and the reflection slope given by
, instead of t and px,
respectively, we need to eliminate px from
equations (12) and (13). This task can be
achieved with the help of the following explicit relation, derived
in Appendix A,
| ![\begin{displaymath}
p_x^2 = {\frac{2\,{{{{\tau }_x}}^2}}
{1 + {v^2}\,\left( 1 + 2\,\eta \right) \,
{{{{\tau }_x}}^2} +
{S}}},\end{displaymath}](img25.gif) |
(14) |
where
=
, and
![\begin{displaymath}
S = \sqrt{-8\,{v^2}\,\eta \,{{{{\tau }_x}}^2} +
{{\left( 1 ...
...\,\left( 1 + 2\,\eta \right) \,{{{{\tau }_x}}^2} \right) }^2}}.\end{displaymath}](img27.gif)
Inserting equation (14) into equations (12)
and (13) yields exact, yet complicated equations,
describing the continuation process for v and
. In
summary, these equations have the form
| ![\begin{displaymath}
\frac{\partial
\tau}{\partial v} = \tau f_v\left(\frac{\partial
\tau}{\partial x},v,\eta \right)\end{displaymath}](img28.gif) |
(15) |
and
| ![\begin{displaymath}
\frac{\partial \tau}{\partial \eta} = \tau f_{\eta}\left(\frac{\partial \tau}{\partial x},v,\eta \right).\end{displaymath}](img29.gif) |
(16) |
Equations of the form (15) and (16) contain all
the necessary information about the kinematic laws of anisotropy
continuation in the domain of zero-offset migration.
Next: Linearization
Up: Alkhalifah and Fomel: Anisotropy
Previous: Introduction
Stanford Exploration Project
11/11/1997