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Reflector mapping imaging condition and image artifacts

Claerbout (1971) expresses the reflector mapping imaging condition as follows:  
 \begin{displaymath}
{\bf r}(x,z)=\frac{ {\bf u}(x,z,t_{d})}{ {\bf d}(x,z,t_{d})},\end{displaymath} (1)
where x is the horizontal coordinate, z is the depth, and td is the time at which the source wavefield ${\bf d}(x,z,t_{d})$ and the receiver wavefield ${\bf u}(x,z,t_{d})$ coincide in time and space. This principle states that the reflectivity strength ${\bf r}(x,z)$ depends only on the source wavefield and on the receiver wavefield at time td.

A practical way to compute the reflectivity strength is discussed in Claerbout's paper Claerbout (1971). The reflectivity strength is computed as:  
 \begin{displaymath}
{\bf r}(x,z)= ({\bf u} \star {\bf d})(x,z,\tau =0),\end{displaymath} (2)
where means cross-correlation and $\tau$ is the lag. This is commonly used in the industry. It has the advantage of being robust, but has the disadvantage of not computing the correct amplitudes Claerbout (1971).

A more general imaging condition can be stated, computing the reflectivity strength as:  
 \begin{displaymath}
{\bf r}(x,z)=\frac{ {\bf u}}{ {\bf d}}(x,z,\tau =0),\end{displaymath} (3)
where the division means deconvolution in time of the receiver wavefield by the source wavefield for each (x,z) and $\tau$ is the lag. It has the potential of accounting for wavefield multipathing during imaging, thus avoiding the creation of image artifacts in the presence of velocity anomalies.

Figures [*] to [*] show the comparison of wavefield deconvolution with wavefield cross-correlation imaging condition. The first row, in Figure [*], simulates the two wavefields coinciding at the reflector depth. The result of the cross-correlation and the result of the deconvolution is shown in the second row. For each case, the zero lag of the wavefield cross-correlation or the zero lag of the wavefield deconvolution is assigned as the reflectivity strength at this depth.

 
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Figure 1
Wavefields coinciding at the reflector depth. (a) Source wavefield. (b) Receiver wavefield. (c) Wavefields cross-correlation. (d) Wavefields deconvolution.
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The first row in Figure [*] / [*] simulates the two wavefields at a deeper / shallower depth than the reflector depth. The second row shows the result of the cross-correlation and the result of the deconvolution. The zero lag value of the wavefield cross-correlation has a value different than zero, thus creates an image artifact at a deeper / shallower depth. In the case of deconvolution imaging condition, the zero lag value is zero, thus no image artifacts are created.

 
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Figure 2
Wavefields at a depth deeper the reflector depth. (a) Source wavefield. (b) Receiver wavefield. (c) Wavefields cross-correlation. (d) Wavefields deconvolution.
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Figure 3
Wavefields at a depth shallower the reflector depth. (a) Source wavefield. (b) Receiver wavefield. (c) Wavefields cross-correlation. (d) Wavefields deconvolution.
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The imaging condition stated in equation (3) makes the strong assumption that the receiver wavefield ${\bf u}(x,z,t)$ can be computed by convolving the source wavefield ${\bf d}(x,z,t)$ by the reflectivity strength ${\bf r}(x,z)$. As we will discuss later, this is true at the reflector depth, but might not be true at a different depth.


next up previous print clean
Next: Deconvolution in the time Up: Valenciano and Biondi: Deconvolution Previous: Introduction
Stanford Exploration Project
11/11/2002