118#118 | (48) |
119#119 | (49) |
We propose to add a mask function defined as
120#120 | (50) |
When 122#122 has enough energy to contribute to the image, the damping factor 114#114 is set to zero. When factor 122#122 is small, the damping factor is kept to avoid zero division. Thus, the imaging condition can be set as
123#123 | (51) |
A simple synthetic was generated to test the preceding idea using wave equation modeling. Figure a shows the downgoing wave, and Figure b the upgoing wave, at a fixed time. Figure shows the mask 124#124 used in this example.
Figure a shows the reflection strength calculated using the imaging condition stated in equation (). Figure b shows the reflection strength calculated using division of the upgoing wavefield 106#106 by the downgoing wavefield 9#9. Figure c shows the reflection strength calculated using the imaging condition stated in equation (), and Figure d shows the reflection strength calculated using the imaging condition stated in equation (). The advantage of Figure d's result over the others is that it has the correct reflection strength value inside the masked area and doesn't diverge outside it because of the damping factor.
In Figure we compare the two imaging conditions stated in equations () and () inside the masked area for two different 114#114. We can see for the imaging condition stated in equation () that the reflection strength inside the masked area doesn't change. This is an important advantage of space variable damping imaging principle, because it let us to build an adaptive mask dependent of the subsurface illumination.
We stack the reflection strength from 11 shots to see how the change observed in one shot affects the final image. The result is shown in Figure . We can see imaging condition from equation () gives the best resolution.