Annual Report 2000 - WIT
Annual Report 2000 - WIT Annual Report 2000 - WIT
218 weight functions from traveltimes only. The actual expression and its derivation are given in Appendices B and D. For the example the only input data used were the velocity model and traveltimes computed with a finite-difference eikonal solver (Vidale, 1990) using the implementation of (Leidenfrost, 1998) and stored on a coarse grid of 50m in either direction. These were used to compute the migration weights as well as to interpolate the diffraction traveltimes on a fine migration grid of 5m in ¹ -direction. Traveltimes were interpolated using the hyperbolic approximation as described in (Vanelle and Gajewski, 2000a). The migration weights were also computed using the coefficients determined from the hyperbolic approximation. The velocity model we used has a plane reflector with an inclination angle of 14º . The velocity is 5km/s in the upper part of the model and 6km/s below the reflector. The reflector depth under the source is 2500m. Ray synthetic seismograms were computed for 80 receivers with 50m distance starting at 50m from the point source. Figure 1 shows the migrated depth section. The reflector was migrated to the correct position and the source pulse, a Gabor wavelet, was reconstructed. Since there are no transmission losses caused by the overburden, the amplitudes of the migrated section should coincide with the reflection coefficients. Figure 2 shows the accordance between amplitudes picked from the migrated section in Figure 1 with theoretical values. Apart from the peaks at 900m and 2500m distance the two curves coincide. These peaks are aperture effects caused by the limited extent of the receiver line. 1.5 Distance [km] 1 2 3 Depth [km] 2.0 2.5 Inclined reflector: migrated depth section Figure 1: Migrated depth section. The reflector was migrated to the correct depth and inclination. The source pulse was correctly reconstructed.
219 Reflection coefficient 0.2 0 Inclined reflector: reflection coefficients 1 2 3 Distance [km] Figure 2: Solid line: picked reflection coefficients from the migrated section in Figure 1, dashed line: analytical values for the reflection coefficients. CONCLUSIONS We have presented a method for the determination of weight functions for an amplitude preserving migration. Traveltimes on coarse grids are the only necessary input data. Since every required quantity can be computed instantly from this coarse grid data alone the technique is very efficient in computational time and storage. Dynamic ray tracing is not required. It is particularly suited to be used in connection with techniques for traveltime computation that can directly provide coarse gridded data, like, e.g. the wavefront construction method which does not require a fine grid for sufficient accuracy of traveltime as, e.g., FD eikonal solvers do. The examples show good accordance between the reconstructed reflectors and theoretical values in terms of position as well as in amplitudes. This demonstrates also the applicability of the method to the special situation of 2.5-D symmetry. ACKNOWLEDGEMENTS We thank the members of the Applied Geophysics Group in Hamburg for continuous and helpful discussions. Special thanks go to Andrée Leidenfrost for providing an FD eikonal solver and thus the necessary input traveltimes. This work was partially supported by the German Research Society (DFG, Ga 350-10) and the sponsors of the Wave Inversion Technology (WIT) consortium.
- Page 180 and 181: ø M ã = ã Ù ø ä Ú ã Ù ø
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- Page 194 and 195: 182 REFERENCES Bourbié, T., Coussy
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- Page 210 and 211: 198 Time (ms) 0 2 4 6 8 10 12 14 16
- Page 212 and 213: 200 of groundwater. ACKNOWLEDGEMENT
- Page 214 and 215: 202
- Page 216 and 217: 204 the wavefront curvature matrix
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- Page 222 and 223: 210 Table 2: Median relative errors
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- Page 226 and 227: 214 PUBLICATIONS Previous results c
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- Page 232 and 233: 220 REFERENCES Bleistein, N., 1986,
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- Page 260 and 261: 248 Ettrich, N., 1998, FD eikonal s
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218<br />
weight functions from traveltimes only. The actual expression and its derivation are<br />
given in Appendices B and D.<br />
For the example the only input data used were the velocity model and traveltimes computed<br />
with a finite-difference eikonal solver (Vidale, 1990) using the implementation<br />
of (Leidenfrost, 1998) and stored on a coarse grid of 50m in either direction. These<br />
were used to compute the migration weights as well as to interpolate the diffraction<br />
traveltimes on a fine migration grid of 5m in ¹ -direction. Traveltimes were interpolated<br />
using the hyperbolic approximation as described in (Vanelle and Gajewski,<br />
<strong>2000</strong>a). The migration weights were also computed using the coefficients determined<br />
from the hyperbolic approximation.<br />
The velocity model we used has a plane reflector with an inclination angle of 14º . The<br />
velocity is 5km/s in the upper part of the model and 6km/s below the reflector. The<br />
reflector depth under the source is 2500m. Ray synthetic seismograms were computed<br />
for 80 receivers with 50m distance starting at 50m from the point source. Figure 1<br />
shows the migrated depth section. The reflector was migrated to the correct position<br />
and the source pulse, a Gabor wavelet, was reconstructed. Since there are no transmission<br />
losses caused by the overburden, the amplitudes of the migrated section should<br />
coincide with the reflection coefficients. Figure 2 shows the accordance between amplitudes<br />
picked from the migrated section in Figure 1 with theoretical values. Apart<br />
from the peaks at 900m and 2500m distance the two curves coincide. These peaks are<br />
aperture effects caused by the limited extent of the receiver line.<br />
1.5<br />
Distance [km]<br />
1 2 3<br />
Depth [km]<br />
2.0<br />
2.5<br />
Inclined reflector: migrated depth section<br />
Figure 1: Migrated depth section. The reflector was migrated to the correct depth and<br />
inclination. The source pulse was correctly reconstructed.