Annual Report 2000 - WIT
Annual Report 2000 - WIT Annual Report 2000 - WIT
æVU ìÿå T ü ýWYXZX[ 9\]9^\ Þ _ Ý Ý Ý Ý Ý Ý Ý ì §Cb æ \] ê \ Ý Ý Ý 216 1997) points out that computing traveltime derivatives along dipping surfaces is expensive and numerically unstable. In this paper we propose an alternative algorithm for determining traveltime derivatives that does not suffer from the instability of numerical differentiation. It is based on a local spherical approximation of the wavefront leading to a hyperbolic expansion of the traveltimes. We determine the complete weight functions from traveltimes sampled on a coarse grid that are at the same time used for the computation of the diffraction time surface needed for the stack. This makes the algorithm computationally efficient in time and particularly in storage. Dynamic ray tracing is not required. For the special case of 2.5-D symmetry we use a simple expression for the out-of-plane spreading that can also be determined from traveltimes and not, as it is usually done, from an integral along the raypath. Following an outline of true amplitude migration using a weighted diffraction stack we will give an expression for the actual form of migration weight functions as they were employed in this work. We will then demonstrate our method by applying it to two examples. Comparison of our results to analytical values will confirm its quality which we also summarize in our conclusions. METHOD (Schleicher et al., 1993) show that a diffraction stack of the form êc ì © dVeCfhgi ©©©© gVj kml (1) ëa æ \] ê \ êOU Ý`_ yields a true amplitude migrated trace if proper weight functions ëaöæ \] ê \ êOU ì are _ applied. In equation n (1) is the aperture of the experiment (assumed to provide sufficient illumination), §Cb æ \] ê \ § c êNc ì @ § c & d¤eofpgi g¤j kml is the time derivative of the input seismic trace in terms of the trace coordinates æ \] ê \ Ý ì at the diffraction traveltime òq for a diffractor at a subsurface point U . b æ \] ê \ b æ \] ê \ êNc ì is given by (2) êNc ìåsr!t ì ì u v æwc Þâòx æ \] ê \ In equation (2) v æwc ì is the shape of the analytic source pulse, ò¨x the reflection traveltime and the geometrical spreading. r is the plane wave reflection coefficient and t expresses transmission losses. The integral (1) cannot generally be analytically solved. It can, however be transformed to the frequency domain and for high frequencies be u approximately evaluated by the stationary phase method. This solution is then transformed back to the time domain and compared to the analytic true amplitude signal [ æ{c ìå u b æ \] ê \ êNcô bzy æ \] ê \ ì ìöå r!t v æ{c ì ò¨x The comparison of [ æwc ì and the result of (1) shows that equation (1) yields indeed bzy a true amplitude trace if the weight functions are chosen to be (Schleicher et al., 1993) (3) Pƒ‚…„{†¦‡Gˆ j " (4) ¥j ] ëa æ \] ê \ êOU ìöå u > & |~}/!€ & |
\]O‘N\¨’¨‘ U”“–•˜— ¨šA› œƒž9ŸšA› œz aZ ¡ ¢ ž ¢¢ ° ¢¢¢ |Ÿ}±¦ § ] £ |~}'¦ § ’ £ Ý ¢¢¢ ¢¢¢ ‹ 217 The matrix is the Hessian matrix of the difference ò € å !€ ê \A‰ ] ÞVòx between diffrac- ò¨q € å Œ , meaning ò tion and reflection traveltime at the stationary point , where Š that in this point the diffraction and reflection traveltime curves are tangent to each other. \A‰ can be expressed in terms of second order spatial derivative matrices of !€ traveltimes which until now were computed by dynamic ray tracing. This is, however, not necessary since these derivatives can be extracted from traveltime data that is required for the construction of the diffraction traveltime surface for the stack anyway. Using these derivatives also gives an effective and highly accurate algorithm for interpolating traveltimes from the coarse input grid to the fine migration grid (Vanelle and Gajewski, 2000a). Also, the geometrical spreading can be written using second order derivatives of traveltimes (see Appendix C). The expression for the weight function we use is |Ÿ}¥¤ƒ¦ §$¨ ]ª©¬« ¦ §”¨ ’®1¯ £ (5) |¥²#³ j fp´i¤µ´Ÿj l _ Ž The angles œz and are the emergence and incidence angles at the source and receiver, is the velocity at the source ¸ ] œ·ž ž and ¸ ’ and are the KMAH indices of the two branches of the traveltime curve. The ¡ matrices and describe the measurement § ’ are second order derivative matrices of © configuration (e.g., common shot). ¦ the traveltimes. All quantities and their determination from traveltimes are explained in detail in the appendices. § ] and ¦ APPLICATIONS In this section we will apply our method. A simple example was chosen in order to allow for comparison of numerically and analytically computed amplitudes. The method is, however, not limited to homogeneous velocity layer models. For convenience reasons we have restricted our example to what is commonly referred to as a 2.5-D geometry (Bleistein, 1986). The need to introduce this concept arises when seismic data is only available for sources and receivers constrained to a single straight acquisiton line. Processing of this data with techniques based on 2-D wave propagation does not yield satisfactory results because the (spherical) geometrical spreading in the data caused by the 3-D earth does not agree with the cylindrical (i.e., line source) spreading implied by the 2-D wave equation. The problem can be dealt with by assuming the subsurface to be invariant in the off-line direction. This symmetry is called to be 2.5 dimensional. Apart from the geometrical spreading the properties involved do not depend on the outof-plane variable and can be computed with 2-D techniques. The geometrical spreading is split into an in-plane part that is equal to the 2-D spreading and an out-of-plane contribution. For the described symmetry the product of both equals the spreading in a true 3-D medium. We determine the out-of-plane spreading along with the migration
- Page 178 and 179: Ý ì á ä é å¤æDçzè ä é
- Page 180 and 181: ø M ã = ã Ù ø ä Ú ã Ù ø
- Page 182 and 183: ã Q c ã ä 170 a=10m; std.dev.=8%
- Page 184 and 185: 172 Frankel, A., and Clayton, R. W.
- Page 186 and 187: 174 It is well-known that inhomogen
- Page 188 and 189: ã ä ä ŸSŸ S ¡S¡ ©©¨¨ æ
- Page 190 and 191: Kneib, 1995 285-6000 superposition
- Page 192 and 193: 180 parameter: Hurst coefficient pa
- Page 194 and 195: 182 REFERENCES Bourbié, T., Coussy
- Page 196 and 197: 184 1999) in multiple fractured med
- Page 198 and 199: ‹œž Ÿ¢¡¤£¦¥ƒ§©¨ ‘
- Page 200 and 201: j jÆÅÇ[È”u j jÎÅÇ[È”uw
- Page 202 and 203: 190 Davis, P. M., and Knopoff, L.,
- Page 204 and 205: 192 properties from the measured se
- Page 206 and 207: 194 discussion of these problems ca
- Page 208 and 209: 196 Altogether, close to 260 shotpo
- 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
- Page 218 and 219: û ò é from ã äñ to ã î§ñ
- Page 220 and 221: é 208 Table 1: Median relative err
- Page 222 and 223: 210 Table 2: Median relative errors
- Page 224 and 225: 212 CONCLUSIONS We have presented a
- Page 226 and 227: 214 PUBLICATIONS Previous results c
- Page 230 and 231: 218 weight functions from traveltim
- Page 232 and 233: 220 REFERENCES Bleistein, N., 1986,
- Page 234 and 235: Š Ê ¦ Í ½ Í ’ » Ö ½ Ê
- Page 236 and 237: !¥”“Z• Ç ¤ ɨ§ — ‘
- Page 238 and 239: 226
- Page 240 and 241: 228 In this paper, we present a mor
- Page 242 and 243: L • MM+,ON N N Ž ú R N N N ú
- Page 244 and 245: 232 Figure 3: The evolution of a WF
- Page 246 and 247: 234 Let us analyze next the computa
- Page 248 and 249: 236 CONCLUSIONS We have presented a
- Page 250 and 251: 238
- Page 252 and 253: ’ Ç r 240 traveltimes, a computa
- Page 254 and 255: Ž Ž Ã Ž 242 Other two approxima
- Page 256 and 257: “ Ã Æ ³ 244 0 0.5 [km] 0 0.5 1
- Page 258 and 259: î r † Û(Û Ü Œ U Ú Ý Ü Û
- Page 260 and 261: 248 Ettrich, N., 1998, FD eikonal s
- Page 262 and 263: ø Ð ¡ Ð÷ö Ð'ø ú Ð ¡ Ð'
- Page 264 and 265: ø ü ø ø ý Þ do ø ý Ü
- Page 266 and 267: ø ö ø ú ü ö ü ¡ ü
- Page 268 and 269: ‹ 256 transport equation. Neverth
- Page 270 and 271: 258 tivalued geometrical spreading
- Page 272 and 273: 260 .
- Page 274 and 275: 262
- Page 276 and 277: … " ¯ ü ý +- 4=° ü ü +
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Þ<br />
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Ý<br />
Ý<br />
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216<br />
1997) points out that computing traveltime derivatives along dipping surfaces is expensive<br />
and numerically unstable. In this paper we propose an alternative algorithm for<br />
determining traveltime derivatives that does not suffer from the instability of numerical<br />
differentiation. It is based on a local spherical approximation of the wavefront leading<br />
to a hyperbolic expansion of the traveltimes. We determine the complete weight<br />
functions from traveltimes sampled on a coarse grid that are at the same time used<br />
for the computation of the diffraction time surface needed for the stack. This makes<br />
the algorithm computationally efficient in time and particularly in storage. Dynamic<br />
ray tracing is not required. For the special case of 2.5-D symmetry we use a simple<br />
expression for the out-of-plane spreading that can also be determined from traveltimes<br />
and not, as it is usually done, from an integral along the raypath.<br />
Following an outline of true amplitude migration using a weighted diffraction stack<br />
we will give an expression for the actual form of migration weight functions as they<br />
were employed in this work. We will then demonstrate our method by applying it to<br />
two examples. Comparison of our results to analytical values will confirm its quality<br />
which we also summarize in our conclusions.<br />
METHOD<br />
(Schleicher et al., 1993) show that a diffraction stack of the form<br />
êc ì<br />
© dVeCfhgi ©©©©<br />
gVj kml <br />
(1)<br />
ëa æ \] ê \<br />
êOU<br />
Ý`_<br />
yields a true amplitude migrated trace if proper weight functions ëaöæ \] ê \ êOU ì<br />
are<br />
_<br />
applied. In equation n (1) is the aperture of the experiment (assumed to provide sufficient<br />
illumination), §Cb æ \] ê \<br />
§ c<br />
êNc ì @ § c & d¤eofpgi g¤j kml is the time derivative of the input seismic<br />
trace in terms of the trace coordinates æ \] ê \ Ý<br />
ì<br />
at the diffraction traveltime òq for a<br />
diffractor at a subsurface point U . b æ \] ê \<br />
b æ \] ê \<br />
êNc ì<br />
is given by<br />
(2)<br />
êNc ìåsr!t<br />
ì ì<br />
u v æwc Þâòx æ \] ê \<br />
In equation (2) v æwc ì<br />
is the shape of the analytic source pulse, ò¨x the reflection traveltime<br />
and the geometrical spreading. r is the plane wave reflection coefficient and t<br />
expresses transmission losses. The integral (1) cannot generally be analytically solved.<br />
It can, however be transformed to the frequency domain and for high frequencies be<br />
u<br />
approximately evaluated by the stationary phase method. This solution is then transformed<br />
back to the time domain and compared to the analytic true amplitude signal<br />
[ æ{c ìå u b æ \] ê \ êNcô bzy æ \] ê \ ì ìöå<br />
r!t v æ{c ì<br />
ò¨x<br />
The comparison of<br />
[ æwc ì<br />
and the result of (1) shows that equation (1) yields indeed<br />
bzy<br />
a true amplitude trace if the weight functions are chosen to be (Schleicher et al., 1993)<br />
(3)<br />
Pƒ‚…„{†¦‡Gˆ<br />
j "<br />
(4)<br />
¥j ]<br />
ëa æ \] ê \<br />
êOU ìöå u > & |~}/!€ & |