f-k spectra
Chapter 8 - Introduction to Petroleum Seismologyf-k spectrums considering different vertical cable samplings.
We have simulated the situation in which the vertical cable receiver spacing is 6.25 m, 12.50 m, 18.75 m, and 25 m. This figure shows the $f-k$ spectrum of some shot gathers for the different receiver spacing considered. We notice that aliasing occurs for a receiver spacing of 18.5 m and greater. As we can see, at 18.5-m and 25-m receiver spacing, some downgoing event aliases are shifted to negative wavenumbers at higher frequencies instead of staying in positive wavenumbers. The same problem happens for upgoing event aliases, which are shifted in positive wavenumbers instead of staying in negative wavenumbers at higher frequencies. So due to aliasing, it is now difficult to achieve a proper up/down separation. A trade-off has to be made between having a good up/down separation and keeping the whole signal spectrum. One possible way for improving the f-k dip filtering is to use an interpolation method, like the f-x interpolation, to create the data required to satisfy the sampling theorem.
Other Images in Chapter 8
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An example of the sailing path of a marine vessel in a towed-streamer survey
Images - Chapter 8
An example of the sailing path of a marine vessel in a towed-streamer survey. Note that the time for turning from one sailing line to another is about nine hours for vessels carrying streamers that are 10 km long. The dotted line indicates the turning legs of the sailing path.
This figure illustrates a typical sailing path of a 3D survey; the vessel travels back and forth, shooting and collecting data along many parallel lines, resulting in seismic data generated along lines 25 to 50 meters apart. Note that it takes about nine hours to turn from one sailing line to another for a vessel carrying 10-km-long streamers. Today, data are recorded even when the vessel is turning.
A shot diagram
Images - Chapter 7 A display of source and receiver distribution of a 2D seismic line in the so-called shot diagram. The rows corresponding to common-shot gathers and columns to common-receiver gathers. The diagonal is the zero-offset section, and all the other lines parallel to the diagonal are common-offset gathers (also known as common-offset sections). The lines perpendicular to the diagonal are the CMP gathers.
Another illustration of towed streamer acquisition
Images - Chapter 7 Another illustration of towed streamer acquisition
Interference noise
Images - Chapter 7 An illustration of interference noise in seismic data before and after. This figure shows the stack of seismic interference noise contaminated shots from another line in the Gulf of Mexico. Interference noise is clearly visible. Attenuation of seismic interference noise can be achieved by the use f-x prediction filters. Courtesy of Western Geco.
Other examples of structural traps
Images - Chapter 1 Structural traps. (A) Tilted fault blocks in an extensional regime. The seals are overlying mudstones and cross-fault juxtaposition against mudstones. (B) Rollover anticline on thrust. Petroleum accumulations may occur on both the hanging wall and the footwall. The hanging wall accumulation is dependent on a subthrust fault seal, whereas at least part of the hanging wall trap is likely to be a simple, four-way, dip-closed structure. (C) Lateral seal of a trap against a salt diapir and compactional drape trap over the diapir crest. (D) Diapiric mudstone associated trap with lateral seal against mud wall. Diapiric mud associated traps share many common features with that of salt. In this diagram, the diapiric mud wall developed at the core of a compressional fold. (E) Compactional drape over a basement block commonly creates enormous low-relief traps. (F) Gravity-generated trapping commonly occurs in deltaic sequences. Sediment loading causes gravity-driven failure and produces convex-down (listric) faults. The hanging wall of the fault rotates, creating space for sediment accumulation adjacent to the fault planes. The marker beds (grey) illustrate the form of the structure that has many favourable sites for petroleum accumulation. Adapted from Gluyas JG and Swarbrick RE (2003) Petroleum Geoscience. Oxford: Blackwell Science.
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