--> Reduction in Bin Size of Seismic Data for Sharper Definition of Geologic Features
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AAPG Annual Convention and Exhibition

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Reduction in Bin Size of Previous HitSeismicNext Hit Previous HitDataNext Hit for Sharper Definition of Geologic Features

Abstract

Ideally, Previous HitseismicNext Hit Previous HitdataNext Hit should be acquired at high spatial and temporal sampling, so that the small subsurface features of interest can be clearly seen on the Previous HitseismicNext Hit Previous HitdisplayNext Hit. Such interpretation is easiest when the geological features of interest are uniformly illuminated, which in turn is possible by recording the scattered Previous HitseismicNext Hit wavefield on a uniform surface grid. The “nominal grid” is defined by the source-to-source spacing within a shot line and the geophone-group-to-geophone-group spacing within a receiver line. One can also increase the trace density by reducing the spacing between shot lines and between receiver lines. Once acquired, Previous HitdataNext Hit processing workflows are designed to retain the highest possible lateral and vertical resolution of the geologic target. Because of the different ray paths, dense acquisition (closer source and receiver lines) provides greater leverage against backscattered ground roll and decreased migration artifacts. Uniform acquisition results in increased lateral continuity of amplitudes that otherwise may be contaminated by acquisition footprint. While there is no substitute for acquiring good quality Previous HitseismicNext Hit Previous HitdataNext Hit that has the above mentioned qualities, it is possible to mimic or address some of the problems that crop up due to the sub-optimum parameterization used in the acquisition, during processing of the Previous HitdataNext Hit. It is possible to regularize the offsets and azimuths of the input Previous HitseismicNext Hit Previous HitdataNext Hit during processing by way of 5D interpolation, which then aids the computation of Previous HitseismicNext Hit attributes. In this presentation we demonstrate the results of reducing the bin size of the Previous HitseismicNext Hit Previous HitdataNext Hit as part of the 5D interpolation process. A comparison of the Previous HitseismicNext Hit amplitude Previous HitdataNext Hit before and after bin size reduction exhibits clearer Previous HitseismicNext Hit signatures corresponding to the features of interest that can be seen on the coherence or curvature horizon slices. One can notice the enhanced resolution of the faults and the suppression of the acquisition footprint. Stratigraphic features such as a distributary channel system seen on the coherence slices may be well imaged at the nominal grid size but the interpolated surface Previous HitdataNext Hit at reduced bin size provides much sharper individual channel limbs. Such enhanced quality imaging of Previous HitdataNext Hit in terms of suitable Previous HitseismicNext Hit attributes helps squeeze out more information from the Previous HitseismicNext Hit Previous HitdataNext Hit and contribute in a generous way to the overall interpretation of the Previous HitdataTop as well.