Cristin-resultat-ID: 1137465
Sist endret: 31. oktober 2014, 15:29
NVI-rapporteringsår: 2014
Resultat
Vitenskapelig artikkel
2014

From mechanical modeling to seismic imaging of faults: A synthetic workflow to study the impact of faults on seismic

Bidragsytere:
  • Charlotte Botter
  • Nestor Cardozo
  • Stuart Hardy
  • Isabelle Lecomte og
  • Alejandro Escalona

Tidsskrift

Marine and Petroleum Geology
ISSN 0264-8172
e-ISSN 1873-4073
NVI-nivå 1

Om resultatet

Vitenskapelig artikkel
Publiseringsår: 2014
Publisert online: 2014
Trykket: 2014
Volum: 57
Sider: 187 - 207

Importkilder

Scopus-ID: 2-s2.0-84902589522

Beskrivelse Beskrivelse

Tittel

From mechanical modeling to seismic imaging of faults: A synthetic workflow to study the impact of faults on seismic

Sammendrag

Although typically interpreted as 2D surfaces, faults are 3D narrow zones of highly and heterogeneously strained rocks, with petrophysical properties differing from the host rock. Here we present a synthetic workflow to evaluate the potential of seismic data for imaging fault structure and properties. The workflow consists of discrete element modeling (DEM) of faulting, empirical relations to modify initial acoustic properties based on volumetric strain, and a ray-based algorithm simulating prestack depth migration (PSDM). We illustrate the application of the workflow in 2D to a 100 m displacement normal fault in a kilometer size sandstone-shale sequence at 1.5 km depth. To explore the effect of particle size on fault evolution, we ran two DEM simulations with particle assemblages of similar bulk mechanical behavior but different particle size, one with coarse (1-3 m particle radii) and the other with fine (0.5-1.5 m particle radii) particles. Both simulations produce realistic but different fault geometries and strain fields, with the finer particle size model displaying narrower fault zones and fault linkage at later stages. Seismic images of these models are highly influenced by illumination direction and wave frequency. Specular illumination highlights flat reflectors outside the fault zone, but fault related diffractions are still observable. Footwall directed illumination produces low amplitude images. Hanging wall directed illumination images the shale layers within the main fault segment and the lateral extent of fault related deformation. Resolution and the accuracy of the reflectors are proportional to wave frequency. Wave frequencies of 20 Hz or more are necessary to image the different fault structure of the coarse and fine models. At 30-40 Hz, there is a direct correlation between seismic amplitude variations and the input acoustic properties after faulting. At these high frequencies, seismic amplitude variations predict both the extent of faulting and the changes in rock properties in the fault zone.

Bidragsytere

Charlotte Delphine Botter

Bidragsyterens navn vises på dette resultatet som Charlotte Botter
  • Tilknyttet:
    Forfatter
    ved Institutt for energi- og petroleumsteknologi ved Universitetet i Stavanger

Nestor Fernando Cardozo Diaz

Bidragsyterens navn vises på dette resultatet som Nestor Cardozo
  • Tilknyttet:
    Forfatter
    ved Institutt for energi- og petroleumsteknologi ved Universitetet i Stavanger

Stuart Hardy

  • Tilknyttet:
    Forfatter
    ved Institució Catalana de Recerca i Estudis Avançats
Aktiv cristin-person

Isabelle Christine Lecomte

Bidragsyterens navn vises på dette resultatet som Isabelle Lecomte
  • Tilknyttet:
    Forfatter
    ved NORSAR

Alejandro Escalona Varela

Bidragsyterens navn vises på dette resultatet som Alejandro Escalona
  • Tilknyttet:
    Forfatter
    ved Institutt for energi- og petroleumsteknologi ved Universitetet i Stavanger
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