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Abstract

AAPG Bulletin, V. 83 (1999), No. 3 (March 1999), P. 410-432.

Polygonal Faults and Their Influence on Deep-Water Sandstone Reservoir Geometries, Alba Previous HitFieldNext Hit, United Kingdom Central Previous HitNorthNext Hit Previous HitSeaNext Hit1

Lidia Lonergan and Joe A. Cartwright2
 

©Copyright 1999.  The American Association of Petroleum Geologists.  All Rights Reserved
 

1Manuscript received January 27, 1997; revised manuscript received July 2, 1998; final acceptance September 22, 1998.
2T. H. Huxley School of Environment, Earth Science and Engineering, Imperial College of Science Technology and Medicine, Prince Consort Road, London SW7 2BP, United Kingdom; e-mail: [email protected]
 

We thank P. Anderton, R. Jolly, P. Mason, S. Reiter, P. Sansom, J. Staffurth, E. Thompson, T. Whitbread, and J. Wonham for help. Special thanks to R. Laver for originally drawing our attention to the zigzag edges on Alba. The financial support of Fina Exploration (Cartwright and Lonergan) and the Royal Society (Lonergan) is gratefully acknowledged. Schlumberger Geoquest provided generous assistance with seismic interpretation software and technical support, and financed color figures. Chevron UK and partners in Block 16/26 are thanked for allowing us to publish seismic data from the Alba three-dimensional data set. H. D. Johnson, S. Laubach, B. Trudgill, and P. Yilmaz, and especially Editor N. Hurley, are thanked for constructive reviews that led to substantial improvements in versions of this paper.
 

ABSTRACT

Polygonal faults attributed to three-dimensional (3-D) volumetric contraction of muddy sediments during early burial are widespread within the Eocene-lower Miocene succession of the United Kingdom central Previous HitNorthNext Hit Previous HitSeaNext Hit. The analysis of a 3-D seismic survey encompassing the Eocene Alba Previous HitfieldNext Hit in the central Previous HitNorthNext Hit Previous HitSeaNext Hit has allowed us to investigate (1) the influence of polygonal faults in surrounding mudrocks on the geometry of the Alba deep-water sandstone reservoir and (2) how the presence of the reservoir sandstone influences the polygonal fault pattern above and below the reservoir.

The main reservoir in the Alba Previous HitfieldNext Hit is an elongate (12 km long, 1-2 km wide, up to 90 m thick), fine-grained, massive sandstone body that may have been deposited in a deep-water channel or slope gully. Although depositional processes likely have been responsible for the dominantly linear sandstone distribution, the current reservoir geometry is largely controlled by the location of polygonal faults in the surrounding hemipelagic mudstones. Sandstones interpreted as injected along faulted margins of the Alba Previous HitfieldNext Hit indicate that faulting facilitated remobilization and sand injection during early burial, further modifying the reservoir shape. Unusual, isolated 1-km-wide subcircular mounds to the west of the main Previous HitfieldNext Hit also are attributed to sand withdrawal and remobilization during early burial.

On a mapped marker horizon in the mudrocks 80-120 m above the reservoir there is a marked decrease in polygonal fault density compared to areas away from the reservoir. On a horizon in mudrocks within 5-50 m of the base of the reservoir there is an increase in horizon disruption due to small faults directly below the sand body. Changes in polygonal fault density and pattern thus may indicate the presence of sandstones and may be a useful exploration tool for explorationists searching for subtle Eocene deep-water sand bodies that typically are poorly imaged on seismic data in the Previous HitNorthNext Hit Previous HitSeaTop

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