Skip to Main Content
Book Chapter

Reservoir Architecture in the Mars Field, Deepwater Gulf of Mexico, USA: The Implications of Production, Seismic, Core and Well-Log Data

By
Tony Reynolds
Tony Reynolds
BP Amoco 501 Westlake Park Boulevard Houston, Texas 77079 reynoltd@bp.com
Search for other works by this author on:
Published:
December 01, 2000

Abstract

The Mars Field was discovered in 1989 in 2,900 ft of water 56 miles south-southeast of the mouth of the Mississippi River. Production commenced in 1996 and since that time the field has produced via natural depletion over 100 million barrels. Today (December, 1999) the field produces from 16 wells completed in ten reservoir intervals at a rate of around 180,000 barrels of oil equivalent a day. All the reservoir sands have been deposited in deep water, in an intraslope basin. The need to understand pressure data collected during production and the requirement to predict two-phase flow and evaluation of a waterflood scheme has prompted review of the architecture of major reservoir intervals. The largest of these reservoirs, the 100m thick Yellow interval, is discussed here.

Appraisal mapping revealed two key geometries: (i) a sheet sand, the Lower Yellow, which was described in two parts, a lower “amalgamated sheet” and an upper “layered sheet” and (ii) an overlying channel complex, the Upper Yellow. Although initially in pressure equilibrium, it was thought that an intervening shale would compartmentalise these intervals into two distinct reservoirs during production.

The present study has refined the appraisal view to reveal eight first order architectural elements, AE1 to AE8, defined and mapped on seismic data. These architectural elements have been divided into second order, sub-seismic elements using wireline log and core data, and characterised in terms of facies proportions, facies successions, reservoir properties, and likely inter-well architecture.

Key findings are that (i) small areas of contact between first order architectural elements have allowed significant pressure communication throughout the Yellow Reservoir; (ii) pressure data do not indicate low vertical permeability in interbedded sand and shale successions previously described as a layered sheet, and an alternative inter-well view of a low net-to-gross channelised sheet is suggested; (iii) aquifer influx has not been observed, suggesting that the original field-wide OWC is perched and that the true OWC is deeper; and (iv) the bulk of the reservoir drive energy is due to time varying compaction.

You do not currently have access to this article.

Figures & Tables

Contents

GCSSEPM

Deep-Water Reservoirs of the World

Paul Weimer
Paul Weimer
Houston, Texas
Search for other works by this author on:
SEPM Society for Sedimentary Geology
Volume
20
ISBN electronic:
978-0-9836097-0-4
Publication date:
December 01, 2000

GeoRef

References

Related

Citing Books via

A comprehensive resource of eBooks for researchers in the Earth Sciences

Close Modal
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close Modal
Close Modal