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The AAPG/Datapages Combined Publications Database
Houston Geological Society Bulletin
Abstract
Abstract: A Dynamic Model for the Permian Panhandle and
Hugoton Fields, Western Anadarko Basin
By
Anadarko Petroleum Corporation
Houston, Texas
Panhandle-Hugoton, the largest North American gas field, has
long been controversial because of extremely subnormal
pressures, variable gas composition and tilted fluid contacts,
commonly attributed to
hydrodynamic
flow
despite the absence of an effective updip
aquifer. These anomalies are explained in
terms of a basin-scale petroleum system history,
largely independent of the geographically
underlying the pre-Permian system.
Hydrocarbons were already being generated
in the deep Anadarko Basin during the Early
Permian, with efficient southward migration
from all potential source rocks via bounding
faults and Pennsylvanian-Permian alluvial fans. Giant Amarillo
Uplift drape structures trapped hydrocarbons immediately following
Permian evaporite deposition. The pre-Laramide
Panhandle Field, at maximum burial depth and
pressure
, contained
most of the oil and gas now found in mid-continent
Permian reservoirs.
The Early Tertiary Laramide Orogeny
redistributed Panhandle Field fluid
columns, possibly spilling gas into the
Hugoton embayment. Subsequent erosion
of Permian reservoir facies in eastern Kansas
allowed water discharge to outcrops at elevations
below the regional hydraulic head. As
regional
pressure
dropped in response, the
Panhandle Field gas cap expanded rapidly,
forcing a Late Tertiary-Quaternary mass movement of gas northward
to fill Hugoton and associated fields.
Panhandle-Hugoton pressures, upon discovery, were subnormal
relative to drilling depth but normal relative to reservoir outcrop
elevations in eastern Kansas, indicating that pressures are
controlled by aquifer communication with the surface rather
than burial depth. Variations in fluid contacts,
pressure
and gas
composition suggest that reservoir fluids are still moving, driven
by decompression and the rapid volumetric expansion of a
supergiant gas accumulation.
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