About This Item
- Full text of this item is not available.
- Abstract PDFAbstract PDF(no subscription required)
Share This Item
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
extreme 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 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.
End_of_Record - Last_Page 53---------------